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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-24-10409-2024</article-id><title-group><article-title>Simulated contrail-processed aviation soot aerosols are poor ice-nucleating particles at cirrus temperatures</article-title><alt-title>Simulated contrail-processed aviation soot aerosols</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Testa</surname><given-names>Baptiste</given-names></name>
          <email>btesta@proton.me</email>
        <ext-link>https://orcid.org/0000-0003-0196-7080</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Durdina</surname><given-names>Lukas</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Edebeli</surname><given-names>Jacinta</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Spirig</surname><given-names>Curdin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9584-1982</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Kanji</surname><given-names>Zamin A.</given-names></name>
          <email>zamin.kanji@env.ethz.ch</email>
        <ext-link>https://orcid.org/0000-0001-8610-3921</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute for Atmospheric and Climate Science, ETH Zürich, Zurich, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Centre for Aviation, ZHAW School of Engineering, Winterthur, Switzerland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Baptiste Testa (btesta@proton.me) and Zamin A. Kanji (zamin.kanji@env.ethz.ch)</corresp></author-notes><pub-date><day>19</day><month>September</month><year>2024</year></pub-date>
      
      <volume>24</volume>
      <issue>18</issue>
      <fpage>10409</fpage><lpage>10424</lpage>
      <history>
        <date date-type="received"><day>17</day><month>January</month><year>2024</year></date>
           <date date-type="rev-request"><day>25</day><month>January</month><year>2024</year></date>
           <date date-type="rev-recd"><day>18</day><month>June</month><year>2024</year></date>
           <date date-type="accepted"><day>16</day><month>July</month><year>2024</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2024 Baptiste Testa et al.</copyright-statement>
        <copyright-year>2024</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/acp-24-10409-2024.html">This article is available from https://acp.copernicus.org/articles/acp-24-10409-2024.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/acp-24-10409-2024.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/acp-24-10409-2024.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e126">Aviation soot surrogates processed in contrails are believed to become potent ice nuclei at cirrus temperatures. This is not verified for real aviation soot, which can have vastly different physico-chemical properties. Here, we sampled soot particles from in-use commercial aircraft engines and quantified the effect of contrail processing on their ice nucleation ability at <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo></mml:mrow></mml:math></inline-formula> 228 K. We show that aviation soot becomes compacted upon contrail processing, but that does not change their ice nucleation ability in contrast to other soot types. The presence of H<inline-formula><mml:math id="M2" 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="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> condensed in soot pores, the highly fused nature of the soot primary particles and their arrangement are what limit the volume of pores generated upon contrail processing, in turn limiting sites for ice nucleation. Furthermore, we hypothesized that contrail-processed aviation soot particles emitted from alternative jet fuel would also be poor ice-nucleating particles if their emission sizes remain small (<inline-formula><mml:math id="M4" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 150 nm).</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Horizon 2020</funding-source>
<award-id>875036</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Bundesamt für Zivilluftfahrt</funding-source>
<award-id>SFLV-2020-080</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e173">Aviation soot particles directly emitted in the upper troposphere at cirrus temperatures have been considered potential ice-nucleating particles (INPs), impacting cirrus cloud properties and hence affecting the Earth radiative budget <xref ref-type="bibr" rid="bib1.bibx33" id="paren.1"/>. However, current aviation soot radiative forcing estimates are associated with large uncertainties, arising mainly from their unconstrained ice nucleation abilities <xref ref-type="bibr" rid="bib1.bibx52" id="paren.2"/>. The ice nucleation properties of real aviation soot have been quantified only recently for the first time, and they suggest a high likelihood of poor ice nucleation ability at cirrus-relevant temperatures (<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>&lt;</mml:mo></mml:mrow></mml:math></inline-formula> 235 K) <xref ref-type="bibr" rid="bib1.bibx53" id="paren.3"/>. This suggests that aviation soot would not perturb the formation of background cirrus clouds and that current radiative forcing estimates need to be updated. Soot particles can also be re-emitted into the upper troposphere via contrails that form in the exhaust wake of aircraft <xref ref-type="bibr" rid="bib1.bibx26" id="paren.4"/>. Once the contrail sublimates, soot residuals inside the contrail ice crystals are released with potentially different properties. Capillary forces arising from water condensed in soot pores <xref ref-type="bibr" rid="bib1.bibx36" id="paren.5"/> may induce the collapse of the soot aggregates <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx3 bib1.bibx11" id="paren.6"/>, promoting the formation of small aggregate voids. Soot residuals from contrails have been shown to enhance ice nucleation of aviation soot proxies <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx20" id="paren.7"/> due to increased porosity upon aggregate compaction, potentially allowing them to compete with background aerosols in cirrus cloud formation. At cirrus temperatures, soot particles nucleate ice via the three-step pore condensation and freezing (PCF) mechanism. First, water vapor condenses into soot pores below water saturation (relative humidity over liquid water (RH<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:math></inline-formula>) <inline-formula><mml:math id="M7" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 100 %), followed by the homogeneous ice nucleation of the pore water, and then there is growth of the ice out of the pore <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx41 bib1.bibx10" id="paren.8"/>. The pore size must be small enough to trigger capillary condensation but larger than the ice germ to allow its nucleation. Pores of relevant diameters for PCF are in the range of 2–30 nm <xref ref-type="bibr" rid="bib1.bibx41" id="paren.9"/> and fall into the mesopore size range of 2–50 nm <xref ref-type="bibr" rid="bib1.bibx21" id="paren.10"/>. Depending on the soot properties (coating, primary particle arrangement), the number of PCF-relevant mesopores in aggregates might increase as a result of compaction, increasing the probability of PCF occurring <xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx17 bib1.bibx61 bib1.bibx44 bib1.bibx39" id="paren.11"/>. <xref ref-type="bibr" rid="bib1.bibx53" id="text.12"/> showed that aviation soot ice nucleation properties are different from the surrogates used in past studies; thus contrail processing from previous studies is likely not representative of aviation soot contrail processing. In this study, we quantify the ice nucleation ability of contrail-processed aviation soot particles sampled from in-use commercial aircraft engines, with an emphasis on their morphological change upon processing. The effect of the aviation soot mixing state on the change in morphology and ice nucleation is also investigated.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Experimental method</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Aviation soot sampling, processing and ice nucleation measurements</title>
      <p id="d1e255">Measurements were conducted at the aircraft engine maintenance and testing facility SR Technics at Zurich Airport. The experimental setup was designed to simulate targeted atmospheric processes and to mimic the contrail processing of the sampled aviation soot particles (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a). Limitations of the ground setup in representing atmospheric processes (e.g., aircraft exhaust evolution, contrail formation) and impacts on the soot ice nucleation ability are discussed in Sect. <xref ref-type="sec" rid="Ch1.S5"/>. Soot particles were sampled from in-use commercial aircraft engines (multiple models from Pratt &amp; Whitney and CFM International) running in an indoor test cell, with air intake at ambient temperature and humidity. The engines were all fueled with Jet A-1 fuel and ran from low to high power (30 %–100 % sea level thrust). The detailed sampling system, which we briefly describe here, is described in more detail in <xref ref-type="bibr" rid="bib1.bibx53" id="text.13"/>. The engine exhaust gas and particles were sampled by a heat-resistant alloy probe <inline-formula><mml:math id="M8" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 m downstream of the engine exhaust nozzle and directed by a long trace-heated line (12 m at 433 K) to a stirred tank, which was in a room next to the engine test cell and acted as an aerosol reservoir where the soot particles accumulated and coagulated (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). The exhaust temperature drops in three steps, from the engine temperature (thousands of kelvins) to the heated line temperature (433 K) and then to room temperature, followed by a third drop from room temperature to the cloud chamber temperature (<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">228</mml:mn></mml:mrow></mml:math></inline-formula> K; see below). Engine emission lasted about 20 min and ice nucleation measurements several hours. The soot size distribution reached in the tank after coagulation was different for each engine owing to the different soot emission indices of the engines tested. The average mode electrical mobility diameter (<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) <inline-formula><mml:math id="M11" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1<inline-formula><mml:math id="M12" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> was 250 <inline-formula><mml:math id="M13" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 50 nm, with minimum and maximum mode diameters of 80 and 450 nm. Contrail processing of the soot particles was conducted following an identical experimental procedure described in, for example, <xref ref-type="bibr" rid="bib1.bibx39" id="text.14"/> and <xref ref-type="bibr" rid="bib1.bibx16" id="text.15"/>. In brief, the polydisperse aerosols were directed from the aerosol reservoir to a first cloud chamber <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx37" id="paren.16"/> set to contrail cloud thermodynamic conditions (<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">228</mml:mn></mml:mrow></mml:math></inline-formula> K and RH<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M16" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 105 %; HINC1 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b), allowing the soot particles to activate and freeze into ice crystals. The sample flow downstream of HINC1 was then directed into a subsaturated flow tube, CATZ (cloud aerosol transitioner Zurich; <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 233 K and RH<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M19" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 56 %), allowing the ice crystals formed in HINC1 to sublimate. At this stage, the sample flow included contrail-processed soot and interstitial soot particles that may not have formed ice in HINC1. Then, contrail-processed and interstitial aerosols were directed into a second cloud chamber (HINC2 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b), whose relative humidity (RH) was varied from ice to liquid water supersaturation. The ratio of aerosol to sheath flow in the cloud chambers was <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula>. The number of soot particles entering HINC2 and ice crystals detected downstream of HINC2 were counted by a scanning mobility particle sizer (SMPS; Electrostatic Classifier 3082, column 3081, CPC 3776 or CPC 3775, TSI Inc., flow mode 0.3 L min<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; SMPS2 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b) and by an optical particle counter (OPC GT-526S, Met One), respectively. The fraction of the soot particles nucleating ice, the activated fraction (AF), is defined as
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M23" display="block"><mml:mrow><mml:mi mathvariant="normal">AF</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">number</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">ice</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">crystals</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">number</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">soot</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">particles</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>

      <fig id="Ch1.F1" specific-use="star"><label>Figure 1</label><caption><p id="d1e465"><bold>(a)</bold> Schematic of the main atmospheric processes associated with aviation soot–cirrus interaction. From left to right: due to the incomplete combustion of aviation fuel, aircraft engines emit soot particles externally and internally mixed with 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> <inline-formula><mml:math id="M25" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> H<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>SO<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and organics (unburned hydrocarbons, oil droplets). Plume particles (mainly soot and H<inline-formula><mml:math id="M28" 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="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>) can activate as cloud droplets and ice crystals <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx58" id="paren.17"/>, forming a contrail cloud due to the high concentration of water vapor and low temperature that can immediately sublimate or persist and subsequently sublimate. The soot ice residuals released upon sublimation are referred to as contrail-processed soot particles. Background aerosol (e.g., dust, solution droplets) and soot can both nucleate ice and form in situ cirrus clouds. <bold>(b)</bold> Experimental setup mimicking the aviation soot atmospheric processes shown in <bold>(a)</bold>. Arrows show the direction of the aerosol flow. See text for details. Abbreviations: CS, catalytic stripper; SMPS, scanning mobility particle sizer; DMA, differential mobility analyzer; CPC, condensation particle counter; HINC, horizontal ice nucleation chamber; TEM, transmission electron microscopy; CATZ, cloud aerosol transitioner Zurich;  OPC, optical particle counter; CPMA, centrifugal particle mass analyzer.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f01.png"/>

        </fig>

      <p id="d1e538">For a part of the experiments, the soot volatile fraction (H<inline-formula><mml:math id="M30" 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="M31" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and organics) was denuded with a catalytic stripper (CS08, Catalytic Instruments; <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">623</mml:mn></mml:mrow></mml:math></inline-formula> K) prior to entering HINC1. In total, four aviation soot populations were studied: unprocessed soot, catalytically stripped soot (CS-soot), contrail-processed soot (CP-soot), and catalytically stripped plus contrail-processed soot (CS-CP-soot). The ice nucleation ability for the unprocessed and CP-soot samples was systematically measured for all engines tested (13 engines in total). The ice nucleation ability of the CS-soot and CS-CP-soot was measured for five engines.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Characterization of aviation soot morphology</title>
      <p id="d1e579">Aviation soot particle morphology was investigated with transmission electron microscopy (TEM) for a few targeted engines. The particles were dried with molecular sieve dryers and collected onto TEM grids (copper formvar <inline-formula><mml:math id="M33" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> carbon, Ted Pella Inc.) with a nanoparticle TEM sampler (Partector TEM, Naneos Particle Solutions GmbH). Unprocessed soot and processed soot (i.e., CS-soot, CP-soot and CS-CP-soot) were collected onto different TEM grids at location TEM1 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b for unprocessed and CS-soot and TEM2 for CP-soot and CS-CP-soot. The Partector TEM sampler uses a soft particle impaction technique (electrostatic precipitation), limiting the effect of the sampling process on the particle morphology. Soot aggregate breaking upon impaction was not observed on the various soot samples. Only clearly isolated soot particles on the grid were imaged to avoid imaging aggregated particles on the grid. Individual soot aggregates were imaged with a JEOL JEM-1400 microscope, and the images processed with the MATLAB (R2020a, MathWorks Inc., Natick, MA, USA) code from <xref ref-type="bibr" rid="bib1.bibx13" id="text.18"/>. The latter was modified to derive the convexity, circularity, aspect ratio, maximal 2D-projected aggregate length (<inline-formula><mml:math id="M34" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>), width (<inline-formula><mml:math id="M35" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula>) and equivalent spherical diameter (<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">eq</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) as described elsewhere <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx7 bib1.bibx8 bib1.bibx39 bib1.bibx53" id="paren.19"/>. In addition, an SMPS (SMPS1 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b) monitored aerosol size distributions upstream of HINC1, allowing comparison of the impact of the various processes on the particle sizes. The particle mass of size-selected unprocessed and CP-soot particles was measured with a centrifugal particle mass analyzer (CPMA; Cambustion Ltd., Cambridge, UK) in tandem with a DMA and CPC similar to  <xref ref-type="bibr" rid="bib1.bibx1" id="text.20"/> and <xref ref-type="bibr" rid="bib1.bibx14" id="text.21"/>. From the mass measurements, information on the morphology of the particles can be extracted. As soot particles are fractal, their mass scales with their diameter following a power law relationship <xref ref-type="bibr" rid="bib1.bibx1" id="paren.22"><named-content content-type="pre">e.g.,</named-content><named-content content-type="post">and references therein</named-content></xref>:
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M37" display="block"><mml:mrow><mml:mi>m</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>C</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi>D</mml:mi><mml:msup><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">fm</mml:mi></mml:msub></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:mspace width="0.33em" linebreak="nobreak"/></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass of the particles with electric mobility diameter <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M40" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is a constant called the mass–mobility prefactor, and <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">fm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass–mobility exponent. The latter is a parameter describing the aggregate morphology, with <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">fm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M43" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 3 for spherical aggregate and <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">fm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M45" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1 for infinite chain-like aggregate. We note that this relation holds for soot particles with constant primary particle sizes. This is not strictly true for aviation soot particles sampled in this study, as shown by the TEM images (see exemplary TEM images in Figs. <xref ref-type="fig" rid="App1.Ch1.S1.F7"/> and <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>). In addition, the relation assumes that the particles were formed in the same environment, which holds in our study since all soot populations underwent similar processes in the combustor and in the aerosol reservoir (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b).</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Ice nucleation measurements</title>
      <p id="d1e787">The ice nucleation onset  (defined as AF <inline-formula><mml:math id="M46" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) of unprocessed and processed aviation soot is summarized in Fig. <xref ref-type="fig" rid="Ch1.F2"/>. Unprocessed aviation soot nucleates ice at or above the RH required for the homogeneous freezing of solution droplets (RH<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>) at 218 and 228 K. CS-soot, on the other hand, nucleates ice at a lower RH compared to unprocessed soot and below RH<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> for a few experiments, giving a larger spread in the onset conditions. Ice nucleation behaviors of unprocessed and CS-soot investigated in <xref ref-type="bibr" rid="bib1.bibx53" id="text.23"/> using the same experimental setup show that aviation soot possesses few mesopores required to trigger PCF; however H<inline-formula><mml:math id="M50" 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="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, present in most samples and thought to be condensed in the soot pores, prevents the freezing of the pore water by lowering its homogeneous ice nucleation rate. Upon stripping, H<inline-formula><mml:math id="M52" 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="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> is largely removed, and the particles can nucleate ice via PCF for a few experiments; for others, the lack of hydrophilic-surface-oxygenated functionalities likely prevented pore filling and subsequent ice nucleation. The overall poor ice nucleation abilities of unprocessed soot and CS-soot were imputed to their limited mesoporosity due to highly overlapping primary particles. CP-soot investigated in the present study also nucleates ice at RH<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> and above at <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">218</mml:mn></mml:mrow></mml:math></inline-formula> and 228 K; i.e., its ice nucleation ability is essentially similar to that of unprocessed soot (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). At 218 K, only 2 out of 13 engines trigger PCF at 5 % RH<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> below RH<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F2"/>, blue outlier scatter points). <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values for the two engines are 350 and 200 nm, compared to the average mode of 250 nm for all experiments. Large soot aggregates have a higher chance of including a cavity that can trigger PCF compared to smaller aggregates due to their higher number of primary particles <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx44 bib1.bibx19" id="paren.24"/>, which explains the higher ice nucleation activity of the 350 nm particle experiment but not that of the 200 nm sample. This implies that aggregate size alone is not a sufficient descriptor to explain the modest ice nucleation ability of the 200 nm diameter soot sample. The CS-CP-soot particles show the lowest median nucleation onset at 7 % and 4 % RH<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> below RH<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> at 218 and 228 K, respectively.</p>

      <fig id="Ch1.F2"><label>Figure 2</label><caption><p id="d1e951">Ice nucleation onset RH<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> range (AF <inline-formula><mml:math id="M62" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) of unprocessed and processed soot at the given temperatures. The boxes extend from the 25th to 75th percentiles, the white bar shows the median, the whiskers include the inter-quartile range and the scatter points show the outlier data points. Panels <bold>(a)</bold> and <bold>(b)</bold> share the same <inline-formula><mml:math id="M64" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis and legend. The dashed black line indicates RH<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx25" id="paren.25"/> and the grey shading its uncertainties in the HINC. The RH<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:math></inline-formula> values are shown by the dashed grey lines in steps of 5 %. The <inline-formula><mml:math id="M67" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis shows the number of measurements conducted per sample type (including different engine types).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Soot morphology</title>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Mass measurements</title>
      <p id="d1e1047">The mass of size-selected unprocessed and CP-soot in the range of 200–400 nm is shown for four engines in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a and in the range of 100–200 nm for the PW4168A engine in Fig. <xref ref-type="fig" rid="Ch1.F3"/>b. Fits to the mass–mobility relation (Eq. <xref ref-type="disp-formula" rid="Ch1.E2"/>) are additionally shown in the figure. The mass–mobility exponent of the unprocessed soot (Fig. <xref ref-type="fig" rid="Ch1.F3"/>a) is smaller than that measured for engine exit plane aviation soot <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx14" id="paren.26"><named-content content-type="pre">about 2.20–2.70 for soot emitted at low to high thrust;</named-content></xref>. This is because the particles sampled in our study undergo coagulation in an aerosol reservoir; as a result, the particles become larger and lacier, which translates to a smaller mass–mobility exponent. This is also visible when comparing images of small and compact uncoagulated particles with unprocessed coagulated soot particles in Figs. <xref ref-type="fig" rid="App1.Ch1.S1.F7"/> and <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>, respectively. As expected, the mass–mobility exponents for the smaller PW4168A soot are higher (<inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">fm</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M69" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.24; Fig. <xref ref-type="fig" rid="Ch1.F3"/>b) and approach values measured for engine exit plane aviation soot. For the engines shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a, the soot aggregate mass increases for given sizes, which we explain by particle densification through its compaction, resulting in a higher mass–mobility exponent. For the smaller PW4168A engine soot particles (<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M71" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 150 nm; Fig. <xref ref-type="fig" rid="Ch1.F3"/>b), we also note a mass change upon contrail processing although this is within the measurement uncertainties. Despite particles passing through the dryer before entering the CPMA, part of the increase in aggregate mass upon contrail processing might be due to water retained in soot aggregates that do not have the time to desorb during the short residence time in the dryer <xref ref-type="bibr" rid="bib1.bibx17" id="paren.27"/>. From our data set, we cannot differentiate between a mass increase from particle restructuring and water taken up, and thus mass–mobility exponents for the CP-soot samples represent higher estimates.</p>

      <fig id="Ch1.F3" specific-use="star"><label>Figure 3</label><caption><p id="d1e1118">Unprocessed and contrail-processed size-selected aggregate mass mode (<inline-formula><mml:math id="M72" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>) as a function of its electric mobility diameter (<inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) for <bold>(a)</bold> the CFM56-7B26/3, CFM56-5B4/P, CFM56-7B27/3 and CFM56-7B24/3 engines and <bold>(b)</bold> the PW4168A engine. Lines show fits to Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>) with retrieved parameters shown in the boxes. Uncertainties in the parameters are shown in parentheses. Panel <bold>(b)</bold> shares its legend with panel <bold>(a)</bold>.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f03.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Size measurements</title>
      <p id="d1e1169">Differences in <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> between unprocessed and processed soot (<inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) are shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/> for the PW4168A, CFM56-7B26 and PW4062A-3 engines. <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values are derived from a lognormal fit to the size distribution measured by the first SMPS (SMPS1 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b) for unprocessed soot, monitoring soot aggregate size change due to coagulation in the aerosol reservoir, and from the second SMPS (SMPS2 in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b), measuring unprocessed and processed soot sizes in parallel with the ice nucleation measurements. Both SMPSs have been calibrated against a reference SMPS. The CS-soot size is essentially similar to the unprocessed soot size (<inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> within measurement uncertainties) for all engines. For CP-soot and CS-CP-soot, <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is decreased for all engines, but it is within measurement uncertainties for the PW4168A engine. We note that although the difference remains within measurement uncertainties, <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is consistently larger for CP-soot compared to CS-CP-soot (as confirmed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS3"/>). This would be expected as soot particles become more hydrophobic upon catalytic stripping and are hence less sensitive to compaction upon contrail processing (discussed further in Sect. <xref ref-type="sec" rid="Ch1.S4"/>).</p>

      <fig id="Ch1.F4" specific-use="star"><label>Figure 4</label><caption><p id="d1e1263">Mode diameter change <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> upon processing of the particles as measured by SMPS1 and SMPS2 (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b) for the given engines.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f04.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Shape analysis from TEM</title>
      <p id="d1e1296">The shape analysis from the TEM images is shown for three engines in Fig. <xref ref-type="fig" rid="Ch1.F5"/>. As expected, for both unprocessed and contrail-processed particles, the convexity increases with decreasing <inline-formula><mml:math id="M81" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>, meaning that smaller soot aggregates are more compact than larger ones. Overall, contrail processing induces a strong increase in convexity and reduction in the <inline-formula><mml:math id="M82" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> of the soot particles for all engine types investigated, which is indicative of aggregate compaction <xref ref-type="bibr" rid="bib1.bibx9" id="paren.28"/> (exemplary TEM images are shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>). The convexity of the CP-soot does not seem to be correlated with the unprocessed soot size; i.e., median <inline-formula><mml:math id="M83" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> values for the unprocessed samples of the investigated engines are 190, 515 and 689 nm, resulting in particle convexity after contrail processing of 0.81, 0.81 and 0.78 (boxplots in Fig. <xref ref-type="fig" rid="Ch1.F5"/>a–c, respectively). This means that, on average, the soot particles become similarly compacted regardless of their initial sizes. This also indicates that the relative increase in compaction is stronger for initially larger aggregates, which are lacier. For instance, the convexity increased by 60 % for 689 nm (median <inline-formula><mml:math id="M84" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>) sized PW4062A-3 soot and by 10 % for 190 nm sized PW4168A soot. We note that the size reductions measured by the SMPS are smaller than those measured from the TEM images. A strict comparison with the TEM measurements is neither possible nor expected because of the different assumptions in electrical mobility sizing and the 2D images used for TEM sizing. Nonetheless, the TEM analysis overall corroborates the size and mass measurements (Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/> and <xref ref-type="sec" rid="Ch1.S3.SS2.SSS2"/>). Upon contrail processing, the aggregate mass at given sizes increases. This, together with a decrease in particle size as revealed by SMPS and TEM images, indicates an increase in particle density caused by the compaction of the aggregates, which become less hollow. CS-soot convexity and <inline-formula><mml:math id="M85" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> (boxplots in Fig. <xref ref-type="fig" rid="Ch1.F5"/>a–c) are similar to unprocessed soot; i.e., the morphology does not change upon stripping. For the three engines investigated, CS-CP-soot shows morphology changes that are similar to CP-soot, i.e., a decrease in <inline-formula><mml:math id="M86" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> and increase in convexity in comparison to the unprocessed soot. However the CS-CP-soot undergoes a smaller size reduction than the CP-soot (see also SMPS measurements in Fig. <xref ref-type="fig" rid="Ch1.F4"/>) and is slightly less convex (most pronounced for the PW4062A-3 engine). Soot aggregates activated in the contrail chamber undergo similar compaction. However, aggregates that did not activate as ice crystals in the chamber (about 80 % at 105 % RH<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">w</mml:mi></mml:msub></mml:math></inline-formula> for both PW4062A-3 CP-soot and CS-CP-soot; Fig. <xref ref-type="fig" rid="Ch1.F6"/>c) might still undergo hygroscopic growth, depending on their hydrophilicity, leading to their partial collapse <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx39" id="paren.29"/>. Ice crystal soot residuals and interstitial soot were both imaged with TEM. The lower convexity and size reduction for CS-CP-soot compared to CP-soot indicate that interstitial CS-CP-soot is less compacted than interstitial CP-soot and that CS-CP-soot is on average more hydrophobic. This is due to the removal of H<inline-formula><mml:math id="M88" 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="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> upon catalytic stripping of the particles <xref ref-type="bibr" rid="bib1.bibx53" id="paren.30"/>. The weaker morphological change for the PW4062A-3 CS-CP-soot could be imputed to a lower content of surface polar groups or higher surface graphitization <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx51" id="paren.31"/> compared to the other engines investigated, which resulted in its lower convexity.</p>

      <fig id="Ch1.F5" specific-use="star"><label>Figure 5</label><caption><p id="d1e1401">Maximum 2D-projected length (<inline-formula><mml:math id="M90" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>) and convexity of unprocessed and processed aviation soot aggregates analyzed from TEM images for three engines. Convexity and <inline-formula><mml:math id="M91" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> distributions are shown for all soot populations in the boxplots (box statistics are as in Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and the density contours in the larger plots only for unprocessed and CP-soot for clarity. The colored areas enclose – from dark to light – about 25 %, 50 %, 75 % and 95 % of the images (one aggregate per image). The number of images analyzed is shown on the <inline-formula><mml:math id="M92" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis below the boxplots. Panel <bold>(a)</bold> shares its legend with panels <bold>(b)</bold> and <bold>(c)</bold>.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f05.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e1453">The inability of CP-soot to promote ice nucleation at RH <inline-formula><mml:math id="M93" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> RH<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) indicates that contrail processing does not generate pores relevant to PCF despite compaction of the soot particles as revealed with imaging, size distributions and size-resolved particle mass measurements. <xref ref-type="bibr" rid="bib1.bibx16" id="text.32"/> observed moderate ice nucleation enhancement for contrail-processed 200 nm propane soot coated with H<inline-formula><mml:math id="M95" 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="M96" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> compared to unprocessed coated soot. The authors explain this by the presence of H<inline-formula><mml:math id="M97" 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="M98" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> condensed in pores and that is redistributed over the newly formed pore network upon compaction, hence limiting the ice nucleation of the pore water. The same argument might explain the inability of contrail-processed aviation soot to promote ice nucleation via PCF. CP-soot ice nucleation AF values for three engines are shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/> (the associated soot size distributions are shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S2.F9"/>), and all have their onsets at RH<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>. We note a small ice nucleation enhancement for the CFM56-7B26 engine after contrail processing that we attribute to the low soot sulfur content for this engine <xref ref-type="bibr" rid="bib1.bibx53" id="paren.33"><named-content content-type="pre">0.02 at. % measured with TEM X-ray spectroscopy;</named-content></xref>.</p>

      <fig id="Ch1.F6" specific-use="star"><label>Figure 6</label><caption><p id="d1e1535">AF ice nucleation curves as a function of RH at 218 K for the given engines. The dashed black line and grey shading indicate RH<inline-formula><mml:math id="M100" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> and associated uncertainties. Panel <bold>(a)</bold> shares its legend with panels <bold>(b)</bold> and <bold>(c)</bold>.</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f06.png"/>

      </fig>

      <p id="d1e1562">As mentioned above, the ice nucleation enhancement upon catalytic stripping (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) is attributed to the removal of H<inline-formula><mml:math id="M101" 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="M102" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> (and organics) condensed in pores while stripping, emptying existing mesopores that become available for water condensation and ice nucleation <xref ref-type="bibr" rid="bib1.bibx53" id="paren.34"/>. Yet, the ice nucleation response to stripping varies between the three engines investigated in Fig. <xref ref-type="fig" rid="Ch1.F6"/>. For the PW4062A-3 soot sample, stripping does not change the ice nucleation AF, presumably due to its hydrophobic surface indicated by the weak morphological change in the corresponding CS-CP-soot sample (convexity <inline-formula><mml:math id="M103" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.64; Fig. <xref ref-type="fig" rid="Ch1.F5"/>c). CS-soot from the PW4168A and CFM56-7B26 engines triggers ice nucleation at a lower RH compared to unprocessed soot, and it is clearly below RH<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula> only for PW4168A. Better soot water uptake capacity for those engines would corroborate their ice nucleation abilities. Differences in primary particle arrangement and overlap could also contribute to the small difference in ice nucleation between CS-soot from the PW4168A engine and that from the CFM56-7B26 engine (exemplary images shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>). A more detailed analysis of primary particle sizes and overlap would be needed to quantify the effect of morphology.</p>
      <p id="d1e1612">For the CS-CP-soot (Fig. <xref ref-type="fig" rid="Ch1.F2"/>), the aggregate compaction upon contrail processing would have increased the number of empty and therefore PCF-relevant mesopores due to formation of new cavities between the soot primary particles <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx19" id="paren.35"/>. Nonetheless, the ice nucleation onset of the CS-CP-soot is close to RH<inline-formula><mml:math id="M105" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>, and these soot particles remain much weaker INPs than soot used as aviation surrogates <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx38 bib1.bibx19 bib1.bibx16" id="paren.36"/> despite similar or stronger compaction of aviation soot <xref ref-type="bibr" rid="bib1.bibx39" id="paren.37"><named-content content-type="pre">median circularity is 0.25 in</named-content><named-content content-type="post">and 0.39 in this study; Table <xref ref-type="table" rid="App1.Ch1.S1.T1"/></named-content></xref>. For PCF to be triggered by soot, the particles need to possess cavities with the right size and shape. Such cavities should be found for soot primary particle diameters (<inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">pp</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of 10 to 30 nm with moderate overlaps <xref ref-type="bibr" rid="bib1.bibx41" id="paren.38"/>. Smaller primary particles need to be close to being in point contact to give rise to cavities that can accommodate the ice germ, and larger primary particles need to strongly overlap to give rise to small enough cavities that can be filled below water saturation. However, at any diameter, the cavities close if primary particles are too fused, inhibiting PCF. Images of the soot particles sampled in this study (Figs. <xref ref-type="fig" rid="App1.Ch1.S1.F7"/> and <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>) reveal that the primary particles are highly fused (strong overlap) and that <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">pp</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ranges from 10 to 90 nm in a single aggregate. This explains why the CS-CP-soot has limited ice nucleation ability upon compaction. Small primary particles might fill the cavities formed between larger ones, reducing the potential for pore volume generation. A combination of the highly fused nature of primary particles and the large <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">pp</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> range together with poor water uptake capacity at low RH <xref ref-type="bibr" rid="bib1.bibx53" id="paren.39"/> contributes to the overall weak ice nucleation abilities of the CS-CP-soot. Nonetheless, contrail processing of the CS-soot leads to a different response, as shown by the large spread of ice nucleation onset values (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and by the AF curves shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>. CS-CP-soot particles from the PW4062A-3 engine are unable to promote PCF despite their large sizes (Figs. <xref ref-type="fig" rid="Ch1.F5"/>c and <xref ref-type="fig" rid="App1.Ch1.S2.F9"/>c). We attribute this to their poor water affinity and moderate compaction (convexity <inline-formula><mml:math id="M109" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.64). In contrast, both PW4168A and CFM56-7B26 CS-CP-soot are similarly compacted (convexity about 0.79). However, only soot from the latter promotes clear PCF. For the PW4168A engine, CS-CP-soot essentially nucleates ice that is similar to its CS-soot sample. The small number of primary particles per aggregate due to small aggregate sizes (median <inline-formula><mml:math id="M110" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M111" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 190 nm) may limit the number of mesopores generated upon contrail processing. CFM56-7B26 soot aggregates are twice the size on average, giving rise to a higher probability of generating cavities and inter-aggregate voids relevant to PCF upon compaction.</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Atmospheric implications and limitations</title>
      <p id="d1e1727">Recent measurements <xref ref-type="bibr" rid="bib1.bibx53" id="paren.40"/> have shown that aviation soot is unlikely to promote ice nucleation below conditions required for the homogeneous freezing of solution droplets (RH<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>), particularly because the sizes of emitted soot particles are below 100 nm, and particles of this size have been shown to be poor INPs in all conditions (for a variety of mixing states and particle morphologies). Here, we show that contrail-processed aircraft turbine engine soot particles (not proxies) remain poor INPs at 218 and 228 K despite strong compaction of the particles upon contrail processing, thought at first to be the reason for ice nucleation enhancement. This supports the results from <xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx30" id="text.41"/>, who estimated that only a small fraction of aviation soot nucleates ice in cirrus atmospheric conditions, leaving cirrus cloud properties essentially unperturbed. Due to constraints on the measurement facility in this work, the representation of aircraft exhaust processes in the ground setup and hence of the aviation soot properties might differ from that at flight altitude. For instance, differences in equilibrium temperatures and dilution would impact the partitioning of volatile unburned hydrocarbons and sulfur compounds and hence the soot ice nucleation ability. The higher temperatures in our setup (433 K and then room temperature; Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/>) compared to upper tropospheric temperature <xref ref-type="bibr" rid="bib1.bibx31" id="paren.42"><named-content content-type="pre"><inline-formula><mml:math id="M113" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 228 K;</named-content></xref> would not promote the condensation of volatiles onto soot as much as would occur at flight altitude temperatures. The interaction of nucleation-mode particles with aviation soot in the young aircraft plume downstream of the engine is thought to increase the soot coating <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx60 bib1.bibx28" id="paren.43"/>, but it does not occur in our ground setup due to the absence of nucleation-mode particles. Thus, soot particles in this study are expected to have a lower amount of coating from this effect. On the other hand, the total particle surface area was less in our ground setup due to the absence of the nucleation-mode particles, and the exhaust gases experienced reduced dilution in the aerosol reservoir with synthetic air, compared to the strong dilution that would occur within the first seconds at flight altitudes <xref ref-type="bibr" rid="bib1.bibx28" id="paren.44"/>. This effect would enhance the condensation of volatiles onto the soot particles in our ground setup. However, even if lower quantities of organics and sulfate were to condense onto the soot particles in the atmosphere, these would first condense into the pores of the soot, due to the capillary effect, and thus inhibit ice nucleation of the soot particles. Thus, our conclusions of the poor ice-nucleating ability of contrail-processed soot would remain the same. Downstream of HINC1, the re-emitted soot aggregates are compacted due to contrail processing and their sizes decrease. We note that, the convexity and size change in the contrail-processed aviation soot sample from this study is very similar to what has been measured for other cloud- and contrail-processed soot types <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx9 bib1.bibx39" id="paren.45"/>. This is explained by the harsh activation process that occurs in HINC1 and CATZ <xref ref-type="bibr" rid="bib1.bibx11" id="paren.46"><named-content content-type="pre">activation in cloud droplets and ice crystals followed by sublimation;</named-content></xref>. Although large compaction was observed in our study (convexity approaching 1), we do not rule out the possibility of a smaller condensation/sublimation rate in the atmosphere leading to larger compaction of the particles. The formation of large soot aggregates <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx48" id="paren.47"/> due to the coagulation between ice crystals and scavenging of interstitial soot aggregates was not possible due to the low concentration of ice crystals and soot and non-turbulent flow in HINC1. Due to the absence of nucleation-mode particles, coagulation of these with ice crystals and with interstitial soot aggregates was not possible in HINC1. However, the absence of these processes does not change our conclusions because adding more organics onto the soot particles would only further result in poor-ice-nucleation activity <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx16" id="paren.48"/>. Gas-phase chemistry and particle oxidation are thought to considerably slow down while particles exit the combustor chamber due to much lower temperatures in the exhaust nozzle and downstream of the engine <xref ref-type="bibr" rid="bib1.bibx59 bib1.bibx12" id="paren.49"/>. Such a drop in temperature was also present in our sampling system (1000 K to 433 K to room temperature); thus the primary particle overlap, size, crystallinity and oxidation should be unaffected and comparable to aviation soot particles emitted in situ. To summarize, soot particles in our ground setup were larger and less dense than in situ soot due to coagulation in our aerosol reservoir. We believe the aggregate compaction in this work is atmospherically relevant as the parameters driving the soot compaction, i.e., RH<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> experienced by the particles and bulk water condensation, were represented in our ground setup. The primary particle properties and oxidation are fixed in the combustor and hence should be representative of their in situ counterparts. Finally, we expect in situ particles to be coated with H<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>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> and organics, but the extent to which the coating of the aviation soot sample in our study is different from in situ aviation soot cannot be established from our study. For this reason, we quantified the ice nucleation ability of coating-free (CS-CP-soot) and coated (unprocessed and CP-soot) soot in our study to constrain the possible effect of different soot mixing states on aviation soot ice nucleation.</p>
      <p id="d1e1810">Aviation soot samples that were catalytically stripped and contrail-processed were able to nucleate ice at around 145 % RH<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> at 218 K (<inline-formula><mml:math id="M118" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 7 % lower than RH<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>). The modest ice nucleation ability for the CS-CP-soot likely arises from increased cavity numbers and sizes within the soot aggregates, which would have been absent in the unprocessed soot samples coated with organics and sulfate. We note that, if glassy organic coatings formed on the contrail-processed (and unprocessed) soot particles, these particles may have formed ice by deposition nucleation <xref ref-type="bibr" rid="bib1.bibx24" id="paren.50"/>, which was not observed due to the high ice nucleation onset above RH<inline-formula><mml:math id="M120" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>. Thicker coatings for flight altitude aviation soot compared to our CP-soot would favor homogeneous nucleation, and thinner coatings would be bound by the ice nucleation ability of our CS-CP-soot sample. Nevertheless, as long as aviation soot is co-emitted with H<inline-formula><mml:math id="M121" 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="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, it is likely to acquire a coating upon emission and further in the exhaust plume <xref ref-type="bibr" rid="bib1.bibx28" id="paren.51"/>; thus we expect our unprocessed and CP-soot samples to be of higher atmospheric relevance to the engines and fuel currently in use.</p>
      <p id="d1e1872">Additionally, we show that aggregate size does not predominantly regulate the ice nucleation of contrail-processed aviation soot, but rather the differences in H<inline-formula><mml:math id="M123" 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="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> coating and primary particle properties do. Even though large aggregates do not necessarily promote PCF upon contrail processing, we stress that very small aggregates can nonetheless inhibit PCF. The PW4168A experiment presented soot with the smallest sizes among our experiments (<inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M126" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 150 nm), which shows that the effect of contrail processing on the ice nucleation ability remains limited. PW4168A soot is compacted upon contrail processing (convexity <inline-formula><mml:math id="M127" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.8), but, due to their small sizes, the aggregates possess too few primary particles to generate PCF-relevant pores upon compaction. Furthermore, we emphasize that relevant sizes for aviation soot are much smaller (only 0.2 %–2 % of particles are larger than 150 nm; Fig. <xref ref-type="fig" rid="App1.Ch1.S2.F9"/>); we thus expect contrail processing to be further limited for aviation soot emitted in situ like it was for our PW4168A sample.</p>
      <p id="d1e1922">The number and size of cavities within the soot aggregates are the primary controlling factors of soot ice nucleation via PCF (Sect. <xref ref-type="sec" rid="Ch1.S1"/>). Cavity formation is controlled by the primary particle morphology (which is determined in the engine combustor and therefore well simulated in our ground setup) and the aggregates' size. High overlap of the primary particles has been observed on soot samples for all tested engines. A smaller aggregate size for aviation soot is expected for turbofan engines; hence we believe that the results from our study, that is, aviation soot particles are poor ice-nucleating particles for cirrus formation, can be generalized to soot emitted with the current aircraft fleet and fuel <xref ref-type="bibr" rid="bib1.bibx23 bib1.bibx49" id="paren.52"><named-content content-type="pre">Jet A/Jet A-1; <inline-formula><mml:math id="M128" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 90 % of global usage;</named-content></xref>.</p>
      <p id="d1e1940">In addition to contrail processing, several soot aging processes can occur in the atmosphere, such as interaction with background aerosols and volatile compounds or oxidation of aerosols by O<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and OH radicals <xref ref-type="bibr" rid="bib1.bibx4" id="paren.53"/>. Interception of soluble aerosol onto the soot surface would increase the amount of soot coating preventing PCF. Exposure of aviation soot to O<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> or OH at flight altitude can cause condensed organics to desorb due to the breaking of covalent bonds with the elemental soot fraction. The oxidized organics could recondense onto the soot due to their lowered volatility, e.g., short alkanes and aldehyde that are soluble in acidic solution <xref ref-type="bibr" rid="bib1.bibx60" id="paren.54"><named-content content-type="pre">e.g., H<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>2SO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> solution;</named-content></xref>, and could lead to a freezing point depression if condensed in pores or prevent water uptake by blocking the pores if they are hydrophobic, inhibiting PCF <xref ref-type="bibr" rid="bib1.bibx18" id="paren.55"/>. Nevertheless, we do not rule out the possibility of the oxidation of soot surface organics also leading to glassy coatings and promoting deposition ice nucleation of the particles <xref ref-type="bibr" rid="bib1.bibx54" id="paren.56"/>.</p>
      <p id="d1e1994">Additionally, the presence of other potent atmospheric INPs would further limit the effect of aviation soot on cirrus cloud microphysical properties. For instance, we note that the CS-CP-soot RH<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> onset remains substantially above that for mineral desert dust, e.g., about 120 % <xref ref-type="bibr" rid="bib1.bibx56" id="paren.57"/>, which outcompete soot ice nucleation.</p>
      <p id="d1e2009">An unknown for the near future is the use of alternative aviation fuel <xref ref-type="bibr" rid="bib1.bibx26" id="paren.58"/>, mainly synthetic fuel and biofuel, used as pure fuel or blended with jet fossil fuel <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx58" id="paren.59"/>. Pure synthetic fuel and biofuel are free of sulfur and aromatics <xref ref-type="bibr" rid="bib1.bibx5" id="paren.60"/>; hence soot emitted from pure alternative fuel or from alternative fuel blended with jet fossil fuel will have different properties than jet fossil fuel soot, therefore affecting its ice nucleation abilities. Changes in soot morphology and nanostructure have been suggested for different types of alternative fuel <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx34 bib1.bibx22 bib1.bibx57" id="paren.61"/>. <xref ref-type="bibr" rid="bib1.bibx34" id="text.62"/> found alternative fuel soot to be generally more graphitized <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx50" id="paren.63"><named-content content-type="pre">i.e., more hydrophobic;</named-content></xref> than Jet A-1 fuel soot. The same authors also observed blended fuel soot associated with an amorphous organic outer shell, potentially increasing or decreasing the soot water uptake capacity depending on the nature of the organics. On the contrary, <xref ref-type="bibr" rid="bib1.bibx55" id="text.64"/> found no change in particle hydrophilicity at cruise thrust between conventional and alternative fuel. Although more such studies would be needed to be quantify the properties of alternative fuel soot, the ice nucleation abilities of sulfur-free aviation soot can be hypothesized from our study. Those might correspond to our CS-CP-soot sample, which is free of sulfur and organics as discussed above and which exhibits moderate ice nucleation ability, particularly in comparison to mineral dust. We note that aviation soot particles emitted from alternative fuel are thought to be smaller on average and emitted at lower concentrations at all sizes <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx42 bib1.bibx43 bib1.bibx34 bib1.bibx35" id="paren.65"/>. We expect both properties to further limit their effect on cirrus clouds.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e2047">This study presents ice nucleation measurements and morphology analysis of polydisperse aviation soot particles sampled from in-use commercial aircraft engines, with a focus on the effect of contrail processing on aviation soot ice nucleation ability. The effect of coating on the ice nucleation ability and morphology of contrail-processed soot was investigated by catalytically stripping the particles at 623 K, removing volatile organics and sulfur. The ice nucleation ability of unprocessed and processed particles was assessed with a continuous-flow diffusion chamber operated at temperatures relevant to cirrus cloud formation (<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>≤</mml:mo></mml:mrow></mml:math></inline-formula> 228 K) and varying RH<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:math></inline-formula> (110 %–170 %). Particle morphology was investigated with electron microscopy, aerosol sizing and mass measurements. The measurements reveal that contrail-processed aviation soot particles are poor INPs, forming ice at RH levels required for homogeneous freezing of solution droplets (RH<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>) despite contrail processing inducing strong compaction of the soot aggregate (i.e., aggregate convexity increased up to 65 % and maximal aggregate length decreased similarly). Results for the catalytically stripped and catalytically stripped plus contrail-processed soot suggest that the presence of H<inline-formula><mml:math id="M137" 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="M138" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> and organics condensed in the soot aggregate cavities prevents the particles from promoting ice nucleation via PCF. After catalytic stripping, large aviation soot aggregates are able to promote PCF, likely due to the formation of new aggregate cavities and voids upon compaction, but still require RH close to RH<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">hom</mml:mi></mml:msub></mml:math></inline-formula>. Limited ice nucleation enhancement for catalytically stripped contrail-processed aggregate is likely due to the soot primary particles being highly fused and their large size range over single aggregate, hence limiting the generation of large cavities upon compaction. Analysis from microscopy images shows that aggregates as small as 150 nm in mode diameter (corresponding to 0.2 %–2 % of the atmosphere-relevant aviation soot size distribution) are compacted upon contrail processing but that contrail processing remains inefficient in promoting PCF for the catalytically stripped particles due to their small sizes. Overall, our results suggest that aviation soot particles would likely not serve as INPs for cirrus formation and that current radiative forcing estimates <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx52" id="paren.66"/> should be updated. Extrapolation of our results to soot emitted from alternative jet fuel also suggests that their ice nucleation activity will likely remain negligible. Other effects of alternative jet fuel or new engine design on contrail formation such as a lower soot emission index remain, however, unquantified.</p>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <label>Appendix A</label><title>TEM images of unprocessed and contrail-processed aviation soot particles</title>

      <fig id="App1.Ch1.S1.F7"><label>Figure A1</label><caption><p id="d1e2122">TEM images of soot aggregates collected downstream of the test cell and undergoing no coagulation. The blue lines on two of the images highlight the length of identifiable primary particles. Regions highlighted with dashed white rectangles show fused primary particles. Note the different scale bars in the images.</p></caption>
        
        <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f07.png"/>

      </fig>

<fig id="App1.Ch1.S1.F8"><label>Figure A2</label><caption><p id="d1e2136">TEM images of unprocessed and contrail-processed soot aggregates for the given engines. Note the different scale bars in the images.</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f08.jpg"/>

      </fig>

      <p id="d1e2146">Aviation soot samples were collected for different engine types and imaged with TEM. In Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F7"/>, exemplary images are shown for particles collected downstream of the test cell similar to <xref ref-type="bibr" rid="bib1.bibx53" id="text.67"/>. Those aggregates undergo no coagulation and presumably no morphological change before sampling. The lengths of primary particles that are unambiguously identifiable are indicated for two images in the figure. The primary particle diameters range from 17 to 64 nm for those images with features close to 100 nm that could correspond to several fused primary particles. Exemplary images of unprocessed and contrail-processed soot aggregates for three engine types are shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F8"/>. Median shape parameters retrieved from the TEM images of unprocessed and processed aggregates are shown in Table <xref ref-type="table" rid="App1.Ch1.S1.T1"/>.</p>

<table-wrap id="App1.Ch1.S1.T1"><label>Table A1</label><caption><p id="d1e2162">Aviation soot shape parameters derived from TEM images for unprocessed and processed particles. Numbers represent median values for four engine types (CFM56-7B26/3, CFM56-7B26, PW4168A and PW4062A-3). The standard deviation (1<inline-formula><mml:math id="M140" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) is shown in parentheses. <inline-formula><mml:math id="M141" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> is the 2D-projected maximal aggregate length, <inline-formula><mml:math id="M142" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> is the 2D-projected aggregate width and <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">eq</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the 2D-projected equivalent spherical diameter.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Soot sample</oasis:entry>
         <oasis:entry colname="col2">Convexity</oasis:entry>
         <oasis:entry colname="col3">Circularity</oasis:entry>
         <oasis:entry colname="col4">Aspect ratio</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M144" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> (nm)</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M145" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> (nm)</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:mi>D</mml:mi><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">D</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">eq</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (nm)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Unprocessed</oasis:entry>
         <oasis:entry colname="col2">0.61 (0.09)</oasis:entry>
         <oasis:entry colname="col3">0.22 (0.04)</oasis:entry>
         <oasis:entry colname="col4">1.51 (0.05)</oasis:entry>
         <oasis:entry colname="col5">490 (179)</oasis:entry>
         <oasis:entry colname="col6">330 (119)</oasis:entry>
         <oasis:entry colname="col7">283 (81)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CS-soot</oasis:entry>
         <oasis:entry colname="col2">0.6 (0.09)</oasis:entry>
         <oasis:entry colname="col3">0.22 (0.04)</oasis:entry>
         <oasis:entry colname="col4">1.45 (0.05)</oasis:entry>
         <oasis:entry colname="col5">509 (170)</oasis:entry>
         <oasis:entry colname="col6">365 (113)</oasis:entry>
         <oasis:entry colname="col7">296 (84)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CP-soot</oasis:entry>
         <oasis:entry colname="col2">0.8 (0.04)</oasis:entry>
         <oasis:entry colname="col3">0.39 (0.03)</oasis:entry>
         <oasis:entry colname="col4">1.34 (0.04)</oasis:entry>
         <oasis:entry colname="col5">257 (100)</oasis:entry>
         <oasis:entry colname="col6">194 (77)</oasis:entry>
         <oasis:entry colname="col7">183 (67)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CS-CP-soot</oasis:entry>
         <oasis:entry colname="col2">0.78 (0.07)</oasis:entry>
         <oasis:entry colname="col3">0.37 (0.06)</oasis:entry>
         <oasis:entry colname="col4">1.35 (0.03)</oasis:entry>
         <oasis:entry colname="col5">302 (86)</oasis:entry>
         <oasis:entry colname="col6">229 (70)</oasis:entry>
         <oasis:entry colname="col7">209 (55)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup>

</oasis:table></table-wrap>


</app>

<app id="App1.Ch1.S2">
  <label>Appendix B</label><title>Aviation soot size distributions</title>
      <p id="d1e2401">Figure <xref ref-type="fig" rid="App1.Ch1.S2.F9"/> shows soot size distributions from the PW4168A, CFM56-7B26 and PW4062A-3 engines (measured with SMPS2 as shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). Aviation soot particles measured in situ <xref ref-type="bibr" rid="bib1.bibx43" id="paren.68"><named-content content-type="pre">CFM56-2-C1 engine fueled with Jet A-1 fuel at medium thrust;</named-content></xref> and at ground level <xref ref-type="bibr" rid="bib1.bibx15" id="paren.69"><named-content content-type="pre">CFM56-7B26 engine fueled with Jet A-1 fuel at 50 %–65 % sea level thrust;</named-content></xref> are shown for comparison. Coagulated particles sampled in this study present narrow size distributions and are shifted to larger sizes compared to uncoagulated particles. Considering that the larger particles nucleate ice at the lowest RH, the largest 0.1 % of soot particles likely contributes to the ice nucleation onsets discussed in the main text (Figs. <xref ref-type="fig" rid="Ch1.F2"/> and <xref ref-type="fig" rid="Ch1.F6"/>). The cumulative fraction distributions reveal that the largest 0.1 % of aerosols in our experiments is considerably larger than the majority of aviation soot sizes measured by <xref ref-type="bibr" rid="bib1.bibx43" id="text.70"/> and <xref ref-type="bibr" rid="bib1.bibx15" id="text.71"/>. The largest 0.1 % of particles for both the CFM56-7B26 and the PW4062A-3 engines is <inline-formula><mml:math id="M147" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 900 nm, and it is <inline-formula><mml:math id="M148" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 450 nm for the PW4168A engine. As a comparison, the largest 0.1 % of in situ aviation soot is <inline-formula><mml:math id="M149" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 200–300 nm. </p>

      <fig id="App1.Ch1.S2.F9"><label>Figure B1</label><caption><p id="d1e2453"><bold>(a–c)</bold> Normalized aviation soot size distributions of unprocessed and processed particles for three engine types. Aviation soot size distributions measured in situ <xref ref-type="bibr" rid="bib1.bibx43" id="paren.72"/> and at ground level <xref ref-type="bibr" rid="bib1.bibx15" id="paren.73"/> are shown for comparison. The same size distributions are shown as cumulative fractions in <bold>(d)</bold>–<bold>(f)</bold>.</p></caption>
        
        <graphic xlink:href="https://acp.copernicus.org/articles/24/10409/2024/acp-24-10409-2024-f09.png"/>

      </fig>


</app>
  </app-group><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e2484">The code used for image analysis in this work was obtained from Dastanpour and Rogak (2014) and modified for the work presented here. The code is available at <ext-link xlink:href="https://doi.org/10.3929/ethz-b-000694152" ext-link-type="DOI">10.3929/ethz-b-000694152</ext-link> (Testa et al., 2024c).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e2493">The data for the figures in this work are available at  <ext-link xlink:href="https://doi.org/10.3929/ethz-b-000649178" ext-link-type="DOI">10.3929/ethz-b-000649178</ext-link> (Testa et al., 2024b).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2502">The experiments were designed by BT and ZAK with help from LD, JE and CS. BT conducted the experiments and performed the data analysis. BT wrote the first draft, and all authors contributed to data interpretation and writing of the manuscript. ZAK supervised the study, conceived the idea and obtained funding.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2508">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e2514">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2520">The work has been supported by the European Commission via their Horizon 2020 research and innovation program under grant no. 875036 (ACACIA project) and the Swiss Federal Office of Civil Aviation, SFLV-2020-080. The authors would like to thank the engine operators of the SR Technics facility for their help and support. We are also grateful to Fabian Mahrt from the Laboratory of Atmospheric Chemistry (PSI) for helpful discussion of the data. We thank Sotiris E. Pratsinis from the Department of Mechanical and Process Engineering (ETH) for lending us a CPC during our measurement campaign and Markus Ammann from the Laboratory of Atmospheric Chemistry (PSI) for lending us the Partector TEM sampler.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2526">This research has been supported by EU Horizon 2020 (grant no. 875036) and the Bundesamt für Zivilluftfahrt (grant no. SFLV-2020-080).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2532">This paper was edited by Ari Laaksonen and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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