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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">WCD</journal-id><journal-title-group>
    <journal-title>Weather and Climate Dynamics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">WCD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Weather Clim. Dynam.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2698-4016</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/wcd-3-1183-2022</article-id><title-group><article-title>Subseasonal precipitation forecasts of opportunity<?xmltex \hack{\break}?> over central southwest Asia</article-title><alt-title>Subseasonal precipitation forecasts of opportunity over central southwest Asia</alt-title>
      </title-group><?xmltex \runningtitle{Subseasonal precipitation forecasts of opportunity over central southwest Asia}?><?xmltex \runningauthor{M. L. Breeden et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Breeden</surname><given-names>Melissa L.</given-names></name>
          <email>melissa.breeden@noaa.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Albers</surname><given-names>John R.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8383-3379</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Hoell</surname><given-names>Andrew</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Cooperative Institute for Research in Environmental Sciences,
University of Colorado Boulder, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>NOAA Physical Sciences Laboratory, Boulder, CO, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Melissa L. Breeden (melissa.breeden@noaa.gov)</corresp></author-notes><pub-date><day>27</day><month>October</month><year>2022</year></pub-date>
      
      <volume>3</volume>
      <issue>4</issue>
      <fpage>1183</fpage><lpage>1197</lpage>
      <history>
        <date date-type="received"><day>27</day><month>June</month><year>2022</year></date>
           <date date-type="rev-request"><day>12</day><month>July</month><year>2022</year></date>
           <date date-type="rev-recd"><day>23</day><month>September</month><year>2022</year></date>
           <date date-type="accepted"><day>7</day><month>October</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://wcd.copernicus.org/articles/.html">This article is available from https://wcd.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://wcd.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://wcd.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e107">Subseasonal forecasts of opportunity (SFOs) for precipitation over
southwest Asia during January–March at lead times of 3–6 weeks are
identified using elevated expected forecast skill from a linear inverse
model (LIM), an empirical dynamical model that uses statistical
relationships to infer the predictable dynamics of a system. The expected
forecast skill from this LIM, which is based on the atmospheric circulation,
tropical outgoing longwave radiation, and sea surface temperatures, captures
the predictability associated with many relevant signals as opposed to just
one. Two modes of variability, El Niño–Southern Oscillation (ENSO) and
the Madden–Julian Oscillation (MJO), which themselves are predictable
because of their slow variations, are related to southwest Asia
precipitation SFOs. Strong El Niño events, as observed in 1983, 1998,
and 2016, significantly increase the likelihood by up to 3-fold of an SFO 3–4 and 5–6 weeks in advance. Strong La Niña events, as observed in 1989, 1999, 2000, also significantly increase the likelihood of an SFO at those same lead times. High-amplitude MJO events in phases 2–4 and 6–8 of greater than one standardized departure also significantly increase the
likelihood of an SFO 3–4 weeks in advance. Predictable atmospheric
circulation patterns preceding anomalously wet periods indicate a role for
enhanced tropical convection in the South Pacific convergence zone (SPCZ)
region, while suppressed convection is observed preceding predictable dry
periods. Anomalous heating in this region is found to distinguish wet and
dry periods during both El Niño and La Niña conditions, although the atmospheric circulation response to the heating differs between each ENSO phase.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e119">Precipitation over central southwest Asia, defined here as 22–48<inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 50–80<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E and encompassing Afghanistan, Pakistan, Iran,
Turkmenistan, Uzbekistan, Tajikistan, and Kyrgyzstan, occurs mainly during
the cold season from November–April and determines the region's subsequent
water supply used for agriculture and consumption (Agrawala et al., 2001;
Barlow et al., 2006). It is in this context that accurate precipitation
predictions are critical, given the effect of water on food security and
livelihoods (Famine Early Warning Systems Network, 2022) in this semi-arid
region (Barlow et al., 2016). However, precipitation forecasts from dynamical
models lack skill by lead times of 3 weeks over southwest Asia (de
Andrade et al., 2018; Pegion et al., 2019). An alternative endeavor is
identifying the smaller subset of forecasts at lead times of 3 to 6 weeks that <italic>are</italic> skillful, so-called “subseasonal forecasts of opportunity”
(SFOs; Lang et al., 2020; Mariotti et al., 2020), by forecasting the forecast
skill (Kalnay and Dalcher, 1987). SFOs can arise from slowly evolving
tropical phenomena such as the El Niño–Southern Oscillation (ENSO;
Newman et al., 2003; Johnson et al., 2014; Domeisen et al., 2019; Mariotti et
al., 2020; Albers and Newman, 2021) and Madden–Julian Oscillation (MJO;
Rodney et al., 2013; Johnson et al., 2014; Li and Robertson, 2015; Mayer and
Barnes, 2021), which can force atmospheric circulation patterns to the
extratropics through anomalous divergence (e.g., Sardeshmukh and Hoskins,
1988).</p>
      <p id="d1e143">Precipitation over southwest Asia may be a favorable target variable and
location for SFOs, as both ENSO (Barlow et al., 2002; Nazemosodat and Ghasemi, 2004; Hoell et al., 2012, 2014a, b, 2015a, b, 2017, 2018a) and
the MJO (Barlow et al., 2005; Nazemosodat and Ghaedamini, 2010; Hoell et al., 2013; Cannon et al., 2017; Hoell et al., 2018b) can modulate precipitation in
this region. Hoell et al. (2018a) considered the sensitivity of southwest
Asian precipitation to central Pacific (CP) and eastern Pacific (EP) El
Niño and La Niña conditions and found that while both CP and EP El
Niño conditions shifted precipitation anomalies towards the upper
tercile, a wide range of extreme precipitation outcomes was still possible.
CP La Niña events shifted precipitation towards the lower tercile, while
EP La Niña events did not significantly shift precipitation in the
region. Hoell et al. (2018b) found that, in the 5 d following MJO
phases 2–4 (enhanced eastern Indian Ocean convection), negative
precipitation anomalies developed as a response to an anomalous upper-level
anticyclone and subsidence. Conversely, MJO phases 6–8 (suppressed eastern
Indian Ocean convection) were associated with anomalous upper-level
troughing, ascent, and positive precipitation anomalies. However, Cannon et
al. (2017) found a nuanced impact of the MJO on extreme western Himalayan
snowfall due to competing influences of the MJO on the dynamic forcing for
vertical motion and moisture availability. The convolved impact of ENSO and
MJO activity on precipitation in the region is cited as an additional
confounding factor that can obscure the nature of the two teleconnections
(Schrage et al., 1999; Hoell et al., 2013; Riddle et al., 2013). Objective
methods for considering this combined influence, as well as how it leads to SFOs,
are therefore of interest to both better provide real-time subseasonal
forecast guidance and understand sources of predictability.</p>
      <p id="d1e146">Based on past success, this study uses a linear inverse model (LIM; Penland
and Sardeshmukh, 1995) and its associated signal-to-noise metric “expected
skill” (Sardeshmukh et al., 2000; Newman et al., 2003) to anticipate SFOs over
southwest Asia. Albers and Newman (2019) used expected skill to identify
SFOs, at the time of forecast, for North Pacific and North Atlantic 500 hPa
geopotential height anomalies. They found that periods of elevated expected-skill forecast by the LIM identified more skillful forecasts compared to the
European Centre for Medium-Range Weather Forecasts (ECMWF) Integrated
Forecasting System (IFS) and National Centers for Environmental Prediction
Climate Forecast System Version 2 (NCEP CFSv2) initialized forecast systems,
implying that sources of predictability are common among various model
types. Albers and Newman (2021) found that North Atlantic Oscillation (NAO)
SFOs could be identified in both the LIM and the IFS and were driven by a set
of ENSO-related climate modes, reflecting the utility of the LIM in
targeting regional phenomena.</p>
      <p id="d1e149">Global processes and their unique interactions with local precipitation and
temperature ultimately produce SFOs and can be identified by training a LIM
on specific regional- <?xmltex \hack{\mbox\bgroup}?>and/or<?xmltex \hack{\egroup}?> large-scale interactions, as demonstrated in Breeden et
al. (2022) and Albers et al. (2022) for North American 2 m temperature
(2mT). Based on these results, here we develop a LIM for subseasonal
precipitation over southwest Asia that has been designed in a similar
manner. We will show that precipitation SFOs determined using LIM expected
skill can successfully be identified for subseasonal precipitation over
southwest Asia with a LIM that is regional in precipitation and temperature
but large-scale with the inclusion of hemispheric tropical outgoing longwave
radiation (OLR), sea surface temperatures (SSTs), and 200 hPa Northern
Hemisphere streamfunctions (<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). Another beneficial
quality of the LIM is the negligible computational power needed to generate
a long record of hindcasts. This study will focus on LIM SFOs and does not
evaluate the skill of other models, though past research suggests that
forecasts generated elsewise can similarly be more skillful during
LIM-identified SFOs (Albers and Newman, 2019, 2021).</p>
      <p id="d1e168">The LIM developed for regional precipitation over southwest Asia is used to
test the hypothesis that SFOs can be anticipated using theoretical expected
skill and are associated with strong ENSO and MJO events. Section 2
introduces the reanalysis and satellite products employed, how the LIM is
constructed, and how SFOs are identified using expected skill. Section 3
shows a comparison of this approach to other methods of anticipating periods
of elevated forecast skill, as well as the correspondence between forecasts of
opportunity and ENSO and the MJO. Section 4 contextualizes results and
proposes next steps.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data</title>
      <p id="d1e186">To train the LIM, <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, 2mT, SST, and OLR data from
Japan Meteorological Agency 55-year Reanalysis (JRA-55; Kobayashi et al., 2015) and precipitation from the Climate Hazards group Infrared Precipitation with
Stations (CHIRPS; Funk et al., 2015) dataset are used for the period January–March in 1982–2020. Variables and their respective domains are listed in Table 1. To consider how forecast skill and forecasts of opportunity change as a function of the ENSO phase, the Niño3.4 index was calculated using SST anomalies averaged from 5<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N–5<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 170–120<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W (Trenberth, 1997; Trenberth and Stepaniak, 2001). For
examining relationships between skill and the MJO, the real-time
multivariate MJO (RMM) index, a combined tropical OLR and circulation index
that is designed to capture characteristics of the MJO (Wheeler and Hendon,
2004), is employed, including RMM amplitude, which measures MJO strength,
and each day's associated MJO phase, which tracks MJO location. Finally,
based on results in Sect. 3b, we assess the strength of tropical OLR
anomalies in the South Pacific convergence zone (SPCZ; box in Fig. 10),
defined as 10<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–2.5<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 140–180<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The time
series of OLR anomalies in this region is considered a third metric, in
addition to Niño3.4 and RMM, that might increase the likelihood of an
SFO occurring.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e258">LIM variables that compose the state vector <inline-formula><mml:math id="M11" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula>,
their domain, and the percent (%) variance explained by the retained empirical orthogonal functions (EOFs).
Variables include the 200 hPa streamfunction (<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), the 2 m
temperature (2mT), the sea surface temperature (SST), and outgoing longwave
radiation (OLR). Precipitation (Precip) from the Climate Hazards group Infrared
Precipitation with Stations (Funk et al., 2015) Version 2.0 dataset
(<uri>https://data.chc.ucsb.edu/products/CHIRPS-2.0/</uri>, last access: 21 October 2021) is also used. JRA-55 and
CHIRPS are used because they are available in near real time (2–3 d lag)
and serve as the basis for experimental real-time forecasts and because they are
available back to at least 1982. <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, SST, and OLR
anomalies are used on a 2.5 <inline-formula><mml:math id="M14" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal grid, while 2mT and Precip are used on a 0.5 <inline-formula><mml:math id="M16" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.5<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid. The EOFs and principal components (PCs) retained in <inline-formula><mml:math id="M18" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula> are not sensitive to the gridding used (not shown).</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.99}[.99]?><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Variable</oasis:entry>
         <oasis:entry colname="col2">Domain</oasis:entry>
         <oasis:entry colname="col3">% variance</oasis:entry>
         <oasis:entry colname="col4">No. EOFs</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">explained</oasis:entry>
         <oasis:entry colname="col4">retained</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">SST</oasis:entry>
         <oasis:entry colname="col2">20<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–20<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 0–357.5<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">63 %</oasis:entry>
         <oasis:entry colname="col4">8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">OLR</oasis:entry>
         <oasis:entry colname="col2">20<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–20<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 0–357.5<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">54 %</oasis:entry>
         <oasis:entry colname="col4">23</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">0–90<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 0–357.5<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">63 %</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Precip</oasis:entry>
         <oasis:entry colname="col2">15–48<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 40–80<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">70 %</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2mT</oasis:entry>
         <oasis:entry colname="col2">15–45<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 40–90<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>
         <oasis:entry colname="col3">77 %</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Linear inverse model</title>
      <p id="d1e583">A LIM assumes that the evolution of a subset of climate anomalies, defined
in the state vector <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula>, can be approximated as the sum of
a slowly evolving, potentially predictable component and a
rapidly decorrelating, unpredictable component. Here we consider the
evolution of the following climate variables (Eqs. 1–2; Table 1):

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M33" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="bold">x</mml:mi><mml:mo>=</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:mi mathvariant="normal">SST</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">OLR</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">mT</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">Precip</mml:mi><mml:mo mathvariant="italic">}</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi mathvariant="bold">Lx</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">F</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where the dynamic operator <inline-formula><mml:math id="M34" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula> represents the predictable
component of the evolution and <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">F</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
represents state-independent white noise forcing that is unpredictable. The
LIM employed in this study is created using an <inline-formula><mml:math id="M36" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula> designed
to capture “slow and predictable” weekly-timescale variability, as in past
studies (Winkler et al., 2001; Newman et al., 2003; Albers and Newman, 2019;
Breeden et al., 2020; Henderson et al., 2020). Any predictable processes
represented by the variables in <inline-formula><mml:math id="M37" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula> are aggregated in the
operator <inline-formula><mml:math id="M38" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>, and their net effect on the predictable
evolution of the system is leveraged in the LIM (i.e., ENSO/MJO
variability). To the extent the key predictable relationships between the
LIM variables, whether truly linear or nonlinear, can be estimated linearly
through the covariance between model variables (Eq. 3), they can be
represented by <inline-formula><mml:math id="M39" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>. As such, the LIM can include more
information than what is retained in models based on the linearized
equations of motion that explicitly exclude nonlinear effects.</p>
      <p id="d1e722"><?xmltex \hack{\newpage}?>Consistently with focusing on the predictable, weekly varying component of the
system evolution, the climate anomalies used in the LIM were calculated by
removing the 40-year daily climatology and then applying a 7 d mean.
Practically, one cannot use anomalies occurring <italic>after</italic> the initialization date to
make a forecast, so instead of a centered 7 d mean, the prior 6 d is
averaged with the initialization date's anomalies to create the 7 d
running-mean anomalies. Many variable combinations and regional domains were
tested, and the combination used here was found to produce the highest
precipitation forecast skill during SFOs over southwest Asia. Since the
leading  empirical orthogonal functions (EOFs) retained in <inline-formula><mml:math id="M40" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula> are not sensitive to small
changes in the 2mT and Precip domains selected, LIM forecasts and SFOs are
also not sensitive to small changes in the regional domains. Note that the
influence of variables that are not explicitly included in this LIM, for
instance slowly evolving soil moisture, can still be implicitly included in
the LIM variables, such as 2mT.</p>
      <p id="d1e736">The instantaneous <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and 5 d lagged
covariance <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> between the state
vector components are used to determine <inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M44" display="block"><mml:mrow><mml:mi mathvariant="bold">L</mml:mi><mml:mo>=</mml:mo><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>×</mml:mo><mml:mi mathvariant="normal">inv</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          As a practical consideration to reduce the dimensionality of
<inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>, each variable in <inline-formula><mml:math id="M46" display="inline"><mml:mi mathvariant="bold">x</mml:mi></mml:math></inline-formula> is truncated
using EOF analysis, where enough EOFs are
retained to capture most of the variance in each variable and region (Table 1). The covariance and lagged covariance are then computed using the
principal components that are retained.</p>
      <p id="d1e830">A specific training lag <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> must be selected to compute
the lagged covariance. If the system were perfectly linear and forced by
white noise, <inline-formula><mml:math id="M48" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula> would not be sensitive to the training
lag, but in practice there are constraints on the range of training lags
that are appropriate, which is determined using the “<inline-formula><mml:math id="M49" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> test” (Penland and
Sardeshmukh, 1995). For this LIM, a training lag of 5 d is used, which
is consistent with the range of stable training lags for LIMs similar to the
one used here (Winkler et al., 2001; Newman et al., 2003; Breeden et al., 2020;
Henderson et al., 2020). For further information on the sensitivity of weekly
LIMs to training lag and additional parameters, the reader is referred to
Sect. 5 of Winkler et al. (2001).</p>
      <p id="d1e859">Similarly to output from numerical forecast models, for each initialization
and lead time <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>, the LIM generates forecasts of the state vector,
<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> (Eq. 4; Fig. 1), by propagating the initial
conditions <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mi mathvariant="bold">x</mml:mi><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">0</mml:mn></mml:mfenced></mml:mrow></mml:math></inline-formula> forward in time.
In the LIM, the propagator <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mi mathvariant="bold">G</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is
determined from <inline-formula><mml:math id="M54" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula> by solving the homogeneous component
of Eq. (2) (Penland and Sardeshmukh, 1995). For this study, forecasts are
generated at a daily time step out to a lead time of 42 d. We note that
because the LIM is trained on daily anomalies with a 7 d running mean
applied, the forecasts are also lower-frequency in nature.
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M55" display="block"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="bold">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="bold">x</mml:mi><mml:mfenced close=")" open="("><mml:mn mathvariant="normal">0</mml:mn></mml:mfenced><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="bold">L</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mi mathvariant="bold">x</mml:mi><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">0</mml:mn></mml:mfenced><mml:mi mathvariant="bold">G</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>
          LIM forecast skill is assessed using 10-fold cross-validation, done by
removing 10 % of the data, re-computing <inline-formula><mml:math id="M56" display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>, and
generating forecasts for the 10 % of initializations that were removed
(e.g., Albers and Newman, 2019). This process is repeated to generate
forecasts for 1982–2020, initialized daily from 1 January–20 March each
year. LIM forecast skill is assessed in two ways: using the anomaly correlation
coefficient (ACC), where the LIM forecast and un-truncated (i.e.,
full-field) verification precipitation is compared at each grid point, and
using the pattern correlation coefficient (PCC), where the LIM forecast and
un-truncated verification precipitation are compared at each time step using
the uncentered, cosine-weighted correlation between all grid points over
southwest Asia (e.g., Albers and Newman, 2019). The ACC measures skill over the
full period while preserving geographic information about skill, while the PCC
measures the average skill over the entire southwest Asian domain but
maintains information about how individual forecasts performed. Average forecasts using different lead times are categorized as follows: week 1 forecast lead times 1–7 d, week 2 forecast lead times 8-14 d, week 3 forecast lead times 15–21 d, week 4 forecast lead times 22–28 d, week 5 forecast lead times 29–35 d, and
week 6 forecast lead times 36–42 d. Weeks 3–4 and weeks 5–6 forecasts are determined
using the corresponding 14 d averaged forecasts at the corresponding lead
times.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e970">Schematic of LIM forecast for a lead time of 15 d.</p></caption>
          <?xmltex \igopts{width=142.26378pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f01.png"/>

        </fig>

<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Forecasts of opportunity</title>
      <p id="d1e986">A common approach to anticipate SFOs is to focus on a specific
predictability source, e.g., strong tropical heating associated with ENSO or
the MJO. However, many potentially predictable signals may be evolving at
any given time (Albers et al., 2022), and the constructive or destructive
interference between each signal's teleconnections may enhance or degrade
the overall predictable forecast signal for variables that we are interested
in, e.g., southwest Asian precipitation. Thus, it is more desirable to use a
method that considers <italic>all</italic> relevant signals and their combined influence to
anticipate the overall likelihood of a skillful forecast over the region of
interest. Here, following Sardeshmukh et al. (2000), the theoretical
expected skill of a perfect, infinite ensemble member forecast, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Eq. 5), is selected to identify SFOs, based on the
method's past success. In particular, <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is calculated using
the pattern correlation version of the LIM signal-to-noise ratio, <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>
(Eq. 6; Newman et al., 2003), and is evaluated over the southwest Asian
domain for each forecast lead time <inline-formula><mml:math id="M60" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> and each initialization date <inline-formula><mml:math id="M61" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>.
As a result, <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are a function of time but not
space:

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M64" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msup><mml:mfenced close="}" open="{"><mml:mrow><mml:mfenced close="]" open="["><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">0.5</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd><mml:mtext>6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">tr</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="bold">F</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:mo>]</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">tr</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="bold">E</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> is determined using <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi mathvariant="bold">F</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, the forecast signal covariance matrix determined at a given lead
time, which indicates the strength of the predictable signal in the
forecasts, and <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi mathvariant="bold">E</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula>, the
forecast error covariance matrix which represents lead-dependent,
unpredictable “noise”:

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M68" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="bold">F</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:mo>〈</mml:mo><mml:mover accent="true"><mml:mi mathvariant="bold">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mfenced close=")" open="("><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfenced><mml:mover accent="true"><mml:mi mathvariant="bold">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mo>′</mml:mo></mml:msup><mml:mo>〉</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="bold">E</mml:mi><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="bold">G</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:msub><mml:mi mathvariant="bold">C</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mi mathvariant="bold">G</mml:mi><mml:msup><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:mo>′</mml:mo></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              where <inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> denotes the matrix transpose. Note that <inline-formula><mml:math id="M70" display="inline"><mml:mi mathvariant="bold">E</mml:mi></mml:math></inline-formula> is not a function of time, which is consistent with the assumption of state-independent noise (Eq. 2), but does vary with forecast lead time <inline-formula><mml:math id="M71" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>.</p>
      <p id="d1e1378">We define SFOs as the top 20 % of expected-skill forecasts as this subset
accurately identifies significantly more skillful forecasts for a range of
lead times (Fig. 2). The ACC and PCC during these dates are compared to the
skill when, instead of expected skill, the top 20 % of Niño3.4
amplitude and RMM amplitude values are used to identify periods of elevated skill.
The skill during these three subsets of forecasts (<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">∞</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>,
Niño3.4, RMM) is compared to the skill of the remaining 80 % of
expected-skill forecasts, and the 95 % confidence level in the skill
differences during the three subsets is assessed nonparametrically, using
bootstrapping with replacement. Similar skill differences were found for a
range of 10 %–25 % of the forecasts in the SFO group, and 20 % was chosen
because it provided the greatest number of samples – useful for further
separating forecasts by ENSO and MJO phase later – but was small enough so that
the subset has significantly elevated skill.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1394">PDFs of actual skill measured by pattern correlation (PCC), for
the top 20 % and bottom 20 % of expected-skill dates for weeks of lead times <bold>(a)</bold> 2 to <bold>(d)</bold> 5. The green circles represent the bootstrapped median values, and the black circles represent the bootstrapped 95th-percentile values.</p></caption>
            <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f02.png"/>

          </fig>

</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <label>2.2.2</label><title>Relative risk</title>
      <p id="d1e1417">A relative-risk ratio is used to quantify shifts in the likelihood of an SFO
occurring as a function of ENSO, MJO, and SPCZ OLR strength. This is done,
for each index, by determining the fraction (FRAC) of SFOs initialized on days with
index values of varying amplitude:
              <disp-formula id="Ch1.E9" content-type="numbered"><label>9</label><mml:math id="M73" display="block"><mml:mrow><mml:mi mathvariant="normal">FRAC</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">no</mml:mi><mml:mo>.</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SFOs</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">no</mml:mi><mml:mo>.</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">dates</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            For ENSO and SPCZ OLR, changes in SFOs during positive and negative index
values of varying threshold are considered, while RMM is always
positive. Instead, we assess changes in SFOs during MJO phases 2–3 or 6–7
and increasing RMM thresholds. To determine the relative risk of an SFO
compared to the probability of one occurring on any random day, we divide
FRAC calculated for each threshold and index group by 0.2 – since for the top
20 % of expected-skill dates, the chance of one occurring on any date in
the forecast period is 0.2:
              <disp-formula id="Ch1.E10" content-type="numbered"><label>10</label><mml:math id="M74" display="block"><mml:mrow><mml:mi mathvariant="normal">relative</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">risk</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">FRAC</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            As an example, for weeks 3–4 SFOs when Niño3.4 <inline-formula><mml:math id="M75" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1.5, 117
SFOs are found during the 269 d exceeding that threshold, corresponding
to FRAC <inline-formula><mml:math id="M76" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.44 and relative risk <inline-formula><mml:math id="M77" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.2. The robustness of these
estimates is evaluated by determining the 95 % confidence bounds around
the relative-risk estimates using bootstrapping with replacement.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e1501">Section 3.1 shows how expected skill can stratify skillful and unskillful
forecasts to identify SFOs and demonstrates how strong ENSO and MJO phases
increase the likelihood of an SFO occurring. Section 3.2 reveals how
anomalous SPCZ OLR is observed during both wet and dry SFOs, as well as how
predictable patterns during El Niño and La Niña conditions are
associated with unique circulation features.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Identifying forecasts of opportunity</title>
      <p id="d1e1511">The distribution of LIM forecast skill, measured by the PCC during the top and
bottom 20 % of theoretical expected-skill forecasts (Eq. 5), confirms
that the high-expected-skill group successfully identifies more skillful
forecasts than the low-expected-skill group (Fig. 2). Note that for each
lead time, the high-expected-skill and low-expected-skill dates identified are not
necessarily the same. For lead times of 2–4 weeks, both the median and
the 95th-percentile values of the PDFs of forecasts initialized on high-expected-skill dates show statistically significant shifts towards higher
PCC, with the greatest skill increases, relative to the bottom 20 % group,
at the shortest lead time of 2 weeks (Fig. 2a). The distribution of the week 2
PCC is also the narrowest for the high-expected-skill group, a reflection of
the more deterministic nature of forecasts at this lead time, particularly
during periods of high signal-to-noise ratios (Eq. 6). As lead time
increases, the distribution of skill widens as forecast uncertainty
increases, so that by week 5, the medians are indistinguishable between the
two PCC distributions. Still, some skillful forecasts remain at week 5 in
the high-expected-skill group, shown by the statistically significant shift
in the 95th percentile of the PCC.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1516">The anomaly correlation coefficient (ACC) for weeks 3–4 forecasts,
evaluated from January–March 1982–2020. <bold>(a)</bold> The ACC for all dates in the record; <bold>(b)</bold> the ACC for the 20 % of forecasts initialized with the highest expected skill; <bold>(c)</bold> the ACC for the 20 % with the highest Niño3.4 amplitude; <bold>(d)</bold> the ACC for the 20 % with the highest RMM amplitude. The black stippling indicates where the skill of the top 20 % of forecasts in each group is statistically significantly different from the skill of the remaining 80 % of forecasts
at the 95 % confidence level, determined nonparametrically with
bootstrapping.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1539">As in Fig. 3 but for weeks 5–6 forecasts.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f04.png"/>

        </fig>

      <p id="d1e1549">Subseasonal precipitation skill, evaluated using the ACC for weeks 3–4 and weeks 5–6,
is low, as discussed in past studies, but increases substantially during
high-expected-skill periods (Figs. 3–4). The LIM “all dates” weeks 3–4 skill of 0.2–0.3 ACCs exceeds the week 3 skill of most of the subseasonal-to-seasonal (S2S) models evaluated by
de Andrade et al. (2018) for November–March 1999–2009 (compare Fig. 3a to
their Fig. 1). Comparing the three approaches to anticipating SFOs – high expected skill, Niño3.4, and RMM – expected skill most successfully
anticipates SFOs at both weeks 3–4 and weeks 5–6. The location of maximum skill
shifts southeastward from weeks 3–4 to 5–6, with skill also weakening at
longer lead times as expected. While there are some regions experiencing a
skill increase during the top 20 % of Niño3.4 and RMM amplitude dates,
the increases are mainly indistinguishable from the skill of the remaining
forecasts (Figs. 3c, d and 4c, d). Splitting the Niño3.4 index to consider
only strong El Niño or La Niña events indicates that some regions do
experience elevated skill during both phases, though in different, localized
regions that only cover a limited portion of the region compared to the
forecasts identified using expected skill (Fig. S1 in the Supplement).</p>
      <p id="d1e1552">Considering PCC during the high-expected-skill, Niño3.4, and RMM dates
confirms that forecasts initialized during periods of high expected skill
generally have higher PCCs than those identified using Niño3.4 and RMM
(Fig. 5). For lead times of between 2–4 weeks, statistically significant median
PCC shifts, as well as the increased probability
density of forecasts with PCC <inline-formula><mml:math id="M78" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5, reflect the increase in skill. By week 5, the
distributions of PCC during high-expected-skill and high-Niño3.4 dates
become indistinguishable, which is consistent with greater similarity in the regions
of skill found using Niño3.4 and expected skill at weeks 5–6 (Fig. 4).
Overall, the expected-skill metric is more effective at anticipating SFOs
than Niño3.4 and RMM.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1564">PDFs of the precipitation PCC for all forecasts (black lines) and the
20 % of forecasts with the highest-expected-skill (blue), the highest-Niño3.4 (red),
and the highest-RMM (green) initializations. The bootstrapped confidence intervals for
the median and 95th percentile of the distribution are shown with the
markers.</p></caption>
          <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f05.png"/>

        </fig>

<sec id="Ch1.S3.SS1.SSSx1" specific-use="unnumbered">
  <?xmltex \opttitle{Relating SFOs to Ni\~{n}o3.4 and RMM indices}?><title>Relating SFOs to Niño3.4 and RMM indices</title>
      <p id="d1e1579">The advantage of using high expected skill to anticipate SFOs is that it measures when the combined signal of <italic>all</italic> forcings (e.g., ENSO, MJO) is high relative to unpredictable noise. High expected skill occurs during periods
of constructive interference between signals, while low expected skill
reflects periods of deconstructive interference (e.g., Farrell, 1988; Farrell
and Ioannou, 1996; Albers and Newman, 2019), and such interference is more
intermittent than the individual forcing elements (Figs. 6, 8). As such,
despite what is shown in Figs. 2–4, many high-expected-skill dates occur
during strong ENSO and MJO events, as indicated by the overlay of SFOs
(black dots) with time series of Niño3.4 (Fig. 6) and RMM (Fig. 8). The
bottom 20 % of expected-skill forecasts are also shown by the vertical
light gray lines to contrast the higher-frequency expected skill with the
lower-frequency Niño3.4 and RMM. The correspondence to Niño3.4 is
considered first. Both El Niño events of 1983 and 2016 coincided with
high-expected-skill dates at weeks 3–4 and 5–6, though on different dates;
conversely, the 1998 event was not associated with any high-expected-skill
dates at weeks 5–6 but was for weeks 3–4. Strong La Niña events, such as in 1999, also reflect periods of high expected skill. Still, there are many
high-expected-skill forecasts initialized on dates with weak Niño3.4
values, as in 2017, since other processes – including ENSO-related heating
not captured by Niño3.4 – can produce a high signal-to-noise ratio.
Moreover, some of the lowest-expected-skill dates occur during strong ENSO
events, such as in 2016 for weeks 3–4 at the beginning of February,
suggesting other processes may have been destructively interfering with the
ENSO-related component.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1587">The color shading shows the Niño3.4 index and is the same in
both panels. The black dots indicate the top 20 % of expected-skill
forecasts, and the gray vertical lines represent the bottom 20 % of
expected-skill forecasts, for weeks 3–4 forecasts <bold>(a)</bold> and weeks 5–6 forecasts <bold>(b)</bold>.</p></caption>
            <?xmltex \igopts{width=389.802756pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f06.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1604">The black line shows the relative risk, relative to the risk on
any given day, of an SFO, meaning one of the top 20 % of expected-skill
dates, occurring when the Niño3.4 index is greater than various
thresholds, with 95 % confidence intervals in gray shading.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f07.png"/>

          </fig>

      <p id="d1e1614">High Niño3.4 index amplitude during both El Niño and La Niña
events leads to increases in the risk of SFO occurrence, though more
strongly during the former than the latter (Fig. 7). There is a greater
relative risk for SFOs in weeks 5–6 than weeks 3–4, suggesting that at
longer lead times within the subseasonal forecast period, ENSO conditions
are increasingly important for SFOs. However, it is important to note that
skill during these periods is overall lower than for weeks 3–4 (Figs. 3–4),
which could be due to the limited capability of ENSO alone to impact
predictability and/or to elevated noise. The asymmetric relative risk during
El Niño and La Niña conditions may reflect the fact that there are
more frequent high-amplitude El Niño events than La Niña events,
increasing the number of samples at higher Niño3.4 thresholds. Indeed,
Niño3.4 exceeds 1.5 <inline-formula><mml:math id="M79" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C on 269 d, compared to 192 d where
Niño3.4 is less than <inline-formula><mml:math id="M80" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5 <inline-formula><mml:math id="M81" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The stronger response during El
Niño conditions than La Niña could also be consistent with Hoell et
al. (2018a), who found precipitation shifts during both CP and EP El
Niño events but only CP La Niña events, although future work is
needed to better explore these nuances.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1644">As in Fig. 6 but for the amplitude of the RMM index during <bold>(a)</bold> MJO phases 2–3 and <bold>(b)</bold> MJO phases 6–7 and for weeks 3–4 expected-skill dates.</p></caption>
            <?xmltex \igopts{width=389.802756pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f08.png"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e1661">As in Fig. 7 but for weeks 3–4 expected skill and for varying
RMM amplitude during either <bold>(a)</bold> MJO phases 2–3 or <bold>(b)</bold> MJO phases 6–7.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f09.png"/>

          </fig>

      <p id="d1e1676"><?xmltex \hack{\newpage}?>Discerning a relationship between MJO phases 2–3 and 6–7, the phases that
impart known teleconnections to southwest Asian precipitation (Hoell et al., 2018b), can be more difficult given the more transient nature of the MJO
compounded with transient expected skill (Fig. 8). Only the relationship
between RMM and weeks 3–4 expected skill is considered, as an MJO
teleconnection at 5–6-week lead times is not physically plausible (e.g.,
Tseng et al., 2018). Still, we do find that particularly strong events for
phases 2–3 and 6–7 increase the relative risk of weeks 3–4 SFOs, though
sampling introduces spread into these estimates (Fig. 9). Some particularly
high-amplitude MJO events, including phases 2–3 in 1985 and 1993 and phases
6–7 in 2005 and 2018, overlap with periods of weeks 3–4 high expected skill,
while some weaker-amplitude events overlap with some of the lowest-expected-skill dates, such as phases 2–3 in late January 2002. The strong RMM phases 6–7
are also associated with an increase in the relative risk of SFOs, which
increases at lower RMM thresholds compared to in phases 2–3 and does not display
the exponential increase at the highest thresholds. These subtle differences
in relative-risk sensitivity could reflect true differences in the MJO
teleconnection to the region or could be due to sampling, as there is high
uncertainty in the relative-risk estimates given the small number of events
observed at such high thresholds.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Characteristics of predictable dry and wet initializations</title>
      <p id="d1e1689">This section considers the composite patterns preceding predictable wet and
dry periods 18 d earlier, revealing the role of anomalous heating near
the SPCZ. Next, composite wet and dry periods are split by their Niño3.4 sign,
revealing how different circulation responses during each phase produce
same-signed precipitation anomalies over southwest Asia.</p>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>All initializations</title>
      <p id="d1e1699">First, we consider the patterns preceding anomalously wet and dry periods
regardless of ENSO phase, where “wet” and “dry” are defined using the top
and bottom terciles of southwest Asian precipitation anomalies,
respectively. Wet and dry dates that were associated with weeks 3–4 high-expected-skill dates initialized 18 d earlier and were also
characterized by a PCC <inline-formula><mml:math id="M82" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0 are considered. A lead time of 18 d is chosen because it falls within the weeks 3–4 forecast period and
provides the clearest circulation structures, which are similar but weaker
at longer lead times (not shown). An 18 d lag is also consistent with the
circulation response to tropical diabatic heating anomalies discussed in Jin
and Hoskins (1995), which peaked about 15 d after the heating occurred.
For these skillful, high-expected-skill forecasts associated with the
development of anomalously wet or dry precipitation anomalies, we consider
the composite circulation and heating patterns observed at the time of
initialization, meaning 18 d before the anomalous precipitation was
observed.</p>
      <p id="d1e1709">Figure 10 shows that during weeks 3–4 SFOs initialized before predictable
wet and dry periods over southwest Asia, anomalies are roughly equal and
opposite in sign. Before dry periods, positive OLR anomalies are located
over the western and central tropical Pacific, signifying suppressed
convection, while a 200 hPa anticyclone (positive <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> anomaly) is located over southwest Asia, consistent with
downward vertical motion and suppressed precipitation. Conversely,
predictable anomalously wet periods are associated with enhanced anomalous
central Pacific convection and a cyclonic <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
anomaly over southwest Asia. One feature present during dry initializations
is a small but statistically significant negative OLR anomaly in the eastern
Indian Ocean, which does not have a counterpart during wet initializations.
Southwest Asian precipitation is strongly linked to heating variability in
this location (Hoell et al., 2012), and the results here suggest that the
relationship might be particularly important for anomalously dry periods.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e1736">Composite OLR (color shading) and <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (black/gray contours) anomalies, during <bold>(a)</bold> high-expected-skill initializations verified on anomalously dry days 18 d later, <inline-formula><mml:math id="M86" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M87" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 142 d, and <bold>(b)</bold> high-expected-skill initializations verified on anomalously wet days 18 d later, <inline-formula><mml:math id="M88" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M89" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 163. The black
contours show positive (anticyclonic) streamfunction anomalies, and the gray
contours show negative (cyclonic) streamfunction anomalies, contoured at an interval
of 3 <inline-formula><mml:math id="M90" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M93" 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> beginning at <inline-formula><mml:math id="M94" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>3 <inline-formula><mml:math id="M95" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M98" 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>. Only anomalies that are statistically significant at the 95 %
confidence level are shown.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f10.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><?xmltex \opttitle{El Ni\~{n}o and La Ni\~{n}a initializations}?><title>El Niño and La Niña initializations</title>
      <p id="d1e1884">Section 3.1 indicated that, while anticipating SFOs based on the Niño3.4
index alone is less successful than expected skill (Figs. 3–4), periods of
strong ENSO activity increase the likelihood of a forecast of opportunity
occurring, particularly during the strongest events (Fig. 7). During either
ENSO phase, periods of anomalously high and low precipitation can occur due
to transient disturbances forming along the subtropical jet. However, the
manner in which precipitation anomalies develop differs between El Niño
and La Niña, due to ENSO's influence on the mean jet and baroclinic
waves (Shapiro et al., 2001), whose life cycles differ under different mean
states (Thorncroft et al., 1993). This section examines how predictable wet
and dry initializations differ by ENSO phase given the hypothesized
differences in teleconnections in each phase.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e1889">As in Fig. 10 but for groups divided by Niño3.4 <inline-formula><mml:math id="M99" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0
(“La Niña”) or Niño3.4 <inline-formula><mml:math id="M100" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0 (“El Niño”) and with
negative SST anomalies in blue contours and positive SST anomalies shown
in red, at a contour interval of 0.5 <inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f11.png"/>

          </fig>

      <p id="d1e1921">Splitting dry and wet forecast initializations into periods when Niño3.4
is positive or negative to reflect El Niño or La Niña conditions,
without losing any samples, indicates that even when preceding same-signed
precipitation anomalies, El Niño and La Niña conditions are
associated with different large-scale circulation patterns (cf. Fig. 11a, c and b, d). By construction, there are clear differences in SST and
OLR associated with El Niño and La Niña conditions, as well as North
Pacific <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> anomalies associated with ENSO-like
tropical heating (Winkler et al., 2001; Breeden et al., 2020; Henderson et al., 2020). During La Niña conditions, dry periods include an anticyclonic
anomaly over southwest Asia, while during dry El Niño initializations
there are cyclonic features north and east of southwest Asia and weak
anomalies directly over the region (cf. Fig. 11a, c). In contrast to the
circulation pattern during dry El Niño periods (Fig. 11c), during wet
periods, El Niño conditions are associated with an amplified
<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pattern, with two high-amplitude cyclonic
anomalies located over Eurasia (Fig. 11d). Conversely, at the time of
initialization during wet La Niña periods, negligible <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> anomalies are observed (Fig. 11b).</p>
      <p id="d1e1958">What distinguishes rainy La Niña or El Niño periods from dry La
Niña or El Niño periods? While the heating and SST dipole patterns
are consistent with each ENSO phase for both wet and dry periods, there are
differences in heating strength and location (cf. Fig. 11a, b and c, d).
Dry La Niña initializations include stronger negative SST anomalies and
suppressed convection in the central Pacific compared to rainy periods,
which instead involve enhanced convection over the Maritime Continent. Dry
El Niño periods include stronger suppressed convection over the Maritime
Continent than wet El Niño dates, coinciding with a hint of a wave train
emanating from the eastern Pacific across North America and the North Atlantic.
Dry La Niña dates are more common than wet La Niña dates, 84 vs. 67 d, while wet El Niño dates are more common than dry El Niño
dates, 96 vs. 57 d, which is consistent with past research linking seasonal mean
departures of southwest Asian precipitation to ENSO (Hoell et al., 2018a).</p>
      <p id="d1e1961">Differencing the dry and wet composites between each ENSO phase reveals the
common element of suppressed SPCZ convection and cooler central Pacific SSTs
during dry periods relative to wet periods (Fig. 12). Dry periods during El
Niño conditions are associated with warmer SSTs in the eastern Pacific than are
wet periods (Fig. 12b), while no such differences in SSTs or OLR are
observed in the eastern Pacific during La Niña conditions (Fig. 12a). While
distinct from one another, the <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> patterns
during both El Niño and La Niña conditions place an anomalous
anticyclone over southwest Asia during dry events, consistent with
suppressed precipitation. The <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mn mathvariant="normal">200</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> patterns
during dry versus wet periods differ, with La Niña conditions displaying
weak anticyclonic anomalies in the subtropical North Pacific and North
Atlantic and El Niño conditions associated with an upper-level wave
train emanating from the eastern tropical Pacific, across the North Atlantic
to Europe, potentially linked to the anomaly over southwest Asia. The
orientation of such a wave train is consistent with the evolution described
by Shaman and Tziperman (2005), who found a northeastward-propagating wave
train emanating from the eastern central Pacific during strong ENSO events,
which ultimately modulated Tibetan snow depth. Thus, while the heating
difference between dry and rainy periods is similar regardless of the ENSO
phase, the impact of the anomalous heating on the circulation is different
but coincidentally yields a reduction in precipitation over southwest Asia.
The different circulation responses are consistent with the modified mean
states of each ENSO phase, though more work is required to further
understand these nuanced relationships, preferably with a larger sample
size. Dry baroclinic modeling experiments could be useful in disentangling
the role of the basic state and thermal forcing in producing this response.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e1988">Composite difference, dry <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> wet, during <bold>(a)</bold> La Niña
conditions (Fig. 11a–b) and <bold>(b)</bold> El Niño conditions (Fig. 11c–d). Plotting conventions are as in Fig. 11, except the contour interval for SST anomalies (blue and red contours) is 0.25 <inline-formula><mml:math id="M108" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f12.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Relative risk associated with SPCZ OLR</title>
      <p id="d1e2027">Given the OLR anomalies in the SPCZ region noted during both predictable wet
and predictable dry forecast initializations (Figs. 10, 12), a time series of OLR
over the region was selected for a final metric to consider related to weeks 3–4 SFOs. Similarly to considering Niño3.4 and RMM, the relative risk of
an SFO occurring increases significantly as the standard deviation of SPCZ
OLR anomalies increases (Fig. 13). The response during negative and positive
SPCZ OLR anomaly values is more symmetric than the risk associated with an
increasing Niño3.4 threshold, which indicated a greater relative-risk
increase during El Niño than during La Niña conditions (Fig. 7), or
comparing the impact of MJO phases 2–3 vs. 6–7 (Fig. 9). This symmetry is
further supported with the 18 d lagged regression of the southwest Asian
precipitation time series with OLR (Fig. S2), although the regression
pattern OLR anomalies are weaker than the composite OLR during the SFOs
considered in Figs. 10 and 12. The SPCZ OLR time series is correlated with the
Niño3.4 index at <inline-formula><mml:math id="M109" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M110" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M111" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.25, an indication that the SFOs associated
with SPCZ OLR are not redundant with Niño3.4-related SFOs and therefore
contain additional information about SFOs related to tropical variability.
As such, the expected-skill approach to SFOs benefits from measuring shifts
in the likelihood of a forecast of opportunity captured by several distinct
indices tracking tropical variability, Niño3.4, RMM, and SPCZ OLR, a
distinct advantage over using an index that tracks only one of these processes
(Figs. 3–4).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e2053">As in Fig. 7 but for using the standard deviation of the SPCZ
OLR anomaly time series, calculated using the boxed region in Fig. 10 and
for weeks 3–4 expected skill.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://wcd.copernicus.org/articles/3/1183/2022/wcd-3-1183-2022-f13.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e2074">In this study, precipitation SFOs are considered over southwest Asia using
LIM expected skill, a metric related to the forecast signal-to-noise ratio
that leverages the constructive interference of all signals impacting
predictability. Strong El Niño, La Niña, and MJO phase 2–3 and phase 6–7
conditions increase the chances that an SFO occurs. A third tropical heating
index, based on anomalous OLR in the SPCZ region, also increases the risk of
an SFO (Fig. 13). The correspondence between expected skill and several
indices highlights the advantage of using expected skill, in that all of
these flavors of tropical heating are registered as high signals. However,
there are still SFOs that do not correspond to any one of these indices,
since other processes, potentially not tropically driven, can produce a high
signal too. Future work could focus on categorizing all SFOs to examine
these potential additional factors.</p>
      <p id="d1e2077">In addition to the confirmed influence of ENSO and MJO activity on southwest
Asian precipitation, anomalous heating across the SPCZ region is a common
element among predictable wet and dry initializations and increases the
relative risk of an SFO. Heating in this region is also associated with
different circulation patterns during El Niño and La Niña conditions
(Fig. 12). How these different circulation patterns are related to
similarly located anomalous heating anomalies is currently not well
understood but likely involves the modified tropopause-level waveguide
present during each ENSO phase, which modulates the extratropical response
to tropical heating (Sardeshmukh and Hoskins, 1988; Newman and Sardeshmukh,
1998; Shapiro et al., 2001). Dry baroclinic modeling experiments with
idealized heating could be used to quantify the contribution of tropical
heating over the Indian Ocean and western Pacific affecting the circulation
over southwest Asia on subseasonal timescales. We also note that, while
widely used, ENSO indices such as Niño3 or Niño3.4 do not capture
the full spectrum of ENSO variability (Penland and Sardeshmukh, 1995; Newman
et al., 2009; Gehne et al., 2014; Henderson et al., 2020; Albers and Newman,
2021). Future work could employ the dynamical decoupling approach of
Henderson et al. (2020) to isolate the ENSO signal and its impact on
precipitation SFOs more holistically.</p>
      <p id="d1e2080">The association between forecasts of opportunity and the MJO is less
constrained given the higher-frequency nature of the MJO and small sample
size once RMM is sorted by phase, but it still indicates a role for strong MJO
events in phases 2–3 or 6–7 to increase the likelihood of a weeks 3–4 SFO
occurring, consistent with prior studies (Cannon et al., 2017; Hoell et al., 2018b). Further suggesting a role for MJO-like heating, predictable heating
patterns associated with forecasts of opportunity indicate a role for
anomalous convection over the Indian Ocean during dry periods, consistent with
MJO phases 2–3 suppressing southwest Asian precipitation (Fig. 10a). Future
work could employ large climate simulation output to enhance sample size and
revisit the MJO–expected-skill relationship and the extent the model can
reproduce the mean state and the MJO itself. Another remaining question that
could be addressed more aptly with a larger sample size is how ENSO and the
MJO act together to impact SFOs for southwest Asian precipitation events,
particularly concerning their magnitude and duration, which was beyond the
scope of this study but merits further investigation.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e2088">The JRA-55 Reanalysis data used in this study are freely available at <ext-link xlink:href="https://doi.org/10.5065/D6HH6H41" ext-link-type="DOI">10.5065/D6HH6H41</ext-link> (Japan Meteorological Agency, 2013), and CHIRPS precipitation is freely available at <uri>https://data.chc.ucsb.edu/products/CHIRPS-2.0/global_daily/netcdf/p25/</uri> (Climate Hazards Center, 2021). The RMM index was accessed at no cost from the Australian Bureau of Meteorology here: <uri>http://www.bom.gov.au/climate/mjo/graphics/rmm.74toRealtime.txt</uri> (Commonwealth of Australia, 2022).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e2100">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/wcd-3-1183-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/wcd-3-1183-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2109">MLB wrote code for calculations, produced all figures, and wrote the manuscript. JRA provided technical expertise on the LIM
and subseasonal forecasting, frequent guidance on computations and figures,
and made edits to the manuscript. AH secured funding for this
project, provided expertise on southwest Asia, provided frequent guidance on figures, and made edits to the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2115">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e2121">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2127">The authors gratefully acknowledge support from the Famine Early Warning
Systems Network and helpful suggestions from the two anonymous reviewers.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2132">This research has been supported by the United States Agency for International Development (grant no. AID-OFDA-T-17-00002).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2138">This paper was edited by Daniela Domeisen and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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