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  <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-18-6585-2018</article-id><title-group><article-title>Meteorological controls on atmospheric particulate pollution during hazard
reduction burns</article-title><alt-title>Meteorological controls on atmospheric particulate pollution</alt-title>
      </title-group><?xmltex \runningtitle{Meteorological controls on atmospheric particulate pollution}?><?xmltex \runningauthor{G. Di~Virgilio et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Di Virgilio</surname><given-names>Giovanni</given-names></name>
          <email>giovanni@unsw.edu.au</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Hart</surname><given-names>Melissa Anne</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3512-8843</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Jiang</surname><given-names>Ningbo</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Climate Change Research Centre, University of New South Wales, Sydney,
2052, Australia</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Australian Research Council Centre of Excellence for Climate System
Science, University of New South Wales, <?xmltex \hack{\break}?>Sydney, 2052, Australia</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>New South Wales Office of Environment and Heritage, Sydney, 2000,
Australia</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Giovanni Di Virgilio (giovanni@unsw.edu.au)</corresp></author-notes><pub-date><day>8</day><month>May</month><year>2018</year></pub-date>
      
      <volume>18</volume>
      <issue>9</issue>
      <fpage>6585</fpage><lpage>6599</lpage>
      <history>
        <date date-type="received"><day>22</day><month>May</month><year>2017</year></date>
           <date date-type="rev-request"><day>28</day><month>September</month><year>2017</year></date>
           <date date-type="rev-recd"><day>22</day><month>January</month><year>2018</year></date>
           <date date-type="accepted"><day>21</day><month>March</month><year>2018</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2018 </copyright-statement>
        <copyright-year>2018</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</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>
    <p id="d1e113">Internationally, severe wildfires are an escalating problem
likely to worsen given projected changes to climate. Hazard reduction burns
(HRBs) are used to suppress wildfire occurrences, but they generate
considerable emissions of atmospheric fine particulate matter, which
depend upon prevailing atmospheric conditions, and can degrade air quality.
Our objectives are to improve understanding of the relationships between
meteorological conditions and air quality during HRBs in Sydney, Australia.
We identify the primary meteorological covariates linked to high PM<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
pollution (particulates <inline-formula><mml:math id="M2" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 2.5 <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m in diameter) and quantify
differences in their behaviours between HRB days when PM<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> remained
low versus HRB days when PM<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> was high. Generalised additive mixed
models were applied to continuous meteorological and PM<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> observations
for 2011–2016 at four sites across Sydney. The results show that planetary
boundary layer height (PBLH) and total cloud cover were the most consistent
predictors of elevated PM<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> during HRBs. During HRB days with low
pollution, the PBLH between 00:00 and 07:00 LT (local time) was 100–200 m
higher than days with high pollution. The PBLH was similar during
10:00–17:00 LT for both low and high pollution days, but higher after
18:00 LT for HRB days with low pollution. Cloud cover, temperature and wind
speed reflected the above pattern, e.g. mean temperatures and wind speeds
were 2 <inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C cooler and 0.5 m s<inline-formula><mml:math id="M9" 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> lower during mornings and
evenings of HRB days when air quality was poor. These cooler, more stable
morning and evening conditions coincide with nocturnal westerly cold air
drainage flows in Sydney, which are associated with reduced mixing height and
vertical dispersion, leading to the build-up of PM<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. These findings
indicate that air pollution impacts may be reduced by altering the timing of
HRBs by conducting them later in the morning (by a matter of hours). Our
findings support location-specific forecasts of the air quality impacts of
HRBs in Sydney and similar regions elsewhere.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e214">Many regions experience regular wildfires with the potential to damage
property, human health and natural resources (Attiwill and Adams, 2013).
Internationally, the frequency and duration of wildfires are predicted to
increase by the end of the century (e.g. Westerling et al., 2006; Flannigan
et al., 2013). Wildfire frequency and duration have increased in western
North America since the 1980s (Westerling, 2016). Their frequencies have also
increased in south-eastern Australia over the last decade (Dutta et al.,
2016), with a predicted 5–25 % increase in fire risk by 2050 relative to
1974–2003 (Hennessy et al., 2005), a risk compounded by climate change (Luo
et al., 2013). In an effort to mitigate the escalating wildfire risk, fire
agencies in Australia, as is the case internationally, conduct planned hazard
reduction burns (HRBs; also known as prescribed or controlled burns). HRBs
reduce the vegetative fuel load in a controlled manner and aim to lower the
severity or occurrence of wildfires (Fernandes and Botelho, 2003).</p>
      <p id="d1e217">Both wildfires and HRBs generate significant amounts of atmospheric emissions
such as particulate matter (PM),<?pagebreak page6586?> which can impact urban air quality (Keywood
et al., 2013; Naeher et al., 2007; Weise et al., 2015), and consequently
public health (Morgan et al., 2010; Johnston et al., 2011). Of particular
concern are fine particulates with a diameter of 2.5 <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m or less,
(PM<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>). Increased PM<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations are related to health
effects including lung cancer (Raaschou-Nielsen et al., 2013) and
cardiopulmonary mortality (Cohen et al., 2005). These impacts can be more
severe for vulnerable groups, like the young (Jalaludin et al., 2008),
elderly (Jalaludin et al., 2006) and individuals with respiratory conditions
(Haikerwal et al., 2016).</p>
      <p id="d1e246">Sydney, located in the south-eastern Australian state of New South Wales
(NSW), is the focus of this study because HRBs make a significant
contribution to PM pollution in this city and the surrounding metropolitan
region (Office of Environment and Heritage, 2016). Sydney is Australia's
largest city with 4.9 million inhabitants (ABS, 2016). Approximately 130 911 ha  in
NSW was treated by HRBs during 2014–15 (RFS, 2015) and this figure is
projected to increase annually (NSW Government, 2016). Smoke events between
1996 and 2007 in Sydney attributed to wildfires or HRBs were associated with
an increase in emergency department attendances for respiratory conditions
(Johnston et al., 2014). Hence, a potential consequence of HRBs is that
Sydney's population experiences poor air quality and its associated health
impacts (Broome et al., 2016). Furthermore, the eastern Australian fire
season is projected to start earlier by 2030 under future climate change
(Office of Environment and Heritage, 2014). This could restrict the period
within which HRBs can occur, potentially exposing populations to particulates
over more concentrated time frames.</p>
      <p id="d1e249">Sydney is located in a subtropical, coastal basin bordered by the Pacific
Ocean to the east and the Blue Mountains 50 km to the north-west (elevation
1189 m, Australian Height Datum). Its air quality is influenced by mesoscale
circulations, such as terrain-related westerly drainage flows in the evening,
and easterly sea breezes in the afternoon (Hyde et al.,
1980).
These processes interact with synoptic-scale high-pressure systems (Hart et
al., 2006). A recent study by Jiang et al. (2016b) further examined how
synoptic circulations influence mesoscale meteorology and subsequently air
quality in Sydney. The results showed that smoke generated by wildfires and
HRBs makes a significant contribution to elevated PM levels in Sydney, in
particular, under a combined effect of typical synoptic and mesoscale
conditions conducive to high air pollution. However, analysis of the local
(i.e. city-scale) meteorological processes that influence air quality during
HRBs is still sparse. Previous research focusing on a single site in Sydney
found that PM<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations were higher during stable atmospheric
conditions and on-shore (easterly) winds (Price et al., 2012). Elsewhere,
PM<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration was mainly influenced by the receptor-to-burn
distance and wind hits during HRBs (Pearce et al., 2012). We therefore have
three aims: (1) summarise the temporal variation in PM<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations
in Sydney and how this relates to HRB occurrences; (2) characterise
PM<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> pollution sensitivities to meteorological and HRB variables to
identify the primary covariates connected to high pollution; (3) identify the
differences in covariate behaviours between HRB days when PM<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
pollution is low, versus burn days when pollution is high. Achieving these
aims will help efforts to forecast the air pollution impacts of HRBs in
Sydney, and more broadly, in Australia or elsewhere in the world.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e300">Locations of meteorological and PM<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> monitoring stations in
the New South Wales Office of Environment and Heritage network in Sydney,
Sydney Airport meteorological station, and Bureau of Meteorology (BoM)
stations (with station numbers) from which rainfall data were obtained.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f01.jpg"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e321">The area type, elevation, location, inter-annual (2005–2016) mean
and standard deviation (SD) PM<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration (<inline-formula><mml:math id="M21" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of
each monitoring site.</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="left"/>
     <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">Site</oasis:entry>
         <oasis:entry colname="col2">Area Type</oasis:entry>
         <oasis:entry colname="col3">Elevation (m)</oasis:entry>
         <oasis:entry colname="col4">Lat,</oasis:entry>
         <oasis:entry colname="col5">Long.</oasis:entry>
         <oasis:entry colname="col6">PM<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> mean</oasis:entry>
         <oasis:entry colname="col7">PM<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> SD</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Chullora</oasis:entry>
         <oasis:entry colname="col2">Mixed residential–commercial</oasis:entry>
         <oasis:entry colname="col3">10</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M25" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.89</oasis:entry>
         <oasis:entry colname="col5">151.05</oasis:entry>
         <oasis:entry colname="col6">7.56</oasis:entry>
         <oasis:entry colname="col7">4.13</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Earlwood</oasis:entry>
         <oasis:entry colname="col2">Residential</oasis:entry>
         <oasis:entry colname="col3">7</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M26" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.92</oasis:entry>
         <oasis:entry colname="col5">151.13</oasis:entry>
         <oasis:entry colname="col6">7.26</oasis:entry>
         <oasis:entry colname="col7">4.34</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Liverpool</oasis:entry>
         <oasis:entry colname="col2">Mixed residential–commercial</oasis:entry>
         <oasis:entry colname="col3">22</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M27" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.93</oasis:entry>
         <oasis:entry colname="col5">150.91</oasis:entry>
         <oasis:entry colname="col6">8.27</oasis:entry>
         <oasis:entry colname="col7">4.85</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Richmond</oasis:entry>
         <oasis:entry colname="col2">Residential–semi-rural</oasis:entry>
         <oasis:entry colname="col3">21</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M28" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>33.62</oasis:entry>
         <oasis:entry colname="col5">150.75</oasis:entry>
         <oasis:entry colname="col6">6.85</oasis:entry>
         <oasis:entry colname="col7">6.29</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2">
  <title>Data</title>
<sec id="Ch1.S2.SS1">
  <title>Meteorological, air quality and temporal variables</title>
      <p id="d1e560">Continuous time series of hourly meteorology and PM<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
(<inline-formula><mml:math id="M30" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> observations between January 2005 and August 2016
(inclusive) were obtained from four air quality monitoring stations (Chullora,
Earlwood, Liverpool and Richmond) in the NSW Office of Environment and
Heritage (OEH) network in Sydney (Fig. 1). Monitoring stations are located at
varying elevations and in semi-rural, residential and commercial areas
(Table 1). These four locations were chosen because they have the longest
uninterrupted record of PM<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> measurements in Sydney. Prior to 2012
PM<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> was measured using tapered element oscillating microbalance (TEOM)
systems. Since 2012 beta attenuation monitors have been used to measure
PM<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. Although there appear to be effects from instrument change, such
effects are generally small if compared to the daily or hourly
fluctuations in PM<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> levels.</p>
      <p id="d1e632">To compare how PM<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations varied over daily and monthly
timescales, we also obtained hourly measurements of PM<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>
(<inline-formula><mml:math id="M38" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, nitrogen dioxide (NO<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (parts per hundred
million – pphm) and oxides of nitrogen (NO<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (pphm) from these
stations. Meteorological variables included in our analyses were surface
wind speed (m s<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, wind direction (<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>), surface air temperature
(<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) and relative humidity (%). Hourly global solar radiation
(W m<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> data were available at the Chullora station only, but were
subsequently omitted as a predictive variable (see Sect. 3.3.1).</p>
      <p id="d1e749">Hourly total cloud cover (okta) and mean sea level pressure (MSLP; hPa) were
obtained from the Australian Bureau of Meteorology (BoM) Sydney Airport
weather station (WMO station number 94767). These are included as covariates
in models for the four monitoring sites. The 24 h rainfall totals
(mm) were approximated for each OEH station from the BoM weather station that
is nearest (Fig. 1).</p>
      <p id="d1e752">Given its role in the turbulent transport of air pollutants (Seidel et al.,
2010; Pal et al., 2014; Sun et al., 2015; Miao et al., 2015), we included
planetary boundary layer height (PBLH) as an explanatory variable. PBLH has
previously been derived from observational meteorological data by Du et
al. (2013) and Lai (2015), using a method which they found was an effective
estimate of the PBLH and its relationship with PM concentrations. Although
direct PBLH<?pagebreak page6587?> measurements would be ideal, these are unavailable for the study
domain at appropriate spatial and temporal resolutions. Hence, we derived
PBLH estimates at the location of each monitoring station from a subset of
the meteorological data following the method used by the above authors
(Eqs. 1 and 2).

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M46" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtext>PBLH</mml:mtext><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">121</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:mfrac></mml:mstyle><mml:mo>(</mml:mo><mml:mn mathvariant="normal">6</mml:mn><mml:mo>-</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mtext>d</mml:mtext></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">0.169</mml:mn><mml:mi>s</mml:mi><mml:mo>(</mml:mo><mml:mtext>ws</mml:mtext><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.257</mml:mn><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn mathvariant="normal">12</mml:mn><mml:mi>f</mml:mi><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mi>h</mml:mi><mml:mi>l</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi>sin⁡</mml:mi><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M47" display="inline"><mml:mi>s</mml:mi></mml:math></inline-formula> is a stability class that estimates lateral and vertical
dispersion, <inline-formula><mml:math id="M48" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> is surface air temperature and <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mtext>d</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is surface dew
point temperature (approximated for the location of each station using the
method proposed by Lawrence, 2005), ws is wind speed, <inline-formula><mml:math id="M50" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> is wind speed
altitude in m for a given monitoring station, <inline-formula><mml:math id="M51" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula> is the station's estimated
surface roughness index, <inline-formula><mml:math id="M52" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> is the Coriolis parameter in s<inline-formula><mml:math id="M53" 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>, <inline-formula><mml:math id="M54" display="inline"><mml:mi mathvariant="normal">Ω</mml:mi></mml:math></inline-formula>
is the earth's rotational speed (rad s<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M56" display="inline"><mml:mi mathvariant="italic">θ</mml:mi></mml:math></inline-formula> is the station
latitude. The stability typing scheme was based on the Pasquill–Gifford
(P–G) stability categories (Turner, 1964), via a turbulence-based method
using the standard deviation of the azimuth angle of the wind vector and
scalar wind speed.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e947">Kernel density function (magnitude-per-unit area) for hazard
reduction burns (HRBs) conducted in the vicinity of Greater Sydney
(2005–2016). The warmer the colour of the kernel density surface, the
more or larger HRBs that have occurred in that area. The kernel density
calculation is weighted according to fire surface area.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f02.jpg"/>

        </fig>

      <p id="d1e956">We calculated the 24 h mean for hourly meteorological and PM<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
measurements, where wind direction was vector-averaged (i.e. averaging the
<inline-formula><mml:math id="M58" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M59" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> wind components). Log-transformations were applied to PM<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
and rainfall. Applying transformations to the remaining explanatory variables
did not greatly reduce heterogeneity.</p>
      <?pagebreak page6588?><p id="d1e991">Temporal variables trialled for inclusion in analyses included day of the
year, weekday, week, month (all representing different seasonal terms) and
year (because air quality varies from year to year). A Julian date variable
was incorporated to represent the longer-term trend in PM<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
concentrations.
<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Burns</title>
      <p id="d1e1010">Historical records of HRBs conducted between January 2005 and August 2016 in
NSW were obtained from the NSW Rural Fire Service (RFS), the firefighting
agency responsible for the general administration of HRBs. There were a total
of 9200 fire polygons in this data set prior to data conditioning (see
Sect. 3). HRBs are conducted predominantly in autumn (months of March to May
in the Southern Hemisphere) and spring (September to November), and often at
weekends, typically, with burns lit in the early morning. Most historical
HRBs have occurred to the west and north-west of Sydney (Fig. 2). Additional
predictive variables derived from the HRB data (all daily values) were total
number of burns, total burn surface area (ha), median burn elevation (m),
median fire duration (days) and median fire distance from the geographic
centre of the monitoring stations (km).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e1015">Box plots showing the variation in PM<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> air quality index
values (AQIs) at four measurement sites in Sydney between 2011 and 2016
during days when there were no fires (neither hazard reduction burns (HRBs)
or wildfires), days when only HRBs occurred without coincident wildfires,
days when wildfires occurred without coincident HRBs, and days with
concurrent HRBs and wildfires. Horizontal black lines on box plots are median
PM<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> AQIs, and their corresponding values are shown above these lines.
Red circles are outliers.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f03.png"/>

        </fig>

      <p id="d1e1042">It is important to note that other potential sources of PM<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> emissions
in Sydney include motor vehicles, soil erosion and occasional dust storms.
Use of domestic wood-fired heaters can also make a substantial contribution
to PM<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations during winter months (June to August), which is
when HRBs are generally not conducted. However, between 2011 and 2016,
average PM<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> air quality index (AQI) values were higher on days when
either HRBs or wildfires occurred relative to days when there were no fires
(Fig. 3).<?xmltex \hack{\newpage}?></p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Methods</title>
<sec id="Ch1.S3.SS1">
  <title>Statistical approach: generalised additive mixed models</title>
      <p id="d1e1085">Generalised additive models (GAMs) (Hastie and Tibshirani, 1990) offer an
appropriate approach with respect to air quality research because
relationships between covariates are often non-linear, an issue which can be
addressed within the GAM framework. In addition to the seasonal pattern of
hazard reduction burning, PM<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations in Sydney also show
daily, monthly, seasonal and annual variation. Adding terms to a GAM to
account for these temporal variations fails to deal with residual
autocorrelation completely, as is evident in the autocorrelation function
(ACF) of the residuals (Fig. S1 in the Supplement). Given the residual
autocorrelation and non-independence of the data, we used a generalised
additive mixed model (GAMM) approach to take account of the seasonal
variation and trends in the data. GAMMs can combine fixed and random effects
and enable temporal autocorrelation to be modelled explicitly (Wood, 2006).
We assumed a Gaussian distribution and used a log link function. Cubic
regression splines were used for all predictors except wind direction and day
of year, which used cyclic cubic regression splines, because there should be
no discontinuity between values at their end points. Experimenting with
alternative smooth classes did not drastically affect model results or
diagnostics. Smoothing parameters were chosen via restricted maximum
likelihood (REML). We implemented GAMMs with a temporal residual
autocorrelation structure of order 1 (AR-1). More complex structures (e.g.
autoregressive moving average models; ARMAs) of varying order or moving
average parameters produced<?pagebreak page6589?> marginally higher Akaike information criteria
(AICs) (e.g. mean <inline-formula><mml:math id="M68" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 259.6) than models with AR-1 autocorrelation (mean
AIC <inline-formula><mml:math id="M69" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 259.02). Omitting a correlation structure entirely produced the
largest AICs (mean AIC <inline-formula><mml:math id="M70" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 279.5). In all cases, the AR models for the
residuals were nested within 1 month (nesting within weeks and years was also
trialled, but produced higher AICs). Autocorrelation plots obtained by
applying the GAMMs using the AR-1 structure showed that short-term residual
autocorrelation in the residuals had been removed relative to using GAMs
(Figs. S1–S2).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <?xmltex \opttitle{PM${}_{{2.5}}$ trend estimates, monthly and daily means}?><title>PM<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> trend estimates, monthly and daily means</title>
      <p id="d1e1134">We first used the GAMM framework to estimate the annual trend in the weekly
mean concentrations of PM<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> for 2005–2015, split by season, with
Julian day as the only predictor. Monthly and daily mean PM<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations for all years were also
compared to assess how concentrations of each pollutant varied with these
timescales. The latter analyses were performed using <inline-formula><mml:math id="M77" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> software for
statistical computing (R Development Core Team, 2015) and the
“openair” package (Carslaw and Ropkins, 2012). The annual trend and
subsequent statistical analyses described below were performed using <inline-formula><mml:math id="M78" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>
software and packages “mgcv” (Wood, 2011) and “nlme” (Pinheiro
et al., 2017).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <?xmltex \opttitle{Identifying the meteorological and burn variables related to elevated
PM${}_{{2.5}}$}?><title>Identifying the meteorological and burn variables related to elevated
PM<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e1212">To assess how PM<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations vary in relation to the
meteorological, burn and temporal variables, the GAMMs were applied to each
monitoring site separately and focused on the period
January 2011–August 2016. There were comparatively fewer HRBs conducted
prior to 2011, hence the choice of this time frame. For each station, we split
the data into two subsets: (1) for all days when HRBs were conducted and the
PM<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration was less than the median PM<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration
for the location in question, “low pollution days”; (2) for all HRB days
when the PM<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration was greater than the median value for the
location in question, “high pollution days” (the minimum/maximum number of
observations in each low/high subset was in the range 179–189). The time
series were conditioned in this manner to better characterise the differences
in covariate behaviours between burn days when pollution remains low versus
burn days and elevated PM<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. Since our focus is specifically on
PM<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations during HRBs, days when wildfires had occurred were
excluded.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e1272">Annual trends in the weekly mean concentrations of PM<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> in
Sydney, split by season for 2005–2015.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f04.png"/>

        </fig>

<sec id="Ch1.S3.SS3.SSSx1" specific-use="unnumbered">
  <title>Model selection</title>
      <?pagebreak page6590?><p id="d1e1295">Using the GAMM framework described above, we started with a model where the
fixed component included all predictive variables. We used variance inflation
factors (VIFs) to test variables for collinearity (Zuur et al., 2010). We
sequentially dropped covariates with the highest VIF and recalculated the
VIFs, repeating this process until all VIFs were smaller than a threshold of
3.5. This VIF threshold was selected as a compromise between the thresholds
of 3 and 10 stipulated in Zuur et al. (2010). Following this process,
explanatory variables were dropped from the initial model if they were not
statistically significant in any case. As a result, global solar radiation,
relative humidity, burn elevation, burn duration, day of the year, weekday, week
and year were excluded.
<?xmltex \hack{\newpage}?>
An intermediate model included HRB distance as a covariate. Exploratory GAMM
analyses using this model configuration revealed that on average, beyond a
distance of ca. 300 km, the influence of prescribed burns on PM<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
concentrations at the target locations was negligible (Fig. S3). Subsequent
models excluded burn distance and burns <inline-formula><mml:math id="M88" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 300 km from the geographic mean
centre of the monitoring stations. Hence, the fixed component of our optimal
model used the following predictors: PBLH, MSLP, temperature, total cloud
cover, rainfall, wind speed, wind direction, number of burns per day, total
area burnt per day and Julian day.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <?xmltex \opttitle{Diurnal variation in relation to elevated PM${}_{{2.5}}$}?><title>Diurnal variation in relation to elevated PM<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e1332">Meteorological covariates relevant to high PM<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations were
identified via the GAMMs based on criteria of statistical significance at
more than one location, or where the influence of covariates on PM<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
showed a marked distinction between pollution conditions. We then used the
hourly meteorological data for these select covariates to compare their mean
diurnal variation on burn days with low versus high pollution. The 95 %
confidence intervals of these diurnal means were calculated using bootstrap
re-sampling with 1000 replicates.<?xmltex \hack{\newpage}?></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e1356">Mean monthly PM<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations for the period 2005 to
August 2016 at four air quality monitoring sites in Greater Sydney <bold>(a)</bold>.
Southern Hemisphere seasons are summer (DJF), autumn (MAM), winter (JJA) and
spring (SON). Mean daily normalised concentrations of PM<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> compared
to the variations of PM<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NO<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> and NO<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f05.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e1420">Adjusted <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M98" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M99" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> values for the smoothers of the optimal
generalised additive mixed models (GAMMs) applied to each monitoring site on
days when hazard reduction burns occurred and with the data split into low
and high air pollution conditions.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right" colsep="1"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Pollution</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center" colsep="1">Chullora </oasis:entry>
         <oasis:entry rowsep="1" namest="col4" nameend="col5" align="center" colsep="1">Earlwood </oasis:entry>
         <oasis:entry rowsep="1" namest="col6" nameend="col7" align="center" colsep="1">Liverpool </oasis:entry>
         <oasis:entry rowsep="1" namest="col8" nameend="col9" align="center">Richmond </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Condition</oasis:entry>
         <oasis:entry rowsep="1" colname="col2">Low</oasis:entry>
         <oasis:entry rowsep="1" colname="col3">High</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">Low</oasis:entry>
         <oasis:entry rowsep="1" colname="col5">High</oasis:entry>
         <oasis:entry rowsep="1" colname="col6">Low</oasis:entry>
         <oasis:entry rowsep="1" colname="col7">High</oasis:entry>
         <oasis:entry rowsep="1" colname="col8">Low</oasis:entry>
         <oasis:entry rowsep="1" colname="col9">High</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2"><inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col3"><inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col4"><inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col6"><inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col7"><inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col8"><inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col9"><inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.38</oasis:entry>
         <oasis:entry colname="col3">0.44</oasis:entry>
         <oasis:entry colname="col4">0.29</oasis:entry>
         <oasis:entry colname="col5">0.60</oasis:entry>
         <oasis:entry colname="col6">0.39</oasis:entry>
         <oasis:entry colname="col7">0.60</oasis:entry>
         <oasis:entry colname="col8">0.29</oasis:entry>
         <oasis:entry colname="col9">0.47</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Variable</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M111" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M112" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M113" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M114" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M115" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M116" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M117" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M118" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">PBLH</oasis:entry>
         <oasis:entry colname="col2">12.7<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">9.1<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">4.0<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">13.2<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">3.3<inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">29.5<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">4.5<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">6.9<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MSLP</oasis:entry>
         <oasis:entry colname="col2">0.0</oasis:entry>
         <oasis:entry colname="col3">0.4</oasis:entry>
         <oasis:entry colname="col4">0.0</oasis:entry>
         <oasis:entry colname="col5">3.7</oasis:entry>
         <oasis:entry colname="col6">0.0</oasis:entry>
         <oasis:entry colname="col7">2.0</oasis:entry>
         <oasis:entry colname="col8">0.0</oasis:entry>
         <oasis:entry colname="col9">1.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Temperature</oasis:entry>
         <oasis:entry colname="col2">0.0</oasis:entry>
         <oasis:entry colname="col3">3.7<inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.8</oasis:entry>
         <oasis:entry colname="col5">2.9</oasis:entry>
         <oasis:entry colname="col6">4.6<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">10.9<inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">0.1</oasis:entry>
         <oasis:entry colname="col9">2.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Cloud cover</oasis:entry>
         <oasis:entry colname="col2">12.9<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">16.9<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">9.2<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">9.9<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">10.6<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">16.9<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">2.9</oasis:entry>
         <oasis:entry colname="col9">7.6<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Rainfall</oasis:entry>
         <oasis:entry colname="col2">2.0</oasis:entry>
         <oasis:entry colname="col3">1.6</oasis:entry>
         <oasis:entry colname="col4">5.7<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">8.9<inline-formula><mml:math id="M138" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">7.3<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">1.2</oasis:entry>
         <oasis:entry colname="col8">8.8<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">3.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Wind direction</oasis:entry>
         <oasis:entry colname="col2">0.0</oasis:entry>
         <oasis:entry colname="col3">1.0<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.0</oasis:entry>
         <oasis:entry colname="col5">1.7<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">0.0</oasis:entry>
         <oasis:entry colname="col7">2.5<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">0.0</oasis:entry>
         <oasis:entry colname="col9">0.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Wind speed</oasis:entry>
         <oasis:entry colname="col2">0.1</oasis:entry>
         <oasis:entry colname="col3">2.4</oasis:entry>
         <oasis:entry colname="col4">3.4</oasis:entry>
         <oasis:entry colname="col5">3.9<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">1.0</oasis:entry>
         <oasis:entry colname="col7">0.0</oasis:entry>
         <oasis:entry colname="col8">5.8<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">0.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HRBs daily frequency</oasis:entry>
         <oasis:entry colname="col2">3.1</oasis:entry>
         <oasis:entry colname="col3">2.3<inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">0.0</oasis:entry>
         <oasis:entry colname="col5">2.8<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">1.1</oasis:entry>
         <oasis:entry colname="col7">3.5<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">0.1</oasis:entry>
         <oasis:entry colname="col9">1.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HRBs area burnt daily</oasis:entry>
         <oasis:entry colname="col2">6.8<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">1.4</oasis:entry>
         <oasis:entry colname="col4">3.0</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
         <oasis:entry colname="col6">1.6</oasis:entry>
         <oasis:entry colname="col7">5.7<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">1.2</oasis:entry>
         <oasis:entry colname="col9">9.5<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Julian Day</oasis:entry>
         <oasis:entry colname="col2">12.1<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">5.9<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">10.1<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">10.7<inline-formula><mml:math id="M155" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">18.8<inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">11.9<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">32.3<inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9">2.6</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e1448">Asterisks denote statistical
significance: <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>*</mml:mo><mml:mo>*</mml:mo></mml:mrow></mml:msup><mml:mo>=</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>.</p></table-wrap-foot></table-wrap>

</sec>
</sec>
<sec id="Ch1.S4">
  <title>Results</title>
<sec id="Ch1.S4.SS1">
  <?xmltex \opttitle{Temporal variation in PM${}_{{2.5}}$ concentrations}?><title>Temporal variation in PM<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations</title>
      <p id="d1e2580">There is an increasing inter-annual trend in weekly mean PM<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
concentrations in all seasons during 2011 to 2015, especially in summer and
winter (Fig. 4). Mean PM<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations range from 6 to
10 <inline-formula><mml:math id="M162" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Mean monthly PM<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> averaged over all years
shows increasing concentrations from early autumn (March), peaking in May,
then decreasing towards the end of winter, before increasing again from early
spring (Fig. 5a). Notably, mean daily PM<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations (averaged
over all years) are higher at weekends relative to other pollutants
(PM<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>; Fig. 5b).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <?xmltex \opttitle{Meteorological and burn variables related to PM${}_{{2.5}}$}?><title>Meteorological and burn variables related to PM<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e2682">Adjusted <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values for high pollution models were between 0.44 and 0.60,
and between 0.29 and 0.39 for the low pollution models (Table 2). PBLH and
total cloud cover were the most consistent predictors of elevated PM<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
during HRBs (Table 2). On high pollution days, PBLH had a statistically
significant, negative influence on predicted PM<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations at all
locations (Fig. 6). This influence was generally more linear on high
pollution days, relative to low pollution days. Notably, fitted curves for
PM<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>–PBLH were steeper at lower altitudes (<inline-formula><mml:math id="M174" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 800 m) in the high
pollution condition. Cloud cover had a negative influence on predicted
PM<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations that was significant in all but one case (Table 2),
though fitted curves do not appear to differ noticeably between pollution
conditions (Fig. 7). Although temperature<?pagebreak page6591?> and wind speed showed a more
variable pattern of statistical significance (Table 2), they exhibited marked
differences in behaviour between low and high pollution days. During high
pollution, temperature typically had a negative, curvilinear influence on
fitted PM<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (Fig. 8). This negative influence flattens or
reverses at temperatures <inline-formula><mml:math id="M177" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 20 <inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. In contrast, the PM<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>–temperature relationship was weak and linear during low pollution days. Wind
speed had a significant influence on PM<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> only at Earlwood and Richmond
(Table 2). During low pollution days, this association is negative at most
locations. During high pollution conditions at Chullora and Earwood, there is
a positive influence on PM<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> at low wind speeds which reverses at
speeds above ca. 2 m s<inline-formula><mml:math id="M182" 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> (Fig. S7). During HRBs and high pollution,
wind direction curves show peaks between approximately 250 and 310<inline-formula><mml:math id="M183" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
at Chullora, Earlwood and Liverpool (south-westerly to north-westerly flows)
(Fig. 9). Earlwood frequently experiences north-westerly flows during spring,
autumn and winter, whilst south-westerly flows are common during the same
seasons at Liverpool (Fig. S4).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e2816">The contribution by the planetary boundary layer height (PBLH)
component of the generalised additive mixed model (GAMM) linear predictor to
fitted PM<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (<inline-formula><mml:math id="M185" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, centred). The solid lines are
the fitted curves. Dotted lines are 95 % confidence bands. Dots are
partial residuals.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e2856">The contribution by the cloud cover component of the GAMM linear
predictor to fitted PM<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (<inline-formula><mml:math id="M188" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M189" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, centred). The
solid lines are the fitted curves. Dotted lines are 95 % confidence bands.
Dots are partial residuals.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e2897">The contribution by the temperature component of the GAMM linear
predictor to fitted PM<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (<inline-formula><mml:math id="M191" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M192" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, centred).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f08.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e2937">The contribution by the wind direction component of the GAMM
linear predictor to fitted PM<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (<inline-formula><mml:math id="M194" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, centred).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e2977">The contribution by the hazard reduction burn (HRB) daily
frequency (number of concurrent burns per day) component of the GAMM linear
predictor to fitted PM<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> values (<inline-formula><mml:math id="M197" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M198" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, centred).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f10.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p id="d1e3017">Mean diurnal variation of hourly PBLH, total cloud cover,
temperature and wind speed for low versus high PM<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> pollution during
HRBs at Liverpool, Sydney (see Figs. S8–S10 for other stations). Shading
represents the 95 % confidence intervals of the means.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/6585/2018/acp-18-6585-2018-f11.png"/>

        </fig>

      <p id="d1e3036">The remaining meteorological predictors either did not show marked
differences between pollution conditions or were statistically significant in
only one instance. Rainfall generally had a negative influence on PM<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
during HRBs (Fig. S5). MSLP had a positive association with higher PM<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
concentrations during low and high pollution (Fig. S6), though this
association was only significant during high pollution at Richmond (Table 2).</p>
      <?pagebreak page6592?><p id="d1e3057">HRB frequency had a significant and positive influence on PM<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> only for
the high pollution condition at Chullora, Earlwood and Liverpool (Table 2 and
Fig. 10). The association between burn area and PM<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> during high
pollution was significant at Liverpool and Richmond only. The influence of
Julian day on PM<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> showed significant non-linear, increasing trends in
all instances.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <?xmltex \opttitle{Differences in covariate behaviours on HRB days with low versus
high PM${}_{{2.5}}$}?><title>Differences in covariate behaviours on HRB days with low versus
high PM<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula></title>
      <p id="d1e3102">Having identified the most informative and consistent meteorological
predictors using the GAMMs, we assessed their mean diurnal variation during
the occurrence of HRBs and low versus high PM<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> pollution in the
following sections.
<?xmltex \hack{\newpage}?></p>
<sec id="Ch1.S4.SS3.SSS1">
  <title>PBLH</title>
      <p id="d1e3120">Taking Liverpool as an example, between 00:00 and 07:00 LT during low
pollution days when HRBs have occurred, the PBLH is on average 100–200 m
higher than during high pollution days (Fig. 11; see Figs. S8–S10 for the
other monitoring stations). From late morning (ca. 10:00 LT) until early
evening (ca. 19:00 LT), the PBLH altitudes of both PM<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> conditions are
very similar, but after 19:00 LT the PBLH is again higher during low
pollution.</p>
</sec>
<sec id="Ch1.S4.SS3.SSS2">
  <title>Total cloud cover</title>
      <p id="d1e3138">During HRBs, mean diurnal variation of cloud cover is between 2 and 7 %
greater during the mornings and evenings of low pollution, compared to high
pollution days (Fig. 11).<?pagebreak page6593?> In contrast, there is minimal difference in cloud
cover during the early afternoon of both conditions.</p>
</sec>
<sec id="Ch1.S4.SS3.SSS3">
  <title>Temperature</title>
      <p id="d1e3147">The temperature is 1–6 <inline-formula><mml:math id="M208" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warmer between 00:00–08:00 LT and
20:00–23:00 LT during HRBs and low PM<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>, in comparison to burns
coinciding with high pollution (Fig. 11). However, there is a clear reversal
in this trend from mid-morning to late afternoon during burns and high
PM<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> when mean temperature is several degrees warmer than during HRBs
and low pollution.</p>
</sec>
<sec id="Ch1.S4.SS3.SSS4">
  <title>Wind speed</title>
      <p id="d1e3184">Mean diurnal wind speed is approximately 0.5 m s<inline-formula><mml:math id="M211" 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> higher in the
mornings and after 18:00 LT during burns and low air pollution in comparison
to speeds during high PM<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> (Fig. 11). In contrast, there is a minimal
difference in wind speeds between 12:00 and 18:00 LT.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S5">
  <title>Discussion</title>
      <p id="d1e3217">Air quality in Sydney is generally good. On the occasions when it is poor,
atmospheric particulates are the principal cause, and HRBs are potentially
one source of high particulate emissions. Sydney's population is projected to
increase (<inline-formula><mml:math id="M213" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 63 %) to over 8 million by 2061 (ABS, 2013), with much
of the expansion occurring at the urban–bushland transition. Even if air
quality remains stable, these demographic changes will increase exposure to
particulate pollution. However, we observed increasing annual trends in
PM<inline-formula><mml:math id="M214" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations. In addition, projected decreases in future
rainfall (Dai, 2013) and increases in fire danger weather are likely to
increase fire activity and lengthen the fire season (Bradstock et al., 2014),
thus amplifying fire-related particulate<?pagebreak page6594?> emissions. Changes in measurement
instrumentation have a potential for introducing systematic biases in these
annual PM<inline-formula><mml:math id="M215" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> trends. Recently, based on the high correlation among
beta attenuation monitors, PM<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> measurements and long-term
nephelometer visibility measurements at each monitoring site, the NSW
Government (2016, 2017a, b) reconstructed a more consistent annual average
PM<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> time series. Their results also showed a tendency of increasing
annual PM<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> levels near 2011–2012 in some Sydney subregions, as is
consistent with the results from this study. Moreover, our study also
indicates that the trends start increasing from 2011 during spring and
winter, which pre-dates the instrumentation change. These results suggest
that the instrumentation changes that occurred in 2012 are likely to have
had minimal impact on the trend analysis reported in this analysis.</p>
      <p id="d1e3273">Relative to other pollutants such as NO<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
concentrations are higher at weekends. PM<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations also start
increasing in autumn with peaks in winter and spring. These patterns may
reflect the timing of HRB occurrences, which occur mainly in autumn, spring
and at<?pagebreak page6595?> weekends, though there is also increased domestic wood-fired heating
during winter. Consequently, conducting multiple, concurrent HRBs during
these periods might exacerbate PM<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations that are already
high relative to baseline.</p>
      <p id="d1e3321">PM<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations tend to be dominated by organic matter (57 %)
during peak HRB periods in autumn. There is also contribution, in order of
apportion, from elemental carbon, inorganic aerosol and sea salt. This
compares to summer months when sea salt plays a larger role, with organic
matter making up just 34 % (Cope et al., 2014). Other days where national
PM<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration standards have been exceeded have been attributed to
wildfires and dust storms. PM<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations also tend to be higher
across the Sydney basin during winter due to smoke from wood fire heaters
used for residential heating; however, exceedances of standards due to these
emissions are rare (EPA, 2015).</p>
<sec id="Ch1.S5.SS1">
  <?xmltex \opttitle{Primary covariates affecting PM${}_{{2.5}}$ and how they differ during
low and high pollution}?><title>Primary covariates affecting PM<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> and how they differ during
low and high pollution</title>
      <p id="d1e3366">PBLH was the most consistent meteorological predictor of PM<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. It had a
significant, negative influence on PM<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> at all locations during HRBs
and “high pollution days”. There was a marked difference in mean diurnal
mixed layer heights between low and high pollution conditions in the early
morning (00:00–07:00 LT) and from 20:00 to 23:00 LT, with the PBLH being
approximately 100–200 m lower at these times during HRBs and high
PM<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. During these two time periods whilst the PBLH is low, mean cloud
cover, temperature and wind speeds are also lower relative to their
magnitudes at corresponding times during low pollution. Essentially, these
early hours of cold, stable conditions with minimal turbulence (i.e.
conditions that are conducive to temperature inversions) prevent the dilution
of PM<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. These subdued conditions often coincide with the night
time–early morning westerly cold drainage flows and low mixing heights
(inhibiting vertical dispersion), leading to the build-up of PM<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
during mornings (Lu and Turco, 1995; Hart et al., 2006; Jiang et al., 2016b).
These pollution-conducive conditions are similar to those identified in Jiang
et al. (2016a) as being related to a ridge of high pressure extending across
eastern Australia, resulting in light north-westerly winds. These
synoptically driven flows, although light, tend to enhance nocturnal drainage
flows, inhibit afternoon sea breeze formation and allow the transportation
of pollutants across the Sydney basin to the coast. There is also a large
difference in mean diurnal temperatures between low and high pollution
conditions from late morning to early evening, with temperatures
3–4 <inline-formula><mml:math id="M233" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warmer during high pollution. During warmer daytime
conditions, PM<inline-formula><mml:math id="M234" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> can be potentially higher without fire events, for
instance, because these conditions tend to be coincident with increased
precursor emissions and generation of secondary organic aerosols in the air.
Furthermore, the fact that early morning and late evening temperatures tend
to be lower during high pollution conditions may indicate the presence of
temperature inversions which hinder atmospheric convection, leading to the
collection of particulates that cannot be lifted from the surface. Cold
morning temperatures can also result in stronger drainage flows into the
Sydney basin. Consequently, if HRBs are being conducted during early mornings
in the hills and mountains to the west of Sydney, this could result in the
dispersion of particles from such sources, possibly into populated areas.</p>
      <p id="d1e3433">These findings indicate how the timing of HRBs can be altered to reduce their
air pollution impacts in Sydney. Conducting HRBs when the PBLH is forecast to
be higher ought to help reduce their air quality impacts in Sydney. More
specifically, conducting HRBs later in the morning (for example by a matter
of hours) is one way of potentially reducing HRB air quality impacts, because
the PBLH generally starts increasing rapidly in height from 07:00 until
12:00 LT. Fires conducted early in the morning when the PBLH is at its
lowest and temperatures are cool will promote effects such as fire smoke
residing near ground level. One constraint concerning later burn times is
that wind speed typically increases as the day progresses. However, the
maximum mean diurnal wind speed was approximately 3 m s<inline-formula><mml:math id="M235" 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> and occurred
at 15:00 LT. This is considerably lower than the RFS's upper-limit of
5.56 m s<inline-formula><mml:math id="M236" 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> for conducting safe HRBs (Plucinski and Cruz,
2015).
An additional caution for conducting burns later in the afternoon is that
onshore coastal breezes can develop during afternoons. The optimal timing of
burns will also be dependent on other factors such as burn intensity,
lighting method, fuel–soil moisture and geographic location.</p>
      <p id="d1e3460">There was a negative association between cloud cover and PM<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> levels.
It is possible that fire agencies conduct fewer HRBs during cloudy conditions
in case of rain. Rainfall (if any) can also scavenge PM pollution out of the
air. However, cloudless skies are also associated with high pressure systems,
and therefore cool air descending, resulting in a stable calm atmosphere and
low PBLH that is not conducive to pollutant dispersion.</p>
      <p id="d1e3472">Although there were similarities in the influence of covariates between
locations, these associations often varied spatially. For example, mean
diurnal PBLH and temperature were lower at Richmond in the early morning and
at night in comparison to the other locations (Fig. S10). Richmond is further
inland than the other monitoring sites and is thus closer to the mountain
range to the west of Sydney. The insights gained into the spatial variation
in the behaviour of covariates can support efforts to create
location-specific particulate pollution forecasts.</p>
      <p id="d1e3476">The north-westerly signal apparent for three of four locations during HRBs
and high pollution may reflect the fact that, overall, the majority of burns
are conducted to the west, north and north-west of Sydney (Fig. 2). From a
management perspective, comparatively greater attention might be devoted to
adapting burn operations in these regions. In the case of Richmond (where
wind direction did not have a<?pagebreak page6596?> statistically significant influence), one
possible explanation is that the daily vector-averaging applied to the wind
data has smoothed out the signal associated with diurnal changes in wind
directions (and speeds), e.g. between drainage flow and sea breezes. Thus, to
some degree, the signal of wind influence may be suppressed in this case.
Another contributing factor could be Richmond's generally closer proximity to
local burns. Also, its geographic location is quite different to that of the
other monitoring sites; it is further inland than the other sites and is thus
closer to the mountain range to the west of Sydney.</p>
      <p id="d1e3479">Using a different analysis approach, Price et al. (2012) found that the
optimum radius of influence of landscape fires on PM<inline-formula><mml:math id="M238" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> was 100 km for
Sydney. We found that whilst close-proximity fires influenced air quality,
fires up to approximately 300 km from monitoring stations also potentially
influenced PM<inline-formula><mml:math id="M239" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>. Longer-range exposures on regional scales,
particularly from multiple HRBs in an air shed can impact communities at
considerable distance under certain atmospheric transport conditions (e.g.
Liu et al., 2009).</p>
      <p id="d1e3500">Multiple concurrent burns are more likely to adversely affect air quality in
Sydney, as indicated by the significant, positive influence of the number of
concurrent HRBs on PM<inline-formula><mml:math id="M240" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> during high pollution days at all locations
except Richmond. In general, greater numbers of concurrent burns within a
given air shed are likely to result in greater quantities of particulate
emissions. The area of these burns would also determine the amount of
particulate emissions generated. HRB total area per day was a statistically
significant predictor at two locations (Liverpool and Richmond). There are
several possible explanations for the fact that burn daily frequency and
area are not significant predictors at all locations. There will be some
noise in total PM<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations contributed by other emission
sources, and this will vary with location. For example, Richmond differs
from the other monitoring sites in that it is near agricultural land, and so
emission sources like soil erosion and fertiliser use will introduce noise
at this location. Investigating the relationships between burnt area and
fire-related tracer species to reduce the noise in total concentrations
contributed by other sources could be attempted in future work. There are
also uncertainties regarding how accurately the area actually burnt was
recorded within some polygons representing HRBs. In particular, to date it
has been difficult to obtain timely and accurate estimates of the actual area
burnt. Moreover, larger burns are often further away from the urban centres
chosen, and are less frequent than smaller burns. In contrast, moderate to
small burns are more frequent and often scattered along the urban fringes
(rather than confined to one location or direction) and thus have a larger effect
on the overall air quality within urban centres. Transport of smoke is
also determined by interactions between basin topography and local or synoptic
wind conditions. However, the interaction between mesoscale geography and
meteorological variables is a factor that could not be easily accounted for
in the present study (i.e. each site is located in a different location,
therefore each has differing topography and land use type).</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e3528">Fine particulate concentrations are increasing in Sydney, and given projected
increases in fire danger weather, intensification in fire activity is
expected to further amplify fire-related PM<inline-formula><mml:math id="M242" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> emissions. We identified
the key meteorological factors linked to elevated PM<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> during HRBs. In
particular, diurnal variation of the PBLH, cloud cover, temperature and wind
speed have a pervasive influence on PM<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations, with these
factors being more variable and higher in magnitude during the mornings and
evenings of HRB days when PM<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> remains low. These findings indicate how
the timing of HRBs can be altered to minimise pollution impacts. They can
also support locality-specific forecasts of the air quality impacts of burns
in Sydney and potentially other locations globally. In addition to mitigating
wildfire risk, HRBs are used globally for forest management, farming, prairie
restoration and greenhouse gas abatement. Future research should incorporate
more sophisticated fire characteristics such as plume height and fuel
moisture into analyses, and also consider the influence of climatic phenomena
on particulate pollution. Synoptic features can also be incorporated into a
future GAMM analysis, as well as modelling the diurnal evolution of
PM<inline-formula><mml:math id="M246" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> pollution due to HRB occurrences.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e3580">Meteorology and air quality data were obtained from the New South Wales Office of Environment and Heritage
(<uri>http://www.environment.nsw.gov.au/</uri>, New South Wales Office of Environment and Heritage, 2005–2016).
Cloud cover and rainfall data were obtained from the Australian Bureau of Meteorology
(<uri>http://www.bom.gov.au/</uri>, Bureau of Meteorology, 2005–2016).
Data on historical burns were obtained from the New South Wales Rural Fire Service
(<uri>https://www.rfs.nsw.gov.au/</uri>, New South Wales Rural Fire Service, 2005–2016).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3592">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-18-6585-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-18-6585-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution">

      <p id="d1e3601">GDV, MAH and NJ conceived the research questions and
aims. GDV designed and performed the analyses with contributions from all
co-authors. GDV prepared the paper with contributions from all
co-authors.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e3607">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><?pagebreak page6597?><p id="d1e3613">This research was supported by the NSW Environmental Trust under grant
2014/RD/0147 and the NSW Office of Environment and Heritage (OEH). We thank
OEH, the Bureau of Meteorology, and the NSW Rural Fire Service NSW (NSW RFS) for providing the air
quality, meteorological and fire data used in this research. We also thank four anonymous reviewers who provided valuable feedback on this research.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Yun Qian<?xmltex \hack{\newline}?> Reviewed by: four
anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Meteorological controls on atmospheric particulate pollution during hazard reduction burns</article-title-html>
<abstract-html><p>Internationally, severe wildfires are an escalating problem
likely to worsen given projected changes to climate. Hazard reduction burns
(HRBs) are used to suppress wildfire occurrences, but they generate
considerable emissions of atmospheric fine particulate matter, which
depend upon prevailing atmospheric conditions, and can degrade air quality.
Our objectives are to improve understanding of the relationships between
meteorological conditions and air quality during HRBs in Sydney, Australia.
We identify the primary meteorological covariates linked to high PM<sub>2.5</sub>
pollution (particulates  &lt; &thinsp;2.5&thinsp;µm in diameter) and quantify
differences in their behaviours between HRB days when PM<sub>2.5</sub> remained
low versus HRB days when PM<sub>2.5</sub> was high. Generalised additive mixed
models were applied to continuous meteorological and PM<sub>2.5</sub> observations
for 2011–2016 at four sites across Sydney. The results show that planetary
boundary layer height (PBLH) and total cloud cover were the most consistent
predictors of elevated PM<sub>2.5</sub> during HRBs. During HRB days with low
pollution, the PBLH between 00:00 and 07:00&thinsp;LT (local time) was 100–200&thinsp;m
higher than days with high pollution. The PBLH was similar during
10:00–17:00&thinsp;LT for both low and high pollution days, but higher after
18:00&thinsp;LT for HRB days with low pollution. Cloud cover, temperature and wind
speed reflected the above pattern, e.g. mean temperatures and wind speeds
were 2&thinsp;°C cooler and 0.5&thinsp;m&thinsp;s<sup>−1</sup> lower during mornings and
evenings of HRB days when air quality was poor. These cooler, more stable
morning and evening conditions coincide with nocturnal westerly cold air
drainage flows in Sydney, which are associated with reduced mixing height and
vertical dispersion, leading to the build-up of PM<sub>2.5</sub>. These findings
indicate that air pollution impacts may be reduced by altering the timing of
HRBs by conducting them later in the morning (by a matter of hours). Our
findings support location-specific forecasts of the air quality impacts of
HRBs in Sydney and similar regions elsewhere.</p></abstract-html>
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