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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-21-8845-2021</article-id><title-group><article-title>Harnessing stratospheric diffusion barriers for enhanced climate
geoengineering</article-title><alt-title>Harnessing stratospheric diffusion barriers for enhanced climate geoengineering</alt-title>
      </title-group><?xmltex \runningtitle{Harnessing stratospheric diffusion barriers for enhanced climate geoengineering}?><?xmltex \runningauthor{N.~O.~Aksamit et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Aksamit</surname><given-names>Nikolas O.</given-names></name>
          <email>naksamit@ethz.ch</email>
        <ext-link>https://orcid.org/0000-0002-2610-7258</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Kravitz</surname><given-names>Ben</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6318-1150</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>MacMartin</surname><given-names>Douglas G.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1987-9417</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Haller</surname><given-names>George</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institute for Mechanical Systems, Swiss Federal Institute of
Technology (ETH), Zurich, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Earth and Atmospheric Sciences, Indiana University,
Bloomington, IN, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Atmospheric Sciences and Global Change Division, Pacific Northwest
National Laboratory, Richland, WA, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Sibley School of Mechanical and Aerospace Engineering, Cornell
University, Ithaca, NY, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Nikolas O. Aksamit (naksamit@ethz.ch)</corresp></author-notes><pub-date><day>11</day><month>June</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>11</issue>
      <fpage>8845</fpage><lpage>8861</lpage>
      <history>
        <date date-type="received"><day>10</day><month>July</month><year>2020</year></date>
           <date date-type="rev-request"><day>11</day><month>September</month><year>2020</year></date>
           <date date-type="rev-recd"><day>23</day><month>April</month><year>2021</year></date>
           <date date-type="accepted"><day>15</day><month>May</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 </copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e129">Stratospheric sulfate aerosol geoengineering is a proposed method
to temporarily intervene in the climate system to increase the reflectance of shortwave radiation and reduce mean global temperature. In previous climate modeling studies, choosing injection locations for geoengineering aerosols has, thus far, only utilized the average dynamics of stratospheric wind fields instead of accounting for the essential role of time-varying material transport barriers in turbulent atmospheric flows. Here we conduct the first analysis of sulfate aerosol dispersion in the stratosphere, comparing what is now a standard fixed-injection scheme with time-varying injection locations that harness short-term stratospheric diffusion barriers. We show how diffusive transport barriers can quickly be identified, and we provide an automated injection location selection algorithm using short forecast and reanalysis data. Within the first 7 d days of transport, the dynamics-based approach is able to produce particle distributions with greater global coverage than fixed-site methods with fewer injections. Additionally, this enhanced dispersion slows aerosol microphysical growth and can reduce the effective radii of aerosols up to 200–300 d after injection. While the long-term dynamics of aerosol dispersion are accurately predicted with transport barriers calculated from short forecasts, the long-term influence on radiative forcing is more difficult to predict and warrants deeper investigation. Statistically significant changes in radiative forcing at timescales beyond the forecasting window showed mixed results, potentially increasing or decreasing forcing after 1 year when compared to fixed injections. We conclude that future feasibility studies of geoengineering should consider the cooling benefits possible by strategically injecting sulfate aerosols at optimized time-varying locations. Our method of utilizing time-varying attracting and repelling structures shows great promise for identifying optimal dispersion locations, and radiative forcing impacts can be improved by considering additional meteorological variables.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e141">Stratospheric sulfate aerosol geoengineering relies on triggering an
atmospheric perturbation through deliberate injections of sulfate aerosols
or their precursors (often SO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) into the lower stratosphere to mimic
the cooling effects seen after large volcanic eruptions (The Royal Society,
2009). Over the last several decades, this has been suggested as a possible
means of reducing some of the impacts of climate change (e.g., Crutzen,
2006). There are, however, many open questions about the effects of
radiative forcing from sulfate injections (Kravitz and MacMartin, 2020). The
importance of choosing the altitude and latitudes of injection, and the
distribution of injection rates across those, has been clearly demonstrated,
as well as adjusting injection locations based on the season (Visioni et
al., 2020). Additionally, even for sulfate aerosols, the method of dispersal
will affect aerosol size distribution and, hence, the amount of material that
needs to be injected. To date, many of these uncertainties are based on a
climate response from fixed-injection locations (e.g., Robock et al., 2008;
Heckendorn et al., 2009; Tilmes et al., 2017), which is a significant limitation<?pagebreak page8846?> for
predicting dispersion in fully turbulent fluid flows. In fact, none of these
studies consider the short-term variations in stratospheric winds or the
organizing role of turbulent coherent structures in these time-varying
flows. Driscoll et al. (2012) showed that it is impossible to correctly
capture the impact of abrupt atmospheric perturbations on surface climate
without a well-resolved stratospheric model. With the great significance of
stratospheric dynamics for teleconnections and the state of the atmosphere
(e.g., Jaiser et al., 2013; Domeisen et al., 2019), how can we optimize where to put aerosols or precursors so that we have greater influence on the mean climate and have better efficiency?</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e155">Example of fluid particle advection for an unsteady geophysical 2D
fluid flow from time <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to time <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. For any arbitrary line of initial fluid particle positions, such as <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), that line will be
a barrier to advective transport and mixing. This is seen in the second
panel as no dark gray fluid has crossed <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> to mix with the light gray fluid.</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f01.png"/>

      </fig>

      <p id="d1e218">While benchmark studies have been quite successful at understanding the mean
climatic response of geoengineering in sophisticated Earth system models
(e.g., Kashimura et al., 2017; Kravitz et al., 2017), the injection protocols
have all neglected presently available short-term predictive information
useful for optimizing particle dispersion. An efficient dispersion of
aerosol precursors is of crucial importance for aerosol coagulation (Kravitz
and MacMartin, 2020); the particle size distribution is a critical and
sensitive parameter for accurately determining surface cooling,
stratospheric warming and changes in stratospheric dynamics (e.g., Rasch et
al., 2008; Heckendorn et al., 2009; Tilmes et al., 2008; Niemeier et al.,
2011). By only considering average flow behavior, one limits geoengineering
evaluations to simple injection protocols that do not fully exploit
turbulence, coherence and mixing in the stratosphere. This increases the
likelihood of a heterogeneous spatial coverage and localized high
concentrations of aerosols, leading to enhanced coagulation and
sedimentation rates (e.g., Pierce et al., 2010). Without a more precise
optimization of injection locations, we limit our ability to accurately
model the full potential impacts of geoengineering.</p>
      <p id="d1e222">Instead of standard fixed-locations, we propose a time-varying injection
location protocol based on the identification and prediction of short-term
Lagrangian stratospheric transport barriers. This method harnesses the
theory of Lagrangian coherent structures (LCSs), a tool for highlighting the
most influential material surfaces solely from fluid velocity fields without
any further modeling of scalar transport (Haller, 2015). For a given
unsteady fluid flow, any arbitrary surface of fluid particles, <inline-formula><mml:math id="M6" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>, will
block advective transport across these surface over time as the surface
deforms with the flow. This is shown in a real 2D velocity field of
geostrophic ocean surface currents in Fig. 1. Here, the blue line <inline-formula><mml:math id="M7" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>
separates regions of light and dark gray fluid particles. As the fluid flows
from time <inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M10" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is an advective transport barrier in that
no dark gray fluid crosses <inline-formula><mml:math id="M11" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> to mix with the light gray fluid. This result
follows immediately from the continuity of the equations defining fluid
motion.</p>
      <p id="d1e276">Instead of looking for material barriers to advective transport, of which
there are infinitely many, LCS theory identifies only exceptional
distinguished material surfaces, such as those that are mathematically
defined to be rotationally coherent, undergo minimal stretching over time
or locally attract or repel nearby fluid particles at a significant rate.
One example of the latter two structures, termed hyperbolic LCSs, and their
time evolution in the same unsteady ocean flow is shown in Fig. 2. Over
the time period <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the structure that is
mathematically defined to most effectively attract nearby particles, and
<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> repels nearby particles. By identifying exceptional material
barriers, such as the saddle feature in Fig. 2, LCS theory allows the
organization of turbulent fluid flows into coherent patterns in a
mathematically rigorous (nonempirical), physical and frame-independent
manner (Haller, 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e325">Example of time evolution of fluid particles surrounding
hyperbolic LCSs in a geophysical fluid flow from time <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is an attracting LCS (unstable manifold), and <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a repelling LCS (stable manifold).</p></caption>
        <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f02.png"/>

      </fig>

      <p id="d1e378">Though using the mathematical definition of LCSs to define atmospheric flow
structures is quite restrictive, LCSs have actually been identified
throughout the atmosphere (Tang et al., 2010; Tallapragada et al., 2011;
Rutherford et al., 2012; BozorgMagham and Ross, 2015; Knutson et al., 2015;
Wang et al., 2017). Of particular relevance to the present research is the
LCSs work of Beron-Vera et al. (2012), who demonstrated how zonal jets behave
as meridional transport barriers at high latitudes. Olascoaga et al. (2012)
analyzed LCSs in stratospheric winds to provide a rigorous definition of the
transport barriers contributing to the loss of ozone from the Arctic ozone
layer, and there was recent success in delineating LCSs along atmospheric
rivers (Garaboa-Paz et al., 2015). Jupiter's Great Red Spot and zonal jets
were identified as material transport barriers through video analysis and
LCS theory (Hadjighasem and Haller, 2016). Using a null geodesic
identification scheme, the northern polar vortex, a significant structure in
high-latitude atmospheric mixing, was accurately identified as a
transport-blocking LCS (Serra et al., 2017). Lastly, Wang et al. (2017) were
able to use a related diagnostic strain tensor field to predict the location
of space shuttle contaminant plumes in the thermosphere after 48 h of
transport. These previous results indicate the potential for the most
influential LCSs to be harnessed for geoengineering purposes. Specifically,
hyperbolic LCSs that maximize or minimize dispersion may be used as
time-varying injection locations that reduce coagulation of aerosols and
increase their lifespan and utility.</p>
      <p id="d1e381">Recently, Haller et al. (2018, 2020) derived an additional objective
criterion that specifically identifies the strongest barriers and enhancers
of diffusive particle transport. That is, one can identify the time-varying
locations of material barriers in a fluid flow that either maximize or minimize the diffusive contribution in the advection–diffusion equations over a given time frame. They have obtained a diffusion barrier strength (DBS) field whose ridges highlight the strongest diffusive transport barriers in forward-time fluid flow analysis and the strongest diffusive transport enhancers by running a
backward-time fluid flow analysis. Neither of these simulations actually
require modeling the evolution of a diffusive scalar field but still
rigorously define the structures that are most influential to diffusive
transport. For atmospheric science, this significantly reduces the
computational burden<?pagebreak page8847?> for predicting how scalar fields will evolve as it
provides quantitative information about future attraction and dispersion
patterns, without needing complex numerical machinery to model the
advection–diffusion equations or making assumptions about their unknown
initial and boundary conditions. In comparison, the effective diffusivity
approach of Nakamura (2008) provides an a posteriori visualization of
Eulerian barriers, but only after scalar transport simulations have been
performed. DBS fields, however, give an a priori (predictive)
characterization of material barriers to diffusion without ever running
diffusive simulations. This new technique increases the rigor of Lagrangian
atmospheric analysis and removes ambiguity arising from the lack of a
universal definition of coherence in atmospheric LCSs work. As such, the DBS
field is perfectly suited to optimizing aerosol dispersion and is
computable solely from available wind field forecasts and hindcasts or
reanalysis.</p>
      <p id="d1e385">In this paper, we evaluate simulated stratospheric flows with the aim
of identifying diffusive transport barriers and informing injection site
selection for enhanced stratospheric geoengineering via aerosols. In doing
so, we provide an initial demonstration of the benefits of incorporating
short-term atmospheric dynamics into geoengineering analyses and provide
suggestions to better assess its potential impacts. Our choice of
dynamics-informed injections is evaluated against fixed-injection protocols
via long-term metrics of pure advective transport and geoengineering
scenarios simulated in a fully coupled climate-model. We find significant
improvement in the ability of injected aerosols to both quickly surround the
Earth and to be able to achieve similar coverage with fewer injection
sites. We then introduce further practical and logistical restrictions on
the DBS-based protocol and maintain our method's improved performance.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Climate model data</title>
      <p id="d1e403">We use CESM2 (WACCM6; Gettelman et al., 2019) under an SSP5–8.5 scenario to
generate global wind fields at 72 levels for 18.75 years of simulation
(Table 1). These fields were computed at a spatial resolution of
0.94<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude and 1.25<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude, with instantaneous
output at 6 h frequency. As vertical motion is minimized over short
timescales along isentropic surfaces, and similar analysis has<?pagebreak page8848?> reliably
identified transport barriers along these surfaces (Serra et al., 2017), we
extracted wind fields on isentropes ranging from <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">280</mml:mn></mml:mrow></mml:math></inline-formula> to 1000 K with 20 K resolution. This is expected to provide a computationally efficient 2D
analysis of material barriers to aerosol and tracer transport. We primarily
focus on the <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">540</mml:mn></mml:mrow></mml:math></inline-formula> K isentrope in the lower stratosphere (approximately
20–25 km above sea level (a.s.l.) in the tropics) as these elevations are at the upper limit of
currently practical aerosol injection heights. The DBS injection protocols
described herein rely only on 14 d windows of wind velocity and can be
applied to wind data at any height. It is reasonable to assume that applying
these methods elsewhere and optimizing injection locations to maximize
dispersion at other heights would be beneficial for aerosol global coverage,
and similar results may be possible.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e450">Flow chart for geoengineering experiments.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f03.png"/>

        </fig>

      <p id="d1e459">A preliminary dispersion analysis was first conducted by approximating
aerosol concentration evolution from the behavior of neutral tracers
(pseudo-aerosols) that perfectly follow the wind fields (Fig. 3; left
column). At the beginning of each month for the full 18.75 years of the CESM2
(WACCM6) model simulation, injection locations were identified using a short
temporal neighborhood of the wind field output from CESM2 (WACCM6) run no. 1. The advection of parcels of neutral tracers from neighborhoods
surrounding those injection points was then computed for the following 50 months in the run no. 1 wind fields. This approximation of transport by
perfectly fluid-following particles inherently assumes that there are
negligible inertial effects, and the vertical motion is not influenced by
radiative heating or cooling of the particle (or gas). While these
assumptions limit any study of climate impacts, these calculations provide a
longitudinal comparison of dispersion from dynamics-informed injections and
traditional injection protocols that spans multiple modes of interannual
climate variability.</p>
      <p id="d1e463">We complement our neutral tracer trajectory analysis with four comprehensive
CESM2 (WACCM6) simulations spanning 1 year after the sulfate precursor
injection (Fig. 3; right column). Each simulation corresponds with
injections during a particular season. These simulations incorporate the
advection of aerosols with full microphysics, atmospheric chemistry and
radiative forcing components, as well as all other Earth system model
components. Again, the performance of DBS-informed and fixed-location sites
are compared. As the inclusion of microphysics and atmospheric chemistry
makes these simulations computationally more expensive, no further
improvements to injection site selection methods were evaluated, though
several suggestions for future work are discussed in Sect. 4.</p>
      <p id="d1e466">We note that, although run no. 1 involves calculation of neutral tracers
(resembling infinitesimal radiatively inert aerosols), run no. 2 involves
injection of the gaseous aerosol precursor SO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. SO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> requires time
to convert to sulfate aerosols (e.g., Mills et al., 2017), and the injection
strategy of SO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (for example, along a longitudinal band instead of
into a single grid box) has been demonstrated to affect aerosol size and,
hence, radiative effects of the injection (e.g., English et al., 2012).
Nevertheless, the purpose of these DBS-informed simulations is to describe
the effects of recognizing transport barriers or atmospheric features that
enhance transport. The applicability of this method is not dependent on
whether a gas or particle is injected.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Lagrangian transport extremizers</title>
      <p id="d1e504">Diffusion barrier strength (DBS) is an objective (i.e., observer-independent)
diagnostic field whose ridges highlight diffusive or stochastic transport
extremizers from velocity data (Haller et al., 2018). For a given
time-varying velocity field <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and
tracer <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi>c</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, we can describe the evolution of this
tracer with the classic advection–diffusion equation as follows:
            <disp-formula id="Ch1.Ex1"><mml:math id="M29" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>c</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>c</mml:mi><mml:mi mathvariant="bold-italic">v</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ν</mml:mi><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="bold">D</mml:mi><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>c</mml:mi></mml:mrow></mml:mfenced><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi>c</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mfenced open="(" close=")"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="bold">D</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the symmetric, positive definite
diffusion structure tensor. The left-hand side of this differential equation
contains the advection of this scalar field, whereas the right-hand side
describes transport due to diffusive processes. Furthermore, we define the
path of a fluid particle in the velocity field
<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> as a solution to the ordinary
differential equation <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>x</mml:mi><mml:mo mathvariant="normal">˙</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mi mathvariant="bold-italic">v</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>,
described by the flow map as follows:
            <disp-formula id="Ch1.Ex2"><mml:math id="M33" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          From here, we define the DBS at a point <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over the
time interval <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>, as follows:
            <disp-formula id="Ch1.Ex3"><mml:math id="M36" display="block"><mml:mrow><mml:mtext>DBS</mml:mtext><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mtext>trace </mml:mtext><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold">T</mml:mi><mml:mo mathvariant="normal">¯</mml:mo></mml:mover><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where overbar denotes the time average of the transport tensor as follows:
            <disp-formula id="Ch1.Ex4"><mml:math id="M37" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">T</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="bold">D</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mo>⊤</mml:mo></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          for <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>∈</mml:mo><mml:mo>[</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e928">Example of DBS-informed injection scheme at 540 K that selects the
injection sites. The global view shows 7 d DBS<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> fields with two sections of disconnected, strongly attracting structures highlighted in the green box. For the larger structure, we then identify all points closer to that attracting structure and select the unique point that will result in
the most significant dispersion of aerosols. This is injection site is shown
as the red dot on the DBS<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> ridge in the inset. Injecting aerosols at these points will cause them to both spread quickly and converge to a large and complex attractor. Units for both forward and backward DBS fields are given per day.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f04.png"/>

        </fig>

      <?pagebreak page8850?><p id="d1e955">The diffusion structure tensor <inline-formula><mml:math id="M41" display="inline"><mml:mi mathvariant="bold">D</mml:mi></mml:math></inline-formula> is capable of
representing parameterizations of many complex diffusion-like processes, but
our research focuses on molecular (i.e., homogeneous, isotropic and steady)
diffusion, in which case <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi mathvariant="bold">D</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is
constantly the identity matrix. In this situation, the transport tensor
<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">T</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> reduces to the inverse of the Cauchy–Green
strain tensor, <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>⊤</mml:mo></mml:msup><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, which also arises in the computation of
the finite-time Lyapunov exponent (FTLE) used in previous atmospheric
transport barrier studies (see, e.g., Beron-Vera et al., 2012; Olascoaga et
al., 2012; Garaboa-Paz et al., 2015; Serra et al., 2017; Wang et al., 2017).
DBS values are, therefore, pointwise equal to the trace of the time-averaged
<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:msubsup><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup><mml:msup><mml:mo>]</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mfenced open="[" close="]"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msubsup><mml:mi mathvariant="bold">F</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mo>⊤</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> tensor. One notable difference
between DBS and FTLE is the inclusion of diffusive or stochastic transport
in the definition of transport barriers or enhancers for DBS, a process
essential to predicting aerosol dispersion in the stratosphere. The
inclusion of diffusion in the transport functional allows for a systematic
search for extremizing surfaces to transport (Haller et al., 2018), thereby
eliminating the ambiguity inherent in various available coherent structure
definitions (see Haller, 2015) or a lack of precision from simple
heuristics. Accounting for diffusive and stochastic transport necessarily
leads to the inclusion of <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>t</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> tensors for all
<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>∈</mml:mo><mml:mo>[</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula> in the definition of the DBS. In contrast, computing the
FTLE only includes the single tensor <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e1187">Using a limited time window of the modeled wind flow for DBS calculations,
we were able to effectively simulate a real-time geoengineering scenario.
For each injection time, <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, in our 18.75 years of simulation (run no. 1), we analyzed 1 week of future flow data and 1 week of previous
flow data as proxies for forecast and reanalysis, respectively, to determine
optimal locations for sulfate injection. The 1 week DBS<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> field was
calculated from <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>, and the under reversal of the direction of
the flow in the reanalysis data, the DBS<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> field was calculated from
<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>. As is described by Haller et al. (2018), the ridges of
DBS<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> highlight the locations of the strongest dispersion (i.e., diffusive transport limiters) on the globe at <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, while the ridges of DBS<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> indicate the locations of the strongest accumulation (i.e., diffusive transport enhancers) at <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. These diffusive transport barriers are
analogous to the structures <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from Fig. 2 but account
for diffusive and advective transport in the flow. To identify DBS
ridges, we advected fluid particles along isentropic surfaces to simplify
calculations and ignored vertical motions.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1338">Summary of the method of identifying injection locations for
DBS-informed injections.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="10cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">DBS-enhanced aerosol injection location search algorithm. </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2"><bold>Input:</bold> wind fields surrounding the injection day (<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) from <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> d. </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><list list-type="order">
                      <list-item>

      <p id="d1e1417">Calculate reanalysis DBS<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> from <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>, and forecast DBS<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>.</p>
                      </list-item>
                      <list-item>

      <p id="d1e1494">Extract attracting ridges as connected components of the DBS<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> field above a fixed threshold via flood-fill algorithms.</p>
                      </list-item>
                      <list-item>

      <p id="d1e1509">Find the seven largest ridges and identify all points that are closer to each ridge than to any other ridge.
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e1514">If we cannot find seven unique ridges, we will use as many unique ridges as we can and separate the ridges into intersections with latitude bands. Then, we will find points closest to our subdivided ridges.</p></list-item></list></p>
                      </list-item>
                      <list-item>

      <p id="d1e1520">If specified, restrict the neighborhood of ridges to that which intersects with neighborhood of airports.</p>
                      </list-item>
                      <list-item>

      <p id="d1e1526">Identify the points with the highest DBS<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> value for each neighborhood, and select the highest seven values.</p>
                      </list-item>
                    </list></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2"><bold>Output:</bold> seven aerosol injection locations optimized for the wind flow on day <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. </oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1563">We identified strongly attracting flow features as connected components of
the DBS<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> field with values above a simple fixed threshold. This
threshold was chosen empirically from the range of DBS values in these
calculations and was constant for all structure identification at all
<inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. As also seen for other objective coherent structures identified
from short-term calculations (e.g., Serra and Haller, 2016), these 7 d
attracting features persist for much longer than their domain of computation
in the flow and continue to attract many nearby fluid particles. Near each
strongly attracting feature, the location with the largest DBS<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> value signals a potential injection site for geoengineering as it indicates the strongest local dispersion over the next 7 d. We
balance strong dispersion and nearby strong attractors to both maximize the
spread of aerosols and to prevent multiple injections being attracted to the
same sections of the same attractor. When possible, this methodology
prevented aerosols or precursors injected at initially distant sites from
traveling great distances only to be attracted to the same portion of the
flow. A flow chart detailing the injection location selection process is
shown in Fig. 4.</p>
      <p id="d1e1595">While we prioritize injecting near unique attractors, this was not always
possible given that single <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">DBS</mml:mi><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ridges could also span much of the
globe, and in rare instances, strong attractors were not present in all
regions. If seven unique attractors are not available at a given time, we
simplify the process and choose the maximal <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">DBS</mml:mi><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> site near an
attractor for each of the following seven latitude bands: [<inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7.5</mml:mn></mml:mrow></mml:math></inline-formula>,
7.5<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>], [<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">7.5</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">22.5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>],
[<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">22.5</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">37.5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>] and [<inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">37.5</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">62.5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>]. This dynamics-based injection
approach, referred to as DI in the text, adapts to any isentrope or future
climate scenario as the injection location choice always depends on the
state of the stratosphere at the time of injection. This automated search
algorithm is summarized in Table 1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1727">Global coverage of potential injection locations for an
airport-bound scenario, including a map of 9300 airport locations (red dots)
and the distance to the nearest airport up to 1000 km.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f05.png"/>

        </fig>

      <p id="d1e1737">As a control study, we ran a baseline scheme that injected sulfate aerosols
at seven fixed-injection locations, referred to in the text as FI (<inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mn mathvariant="normal">15</mml:mn><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>±</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude at 260<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude),
similar to those explored by others (e.g., Robock et al., 2008; Heckendorn et
al., 2009; Tilmes et al., 2017). Lastly, we ran a scenario where
DBS injections were restricted to within 1000 km of an airport (scenario ADI
in the text; Global Airport Database, 2020) as a logistical handicap more
similar to real-world possibilities (Fig. 5). For both the unrestricted
DBS and the airport protocols, we limited the selection of injection
locations to latitudes between <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">62.5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> to avoid trapping by
meridional barriers near the poles (Beron-Vera et al., 2012) while
maximizing global coverage. Despite this restriction, the stratospheric flow
sufficiently mixed aerosols across the globe, as with the FI experiments.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Geoengineering performance metrics</title>
      <?pagebreak page8851?><p id="d1e1815">For our basic dispersion analysis, we evaluated the effective global
coverage and rate of dispersion via an average minimum distance metric,
defined as follows:
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M96" display="block"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mfenced close=")" open="("><mml:mi>t</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:msub><mml:mo>∑</mml:mo><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>∈</mml:mo><mml:mi>D</mml:mi></mml:mrow></mml:msub><mml:mi mathvariant="normal">min</mml:mi><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfenced><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>∈</mml:mo><mml:mi>D</mml:mi></mml:mrow></mml:math></inline-formula> are all points on the globe, <inline-formula><mml:math id="M98" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> is the great circle
distance, <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the location of all neutral (pseudo-aerosol)
tracers at time <inline-formula><mml:math id="M100" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M101" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is the number of grid points on the globe used
for the calculation. Lower values of <inline-formula><mml:math id="M102" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> indicate a shorter distance from
any point on the globe to the nearest pseudo-aerosol tracer and, thus, imply
better coverage. As volumetric or mass concentrations of aerosols are
driving factors in many of the microphysical processes governing aerosol
lifespan, we also calculated the entropy of the distribution of the
pseudo-aerosols in our infinitesimal neutral tracer experiment. For a given
probability <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on a discretized grid of (unequal) bins (such as tracer
concentration), we determine the following:
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M104" display="block"><mml:mrow><mml:mi>E</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mo>∑</mml:mo><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>∈</mml:mo><mml:mi>D</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi>p</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:msub><mml:mi>log⁡</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the size of a bin (Harris, 2006). The evolution of the
entropy of each injection protocol was normalized by the entropy of a
perfectly uniform distribution on the same discrete grid to give a
normalized entropy value in the interval [0, 1].</p>
      <p id="d1e1997">At the beginning of each month during the 18.75-year CESM2 simulation, we
initiated advection of fluid-following neutral tracers from seven DI sites,
seven ADI sites and seven FI sites that lasted for 50 weeks. In these
initial experiments, we did not run a new simulation of CESM2 (WACCM6) but
used the advection of neutral tracers in wind fields generated by
CESM2 (WACCM6; run no. 1) to approximate the dispersion dynamics of aerosols
in a fully turbulent stratosphere (left column of Fig. 3).</p>
      <p id="d1e2000">In our second round of experiments, we used the precomputed wind fields from
CESM2 run no. 1 to determine injection sites, and then ran new CESM2
simulations starting in each season (run no. 2) with 10 Tg SO<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
injections that included fully coupled microphysics. In this way, the
atmosphere was influenced by geoengineering in run no. 2 but not in our
neutral tracer experiments. The effective global coverage, SO<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
and effective radii were then compared for the two DBS-informed (DI and ADI
in the text) protocols and one fixed (FI) injection protocol.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>DBS influence on pseudo-aerosol dispersion</title>
      <p id="d1e2037">For the infinitesimal neutral tracer advection experiment (Fig. 3; left
column), the global coverage of pseudo-aerosols injected at seven
dynamically varying DBS locations was much greater than coverage from the
seven fixed (FI) locations. We found an immediate increase in global
coverage for the DI experiments, as predicted from the mathematical
definition of large DBS<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> values. Zonal concentrations of
pseudo-aerosol tracers were calculated as the fraction of the total number
of tracers present in a given discrete latitude band.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2051">DBS-informed injection yields significantly enhanced coverage over
fixed-location injections over short-term, 7 d periods. Zonal
concentrations in panels <bold>(a)</bold>–<bold>(d)</bold> are calculated as the fraction of the total number of neutral tracers (pseudo-aerosols) in a given latitude band at a given time. The time evolution of zonal concentration over 1 week of transport from the two injection protocols is displayed in panels <bold>(a)</bold>–<bold>(d)</bold>, with the respective normalized entropy values in panels <bold>(e)</bold>–<bold>(f)</bold>.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f06.png"/>

        </fig>

      <?pagebreak page8852?><p id="d1e2079">Figure 6a and c detail how the zonal concentrations of these idealized
sulfates injected at the standard FI sites evolve over the first 7 d
of transport during boreal summer and winter, respectively. While there is
north–south meandering of the injected tracers, the fixed-injection scheme
resulted in little to no dispersion by the end of the first week. In
contrast, after only 3 d of transport, Fig. 6b and d show that the
DI tracers have begun efficiently spreading and increasing global coverage.
As discussed later and exhibited in the full microphysics simulations in
the next section, this immediate dispersion (which, while idealized in run no. 1, could apply to aerosols or their gaseous precursors) has an impact on
the rate of coagulation, sedimentation and the effective radii and lifespan
of the aerosols. By the end of 7 d, the DI tracers have covered a
large portion of the Northern and Southern hemispheres from <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> to
70<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for both the summer and winter injections. This difference in
global coverage between DI and FI schemes is further quantified by the
normalized entropy of pseudo-aerosol tracer distributions for the two
protocols. In the bottom two subplots of Fig. 6e and f, the
pseudo-aerosol tracer distribution from the DI protocol has greater entropy
(Eq. 2) after 1 d of transport with that performance gap widening for
the entire week. At the same time, the near-constant entropy for the FI
experiments verifies that those clusters of neutral tracers have not yet
dispersed and create a longer window of time for sulfate hot spotting
and coagulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2104">Normalized entropy of DBS-informed injections under a varying
number of sites for the summer simulation in Fig. 6. Through optimizing
injections near dispersion-enhancing transport barriers, we are able to
achieve significantly more uniform distributions of aerosols with fewer
necessary injection sites.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f07.png"/>

        </fig>

      <p id="d1e2113">The enhanced dispersion, made possible by harnessing DBS information, also
allows for a streamlining of injection operations. Using the same time
period from Fig. 6a and b, we were able to leverage the improved distributions
of pseudo-aerosols and test how reducing the number of DBS injection sites
would influence the subsequent global coverage. Figure 7 shows that, for one
such test, almost immediately, there is a negligible reduction in entropy
when reducing from seven DBS-informed injections to six. That is, within the
first day of dispersion, reducing the number of injection locations and the
amount of injected material by nearly 15 % does not impair the performance
of our DBS protocol to levels below that of the fixed locations. After 3 d, when the influence of strong DBS barriers has been more effective, one
can reduce injections to only two DI sites and still obtain a more uniform
concentration distribution than with seven FI sites. From 4 d to the
end of the first week, a single injection site was dispersing
pseudo-aerosols in the stratosphere more effectively than the combination of
all seven fixed sites. Not only could a well-informed choice of<?pagebreak page8853?> injection
locations provide significant benefits for increasing concentration
homogeneity (thereby more evenly influencing radiative forcing and reducing
hot spotting), there can be significant strategic and economic advantages of
DBS-informed geoengineering programs.</p>
      <p id="d1e2116">To determine if injecting at DI sites would consistently increase dispersion
over all seasons and over many years, we consider the cumulative statistics
of many long-term advection models. At monthly intervals, the same 7 d
reanalysis and forecast method was used to choose DI locations, both with
and without a 1000 km distance restriction to the nearest airport (ADI).
After 1 week, 10 weeks and 50 weeks of transport, <inline-formula><mml:math id="M111" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> values (Eq. 1)
were computed and compared to the FI protocol. Figure 8 shows the results of
this experiment for transport periods spanning the whole 18.75 years.
Clusters of <inline-formula><mml:math id="M112" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> values indicate variance in the response of
pseudo-aerosol transport to different DBS ridge structures over time, but
mean values of those clusters (indicated by horizontal lines) consistently
show improved coverage compared to the FI protocol. As noted before, the
most considerable enhancement in dispersion was seen immediately, supporting
the potential for this approach to influence aerosol microphysics during the
first week of transport. After 10 weeks, DI injections were still more
effective at global coverage than the FI protocol, even with the airport
restrictions, but at yearly timescales, the average improvement was minimal.
It should be noted that the variance of global coverage was also lowest for
DI seeding at 10 and 50 weeks.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2135">Average distance to the nearest aerosol (Eq. 1), with injections
initialized each month for 18.75 years. The top three subplots compare the
fixed location (FI) protocol to the DBS-informed (DI) injection after 1 week, 10 weeks and 50 weeks of transport, with cluster means marked by
respective horizontal lines. The bottom three subplots are analogous with
the added restriction that DBS-informed injections must also be within 1000 km of an airport (ADI). Both DBS approaches outperform the fixed injection protocols up to 10 weeks, suggesting flexibility of the protocols and utility of harnessing Lagrangian coherent structures for enhancing
dispersion.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Full atmospheric chemistry and microphysics simulations</title>
      <p id="d1e2152">Beyond improved advective transport of aerosols or precursors, we also wish
to investigate the role that diffusion transport barriers may play in
dampening microphysical processes that can reduce the lifespan of
geoengineering aerosols, such as coagulation and sedimentation, in a fully
coupled climate model. To address this, we applied the DI and ADI site
selection methods at the beginning of 4 months (January, April, July and
September) during 1 year of CESM2(WACCM6) output. We then reran 12
CESM2 (WACCM6) simulations with injections of 10 Tg of SO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for the three
separate protocols on a given day, <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, in each season. For each model
run, the SO<inline-formula><mml:math id="M115" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was divided evenly between the seven fixed or dynamic
injection sites on the 540 K isentrope. This provided 12-year-long model
simulations that calculated the total evolution of injections from each
geoengineering protocol. The average effective radii of the resulting
sulfate aerosols, total column SO<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden (kilograms per square meter – <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">kg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) and
top-of-atmosphere radiative forcing was measured on a lat–long grid over
isentropes from 360 to 720 K. The seasonal experiment names referred to in
this section correspond with the boreal season.</p>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Aerosol burden</title>
      <p id="d1e2217">As DBS ridges and this particular coherent structure view of stratospheric
dynamics are mathematical tools for addressing dispersion and transport, we
initially focus on enhancements in SO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> dispersion and global coverage
when using DBS-informed site selections. To account for the natural
variability in the SO<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden in our control runs, effective coverage was
quantified from the cells whose total column SO<inline-formula><mml:math id="M120" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden exceeds 5
times the average global burden for the 1 week prior to sulfate injection.
The amount of global coverage is then the percent of the surface area of the
Earth, with SO<inline-formula><mml:math id="M121" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> exceeding this threshold. Around 1 % of the surface
area of the Earth exceeds this threshold prior to injection.</p>
      <p id="d1e2256">Figure 9 shows the difference in global coverage between the DBS schemes and
the FI protocol. A consistent short-time pattern was evident in these time
series for all the injections for four seasons. There is an immediate positive
difference with the DBS approaches as a greater percent of the Earth is
efficiently covered by an above-average SO<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden. This initial
improvement in coverage peaks between 1 and 2 weeks after injection
and is attributed to high DBS<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> values at injection locations and an
enhanced ability to strategically spread along nearby jets and eddies that
were present in the DBS<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> fields. These dispersion patterns and their
correlation with DBS<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> ridges can be seen in the SO<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
plots of Fig. 10. This immediate improvement can be as high as 5 % more
global coverage, equating to a change in net radiation over an additional 32 million km<inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> or more than the equivalent surface area of North America.</p>
      <p id="d1e2314">After the initial peak improvement in global coverage, there is often a
rebound in Fig. 9, at which point the FI aerosols can cover up to 12 %
more of the globe. Surprisingly, after this local minimum, there is always a
secondary peak, sometimes larger than the first, showing a response in
global coverage using the DBS methods well past the computational
limitations of the original DBS ridges. This second peak in performance
occurs between 6 and 10 weeks after injection, and enhanced coverage
by the DBS methods can extend until all three experiments achieve total
global coverage.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e2320">Analysis of CESM2 (WACCM6) output showing the increase in percent
of the Earth's surface surrounded by an SO<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden greater than 5
times the global mean from the week prior to injection as compared to fixed
injection protocols. Large subplots show the first 90 d after injection,
and the smaller subplots show the first full year.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f09.png"/>

          </fig>

      <p id="d1e2338">Notably, the spring and summer season injections had much smaller relative
improvements in their initial peaks in Fig. 9. A closer investigation of
the dispersion patterns in Fig. 10 begins to explain why. The left three
columns of Fig. 10 show the SO<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden, with the two inset percentages
in each plot detailing the proportion of the respective hemisphere's (north
or south) surface area covered by 5 times the pre-injection burden means. The
right column shows the DBS<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> field calculated for the 540 K isentrope
wind fields from the injection time <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> d, so that the
location of attracting structures coincides with the concurrent dispersion
patterns. The winter injections occurred in the presence of strong
attracting features in most latitude bands, and the DBS-informed methods
were able to exploit these,<?pagebreak page8854?> especially in the Northern Hemisphere.
Dispersion along these attracting features continued to enhance coverage for
DI and ADI injections well after the snapshot in Fig. 10. During spring,
the DBS-informed injections exploited the similar attracting features in the
Northern Hemisphere (13 % vs. 12 % coverage), but in the Southern
Hemisphere, attracting ridges around <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> blocked aerosols from
migrating further south in all three experiments.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e2405">Analysis of CESM2 (WACCM6) output, showing the SO<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
after 7 d of transport for the three injection protocols in each
season. The percent of the Earth's surface covered by an SO<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
greater than the global mean from the week prior to injection is noted in
the top left of each panel. Original injection locations for each experiment
are shown as red dots. Units for the color map are kilograms per square meter.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f10.png"/>

          </fig>

      <p id="d1e2432">The summer injections occurred during an absence of strong attracting or
repelling structures, except a dominant circumpolar feature in the Southern
Hemisphere. The DBS<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> values for sites chosen north of <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">37.5</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
for the summer DI and ADI experiments were the lowest of all the
experiments. In the Northern Hemisphere, aerosols spread by way of these
locally maximal DBS<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> injection sites, but no strong anticyclonic
structures, such as those found in the other seasons, were present. This
prevented Northern Hemisphere aerosol clouds from deforming along
space-filling spiral features, such as in the south and in other seasons. The
autumn injection occurred during a time with stronger DBS<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> and
DBS<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> ridges than the summer injection and allowed for an enhanced
dispersion in the south, especially for the DI experiment. The true strength
of the DBS approach can be seen in the autumn experiment as only minor
modifications in the Southern Hemisphere were necessary to achieve
considerable enhancement in coverage. After 7 d, DI SO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
was above our threshold for 21 % of the globe, versus only 16 % from FI.
This advantage comes solely from enhanced performance in the Southern
Hemisphere, where DI coverage was 13.4 % and FI lagged at 6.8 %. This
significant advantage came from only a minimal change in injection point.
The southernmost DI site was 0.25<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude further south than the FI
site, and less than 650 km away, but the presence of strong DBS<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula>
ridges and complementary high DBS<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> values allowed for a beneficial
optimization.</p>
      <p id="d1e2526">Figure 11 details the SO<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden after 8 weeks of transport. At
this point, during the last oscillation of Fig. 9 prior to total coverage,
the three injection techniques begin to converge. Notable exceptions to this
are the enhanced polar coverage in the winter DI injection in the autumn ADI
experiment.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e2541">Analysis of CESM2 (WACCM6) output showing the SO<inline-formula><mml:math id="M148" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
after 8 weeks of transport for the three injection protocols in each
season. The percent of the Earth's surface covered by an SO<inline-formula><mml:math id="M149" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden
greater than the global mean from the week prior to injection is noted in
the top left of each panel. Units for the color map are kilograms per square meter.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f11.png"/>

          </fig>

</sec>
<?pagebreak page8855?><sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Effects on radiative forcing</title>
      <p id="d1e2576">The dispersion patterns caused by the hyperbolic coherent structures in the
stratosphere discussed in the previous section impacted the
top-of-atmosphere radiative forcing (RF) in a complex way. The net shortwave
and longwave fluxes were calculated for each grid cell on each day, as were
the radiative fluxes for a control run over the same period without
geoengineering. The control fluxes were then subtracted from net fluxes to
give a spatial and temporal distribution of the relative influence of each
injection scheme. This change in RF is directly correlated with a change in
temperature and is a strong indicator of the climatic influence of
geoengineering (Hansen et al., 1997; Gregory et al., 2004).</p>
      <p id="d1e2579">Comparing the global effect of the FI protocol with DI and ADI, we find the
cumulative impact of the DI and ADI injection was stronger in many cases.
Table 2 shows the mean global change in RF for each injection protocol,
during each experiment, after three periods of time (10, 30 and 365 d) and calculated as the average difference in net radiation at the
respective time after injection. The three values in each column correspond
to the global average FI (black), DI (orange) and ADI (green) difference
from the control run in watts per square meter. Gray shaded cells indicate times at
which FI resulted in stronger radiative forcing than DI and ADI. Bold DI and
ADI values indicate a statistically significant difference (at 95 %) in RF
from the FI protocol using a two-sided <inline-formula><mml:math id="M150" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e2592">Global average improvement in RF (watts per square meter) at specified
intervals after injection as compared to CESM2 (WACCM6) control runs for FI,
DI and ADI injection schemes (left, middle and right, respectively). Bold values indicate a statistically significant difference in mean RF between FI and the corresponding DBS-informed injection on that day. <inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mo>⊗</mml:mo></mml:msub></mml:math></inline-formula>
subscripts indicate times at which FI resulted in stronger RF than both DI
and ADI.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">10 d</oasis:entry>
         <oasis:entry colname="col3">30 d</oasis:entry>
         <oasis:entry colname="col4">365 d</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Winter</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.4</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.0</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.9</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">5.0</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mn mathvariant="normal">6.2</mml:mn><mml:mo>⊗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7.6</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">3.6</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mo mathvariant="bold">+</mml:mo><mml:msub><mml:mn mathvariant="bold">0.4</mml:mn><mml:mo>⊗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Spring</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.1</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.3</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">2.0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7.6</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.7</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:msub><mml:mn mathvariant="bold">6.1</mml:mn><mml:mo>⊗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11.1</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11.2</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">9.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Summer</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.2</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mn mathvariant="normal">0.8</mml:mn><mml:mo>⊗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4.0</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">6.1</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">6.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.4</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.0</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:msub><mml:mn mathvariant="bold">2.0</mml:mn><mml:mo>⊗</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Autumn</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.0</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.1</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.4</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9.9</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">11.1</mml:mn></mml:mrow></mml:math></inline-formula>/<inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mo mathvariant="bold">-</mml:mo><mml:mn mathvariant="bold">4.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e3050">Over the first 10 d of transport, the range of time for which our DBS
methods can be mathematically supported, both global coverage and RF was
often improved with DBS-informed injection. As could be expected from
Sect. 3.2.1, there was a reduction in RF for summer DI and ADI
experiments. This corresponds with a lack of attracting and repelling
structures and questionable conditions in which to apply our injection
site selection algorithm. After 30 d, only winter and spring RF for FI
outperformed DI or ADI. This is during the rebound period detailed in Fig. 9. At this point, well beyond the time horizon of our DBS calculations,
summer and autumn DI and ADI had stronger RF than FI. After 365 d of
transport, FI outperformed the DBS protocols for the winter and summer
injections. At these timescales, it can be safely assumed that the chaotic
nature of stratospheric winds prevents any intelligible dependence on
initial conditions for these injection experiments. There exists a complex
nonlinear relationship between global coverage and RF; however, during the
forecast windows we have investigated, there is a strong correlation between
the enhanced<?pagebreak page8856?> dispersion from DBS-informed injections and RF. For longer-term
trends, one likely needs to couple the short-time dispersion with other
influential climatic variables, such as the season of injection (e.g., Visioni et
al., 2020).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Aerosol-effective radii</title>
      <p id="d1e3061">The last metric from the geoengineered CESM2 simulations we analyzed is the
effective radius of aerosols (Fig. 12). The time evolution of the
mass-averaged SO<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> aerosols was calculated on the 540 K isentrope, at
the height where injection occurred. To prevent contributions of naturally
occurring aerosols, the averages were calculated only using grid cells where
the SO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden exceed 5 times the pre-injection mean. During the
winter season, the most dramatic change in radii occurred, with peak values
for the simple injection protocol clearly exceeding the DI and ADI methods.
Differences in other seasons were more minor, but the injection protocol
peaked at higher values for both the spring and autumn experiments as well.
During summer, there was reduced performance with the DBS-informed
injections, as was also indicated in the RF and SO<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden analysis.</p>
      <p id="d1e3091">The improvement that was possible during the winter injection is notable as
it suggests that a better understanding of the connection between stratosphere
dynamics and chemistry can clearly be beneficial for aerosol geoengineering.
This is<?pagebreak page8857?> important because larger aerosols backscatter less (meaning more
aerosol is required to achieve a given level of radiative forcing), heat the
stratosphere more (resulting in greater side effects on stratospheric
circulation and surface climate) and have increased sedimentation
velocities (also meaning more aerosol is required; Pierce et al., 2010;
Tilmes et al., 2017; Simpson et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e3096">Mass-averaged effective radius of injected SO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> aerosols on
the 540 K isentrope spanning 1 year of CESM2 (WACCM6) simulations after
injection.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/8845/2021/acp-21-8845-2021-f12.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Discussion and conclusion</title>
      <p id="d1e3124">Here we have explored the use of diffusive transport barriers to guide
strategic injection locations for stratospheric aerosol geoengineering.
Compared to commonly used methods that rely on fixed-injection locations,
this dynamic site selection allows for immediate improvements in particle
dispersion and better global coverage, often with fewer injection sites.
This has important implications for previous studies regarding the
efficiency of aerosol optical depth versus injection rate. In particular, by
focusing on only fixed-injection locations (e.g., Robock et al., 2008; Tilmes
et al., 2017, among others) these studies neglected an influential variable, namely
the time-varying locations of stratospheric diffusive transport barriers. It
is safe to assume that, since these studies did not optimize injections for
dispersion, they have thus far underestimated what is possible for
geoengineered sulfate aerosols reflectance. Using a Lagrangian coherent-structure-informed approach via DBS fields shows promise for strengthening
the role that geoengineered aerosols can play in altering climate dynamics,
especially at short timescales or if logistical restrictions mean injection
sites must be strategically chosen.</p>
      <p id="d1e3127">With dynamic injection locations, initial particle concentrations spread
much more quickly, as indicated in our tracer experiments (Figs. 6 and 8)
and in the full CESM2 simulations (run no. 2; Figs. 10 and 11). This
reduces the probability of coagulation for each individual injection and
likely influenced lower peak effective radii present in DI and ADI
experiments (Fig. 12; e.g., Mills et al., 2017). With reduced coagulation,
there will be a slower descent of sulfates from the stratosphere (and out of
action) and increased<?pagebreak page8858?> scattering. Second, increased dispersion
uniformity, as quantified by normalized entropy in Figs. 4 and 5, will
reduce local stratospheric heating and result in more uniform radiative
forcing. This is because heat transfer to aerosol particles in a given
volume is proportional to the mass, which is reduced by lower
concentrations. Lastly, in the fully coupled CESM2 (WACCM6) run no. 2
experiments, DBS-informed injections improved global coverage by SO<inline-formula><mml:math id="M192" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>.
This ability to more quickly achieve total coverage provides an opportunity to
strategize geoengineering protocols with a shorter window for interference
in chaotic flows.</p>
      <p id="d1e3139">The results here indicate a predictable enhancement of dispersion for
geoengineering if influential hyperbolic structures are present in the
stratosphere. When there are strong short-term DBS<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FW</mml:mi></mml:msub></mml:math></inline-formula> and DBS<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula>
ridges, such as in the winter, spring and autumn CESM2 run no. 2
experiments, we show that we can exploit these ridges to optimize the
immediate dispersion of aerosols. Additionally, the fine-scale behavior of
aerosol dispersion can be explained by the presence of influential
structures, such as the attraction and blocking that occurs in the Southern
Hemisphere run no. 2 spring experiment. These fine-scale structures have not
been actively considered in geoengineering research but may be exploited, as
is clear in the Northern Hemisphere for the winter and spring experiments
(Fig. 10). In our fully coupled microphysics and atmospheric chemistry
climate simulations, we also verified that initial improvements in particle
dispersion from simplified flow calculations can result in less coagulation
and increased aerosol spread, as evidenced by more areal coverage by SO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>
burden and reduced effective aerosol radii. The enhanced global distribution
of SO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> for the two DBS-informed injection protocols after months of
transport (e.g., Fig. 11) speaks to the utility of the strategic placement of
aerosols or precursors near hyperbolic structures, as do long-term radiative
forcing improvements (Table 2) and correlated, yet complex, relationships
with reducing average effective radii.</p>
      <p id="d1e3178">The extent of this influence is dramatically portrayed in the autumn CESM2
run no. 2. At this time, a minimal modification of the injection site in the
Southern Hemisphere near strong hyperbolic structures and a change of less than
650 km resulted in aerosols spreading over an additional 7.5 % of that
hemisphere after 7 d. After 8 weeks, this immediate DI dispersion
benefit was not as noticeable, but the ADI scheme still contributed to
improved coverage over the FI aerosols. The enhanced coverage in the autumn
experiment is, furthermore, coincident with a considerable improvement in RF
for the DI experiments at 10, 30 and 365 d. Additionally, there was a
minor but statistically significant reduction in average aerosol radii
(<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> 1 year after the SO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> injection. At longer timescales for several of the other CESM2 run no. 2 geoengineering experiments,
the relationship between immediate enhanced dispersion, radiative forcing
and aerosol radii was less clear. For example, in spring, the ability to
achieve global coverage and reduce radiative forcing at long timescales was
best for the DI protocol, but there was not a similar improvement in average
aerosol effective radius. In the winter DI simulation, there was a
significant reduction in aerosol radius and improved coverage compared to
FI, but there was a weaker effect on radiative forcing 1 year after
injection.</p>
      <p id="d1e3215">To manage uncertainties in atmospheric flow and climate response, several
recent geoengineering climate modeling studies have employed a feedback
algorithm that adjusts the SO<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> injection rate at one or more latitudes
(Jarvis and Leedal, 2012; MacMartin et al., 2014; Kravitz et al., 2017) in
response to changes in surface climate; studies to date have updated the
forcing once per year. In future studies, this slow feedback could be
integrated with DBS-informed injection.<?pagebreak page8859?> Outlining this process, for every week
of simulation, new injection locations would be determined based on wind
fields from the previous week, using the DBS algorithm described previously
to find locations within different latitude bands. The model would then be
run forward for a week with the SO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> injected at those locations. This
process, which essentially constitutes a form of model predictive control
(García et al., 1989), could be carried out for a year, at which point the
injection rates to use in each latitude range would be updated using the
same slow climate-response-dependent feedback.</p>
      <p id="d1e3236">This research has shown that adapting aerosol geoengineering injections
methods by considering 2D Lagrangian coherent structures provides an obvious
advantage for dispersion of aerosols by enhancing longer-term dispersion
dynamics from only short forecast data. All results in Sect. 3.1 suggest
DBS-informed sites reliably outperform fixed locations when considering
aerosol dispersion along isentropes as is rigorously guaranteed in the DBS
metric derivation. The site-selection algorithm developed herein, however,
does not consider the full three-dimensionality of stratospheric flows or
any knowledge about common meteorological and climatic features. Thus, the
user-independent injection protocol does not always result in enhanced
radiative forcing or global coverage when strong attracting and repelling
features are not present in all regions, such as the summer experiments in
CESM2 run no. 2. With this is mind, we suggest that future injection
experiments use DBS fields and diffusive transport barriers to constrain
their choice of injection site but allow for user intervention in the
absence of such strong dispersive ridges and consider other influential
variables, such as seasonality of injection (e.g., Visioni et al., 2020), and
aerosol microphysics, such as temperature and humidity.</p>
      <p id="d1e3239">In one injection season (winter), there is an appreciable reduction in the effective radius, and a more negligible effect in the others. This indicates
that there is both the potential for dynamic injection to result in smaller
aerosols, and it suggests there is room for improving our understanding of
the role that dispersive stratospheric dynamics play in aerosol coagulation.
Future work along these lines may further improve upon the findings
indicated here and help us to understand the limits of what improvement
in reducing aerosol size is still possible by considering time-varying,
small-scale turbulent features.</p>
      <p id="d1e3242">Related to this study is the proposed idea of direct injection of
H<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>SO<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> droplets, instead of SO<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas, which would ostensibly
create a more monodisperse particle distribution and, thus, delay coagulation
(Pierce et al., 2010). Further investigation is warranted to understand the
relative effects of this method vs the SO<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> injection simulated in our
CESM2 (WACCM6) simulations, particularly if injection locations are chosen
dynamically. This is especially important given the stratospheric chemistry
involved in SO<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> injection, including the approximately 1-month
timescale of conversion from SO<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to sulfate aerosols, although, in
principle, a transport barrier would apply to both gases and particles.</p>
      <p id="d1e3300">The results presented here are for a single model; different models will
indicate different stratospheric features and, thus, different transport
barrier locations and strengths. Of key importance is that the long-term
dispersion analysis and structure identification methodology relied on
2D transport along isentropes. This method has proven to be
successful for advancing the goals of optimizing sulfate precursor
injections; a full 3D computation of DBS fields would further
improve the results. On reviewing the results, it appears there was an
overemphasis on the ability to separate unique attracting structures
from the 2D isentrope data. With the automated algorithm defined in Table 1,
pairs of injection sites were sometimes chosen to be close together as it
appeared their injected aerosols would end up on separate structures. In
fact, these features may have actually been connected along the third
dimension. Additionally, long-term trends of the SO<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> burden present in the
stratosphere were mixed, suggesting further considerations of seasonality
(e.g., Visioni et al., 2020) and consideration of what structure is likely
being represented by a DBS<inline-formula><mml:math id="M208" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">BW</mml:mi></mml:msub></mml:math></inline-formula> ridge (e.g., a jet stream, polar vortex or
something much less substantial).</p>
      <p id="d1e3321">Though not investigated in the present research, with the introduction of
stratospheric heating, cross-isentropic flow is likely to occur (e.g.,
vertical uplift from the heating), potentially justifying a
3D analysis for the flows used here. Vertical transport of
aerosol is likely inevitable, but a 3D DBS analysis would exponentially
increase the complexity and the computational costs of finding injection
locations. The currently proposed isentrope method is found to improve
injection protocols at little to no increased operational cost as there are
clear advantages in the short-time dynamics when using the DBS forecasts. One
alternative improvement to 3D DBS fields would be a simultaneous 2D analysis
of structures on a range of isentropes.</p>
      <p id="d1e3325">Several studies have found that the injection rate of SO<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is the
limiting factor in geoengineering efficiency by increasing the coagulation
(Heckendorn et al., 2009; Niemeier et al., 2011; Niemeier and Timmreck,
2015). These studies, however, did not optimize the dispersion of SO<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
during the first days following injection and, therefore, did not maximize
the potential of sulfate injections and consequent radiative forcing in
model simulations. We conclude that the exploitation of readily available,
short-range wind forecasts and reanalysis are a catalyst that will allow
better understanding of what can be achieved with climate geoengineering. It
is possible that one of the reasons the improvements seen here are not more
drastic is the acute focus on the response to large individual injections, which is a
method not commonly used. We ran simulations that included a single day of
injection in an effort to demonstrate dispersion capabilities. As the
ability of DBS ridges to predict dispersion dynamics has now been shown, a
logical next step is to pursue more climate focused studies, such as
injecting less mass over many successive<?pagebreak page8860?> injections using concurrent
predictions. While the use of DBS-informed injections does not address many
of the potential hazards of geoengineering (e.g., Robock et al., 2008;
Heckendorn et al., 2009), it is an important step forward towards assessing
the feasibility of geoengineering to prevent the climate from crossing a
critical tipping point.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e3351">MATLAB code to calculate DBS fields can be found at <uri>https://github.com/haller-group/BarrierTool.git</uri> (last access: 8 December 2020).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3360">The ocean flow data used for Figs. 1 and 2 can be obtained from AVISO (<uri>http://www.aviso.oceanobs.com</uri>, last access: 19 November 2019). All climate data were generated using the open access Community Earth System Model. The model, support, and associated publications can be found at <uri>https://www.cesm.ucar.edu</uri> (last access: 29 October 2018).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3372">NOA, BK, DGM and GH contributed to the writing of this paper and the analysis of results. NOA and GH developed the experiment design and methods. BK performed all CESM2 (WACCM6) model simulations. NOA performed all other tracer and DBS computations.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3378">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3384">The authors would like to express their gratitude to Rolf Müller and the two anonymous referees for their suggestions that improved the paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3389">Support for Ben Kravitz has been provided, in part, by the National Science Foundation (grant no. CBET-1931641), the Indiana University Environmental Resilience Institute, and the “Prepared for Environmental Change” Grand Challenge initiative. The Pacific Northwest National Laboratory is operated for the US Department of Energy by the Battelle Memorial Institute (grant no. DE-AC05-76RL01830). This research has been supported, partly by Lilly Endowment, Inc. through its support for the Indiana University Pervasive Technology Institute and partly by the Indiana Metabolomics and Cytomics Initiative (METACyt). The Indiana METACyt Initiative at Indiana University has also been partly supported by the Lilly Endowment, Inc.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3395">This paper was edited by Rolf Müller and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>Harnessing stratospheric diffusion barriers for enhanced climate geoengineering</article-title-html>
<abstract-html><p>Stratospheric sulfate aerosol geoengineering is a proposed method
to temporarily intervene in the climate system to increase the reflectance of shortwave radiation and reduce mean global temperature. In previous climate modeling studies, choosing injection locations for geoengineering aerosols has, thus far, only utilized the average dynamics of stratospheric wind fields instead of accounting for the essential role of time-varying material transport barriers in turbulent atmospheric flows. Here we conduct the first analysis of sulfate aerosol dispersion in the stratosphere, comparing what is now a standard fixed-injection scheme with time-varying injection locations that harness short-term stratospheric diffusion barriers. We show how diffusive transport barriers can quickly be identified, and we provide an automated injection location selection algorithm using short forecast and reanalysis data. Within the first 7&thinsp;d days of transport, the dynamics-based approach is able to produce particle distributions with greater global coverage than fixed-site methods with fewer injections. Additionally, this enhanced dispersion slows aerosol microphysical growth and can reduce the effective radii of aerosols up to 200–300&thinsp;d after injection. While the long-term dynamics of aerosol dispersion are accurately predicted with transport barriers calculated from short forecasts, the long-term influence on radiative forcing is more difficult to predict and warrants deeper investigation. Statistically significant changes in radiative forcing at timescales beyond the forecasting window showed mixed results, potentially increasing or decreasing forcing after 1 year when compared to fixed injections. We conclude that future feasibility studies of geoengineering should consider the cooling benefits possible by strategically injecting sulfate aerosols at optimized time-varying locations. Our method of utilizing time-varying attracting and repelling structures shows great promise for identifying optimal dispersion locations, and radiative forcing impacts can be improved by considering additional meteorological variables.</p></abstract-html>
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