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  <front>
    <journal-meta><journal-id journal-id-type="publisher">HESS</journal-id><journal-title-group>
    <journal-title>Hydrology and Earth System Sciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">HESS</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Hydrol. Earth Syst. Sci.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1607-7938</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/hess-21-5493-2017</article-id><title-group><article-title><?xmltex \hack{\vspace*{3mm}}?>Technical note: Combining quantile forecasts and predictive distributions of streamflows</article-title>
      </title-group><?xmltex \runningtitle{Forecast combination}?><?xmltex \runningauthor{K. Bogner et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bogner</surname><given-names>Konrad</given-names></name>
          <email>konrad.bogner@wsl.ch</email>
        <ext-link>https://orcid.org/0000-0002-4361-7751</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Liechti</surname><given-names>Katharina</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zappa</surname><given-names>Massimiliano</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2837-8190</ext-link></contrib>
        <aff id="aff1"><institution>Swiss Federal Institute for Forest, Snow and Landscape Research WSL, Birmensdorf, Switzerland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Konrad Bogner (konrad.bogner@wsl.ch)</corresp></author-notes><pub-date><day>8</day><month>November</month><year>2017</year></pub-date>
      
      <volume>21</volume>
      <issue>11</issue>
      <fpage>5493</fpage><lpage>5502</lpage>
      <history>
        <date date-type="received"><day>17</day><month>May</month><year>2017</year></date>
           <date date-type="rev-request"><day>29</day><month>May</month><year>2017</year></date>
           <date date-type="rev-recd"><day>26</day><month>September</month><year>2017</year></date>
           <date date-type="accepted"><day>4</day><month>October</month><year>2017</year></date>
      </history>
      <permissions>
        
        
      <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://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017.html">This article is available from https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017.html</self-uri><self-uri xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017.pdf">The full text article is available as a PDF file from https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017.pdf</self-uri>
      <abstract>
    <p>The enhanced availability of many different hydro-meteorological modelling
and forecasting systems raises the issue of how to optimally combine this
great deal of information. Especially the usage of deterministic and
probabilistic forecasts with sometimes widely divergent predicted future
streamflow values makes it even more complicated for decision makers to sift
out the relevant information. In this study multiple streamflow forecast
information will be aggregated based on several different predictive
distributions, and quantile forecasts. For this combination the Bayesian
model averaging (BMA) approach, the non-homogeneous Gaussian
regression (NGR), also known as the ensemble model output statistic (EMOS)
techniques, and a novel method called Beta-transformed linear
pooling (BLP) will be applied. By the help of the quantile score (QS) and the
continuous ranked probability score (CRPS), the combination results for the
Sihl River in Switzerland with about 5 years of forecast data will be
compared and the differences between the raw and optimally combined forecasts
will be highlighted. The results demonstrate the importance of applying
proper forecast combination methods for decision makers in the field of flood
and water resource management.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The combination, or aggregation, of differing probability distributions into
a single one could result in beneficial effects, since the differences
between various forecast systems provide a better understanding of the
uncertainty about the target quantities, and the aggregates may reflect more
accurately the information. However,
the biggest advantage of aggregation is that the forecaster is not forced to decide
a priori which forecast system is the most reliable at the actual point of issuing
a forecast, because the combination method will be optimized at each forecast run
by taking into consideration the quality of the forecast from previous time steps.
Thus, the data themselves will automatically lead to the optimal decision
incorporating
all available information about the different deficiencies and strengths of the individual forecast systems.</p>
      <p>In econometrics and related disciplines, the combination of forecasts has a
long tradition starting with <xref ref-type="bibr" rid="bib1.bibx6" id="normal.1"/> suggesting the use of empirical
weights derived from “out of sample” forecast variances. An overview of the
last 40 years of forecast combination in the field of economics
can be found in <xref ref-type="bibr" rid="bib1.bibx48" id="normal.2"/>. <xref ref-type="bibr" rid="bib1.bibx42" id="normal.3"/>
was one of the first who outlined the advantages of forecast combinations in
meteorology and <xref ref-type="bibr" rid="bib1.bibx40" id="normal.4"/> showed different methods of combining the
output of different hydrological models. In <xref ref-type="bibr" rid="bib1.bibx1" id="normal.5"/> different
combination methods for hydrological forecast models are compared.
<xref ref-type="bibr" rid="bib1.bibx14" id="normal.6"/> compare different model averaging approaches, showing that a
simple regression method could result in improvements comparable to more
sophisticated methods.</p>
      <p>In general the challenge of model combination is that, apart from the simple
model averaging methodologies, different weights need to be assigned
according to the quality of the forecast of the preceding days and periods. A
frequently used method for model averaging and forecast combination is the
method of Bayesian model averaging (BMA) introduced by <xref ref-type="bibr" rid="bib1.bibx31" id="normal.7"/> and
<xref ref-type="bibr" rid="bib1.bibx36" id="normal.8"/>, where the weights are based on posterior model probabilities
within a Bayesian framework. The BMA method has been applied in the field of
ensemble forecast calibration (<xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx16" id="altparen.9"/>) and for flood
forecasting purposes, e.g. in <xref ref-type="bibr" rid="bib1.bibx3" id="normal.10"/>, <xref ref-type="bibr" rid="bib1.bibx47" id="normal.11"/>,
<xref ref-type="bibr" rid="bib1.bibx43" id="normal.12"/>, and <xref ref-type="bibr" rid="bib1.bibx23" id="normal.13"/>.</p>
      <p>In <xref ref-type="bibr" rid="bib1.bibx21" id="text.14"/> and <xref ref-type="bibr" rid="bib1.bibx22" id="text.15"/> the term “calibration” is used to
describe the statistical consistency between the distributional forecasts and
the observations and is a joint property of the predictions and the events
that materialize. A state of the art calibration and bias correction method
is non-homogeneous Gaussian regression (NGR), also known as the ensemble
model output statistic (EMOS) technique of <xref ref-type="bibr" rid="bib1.bibx21" id="normal.16"/>. It fits a single
parametric predictive probability density function (pdf) using summary
statistics from the (multi-model) ensemble and corrects simultaneously for
biases and dispersion errors. Also, NGR has been applied many times
successfully for calibrating and combining hydro-meteorological ensemble
forecasts (see for example <xref ref-type="bibr" rid="bib1.bibx24" id="altparen.17"/>).</p>
      <p>The Beta-transformed linear pooling (BLP) approach, which has been developed
recently by <xref ref-type="bibr" rid="bib1.bibx37" id="normal.18"/> and <xref ref-type="bibr" rid="bib1.bibx20" id="normal.19"/> for combining predictive
distributions, will be tested and compared with the NGR and the BMA in this
study. To the author's knowledge the BLP and the associated estimation of
weights, which assign relative importance to the individual predictive
distributions, have not been applied to hydrological forecasts so far.</p>
      <p>Before the combination methods are applied, the errors of the hydrological
model are corrected in order to minimize the difference between the last
available observation and the predictions at the time of initialization of
the forecast. This process of error correction is later on called
post-processing, since it starts after completing the hydrological
simulations and predictions given meteorological observations or forecasts.
Depending on the post-processing method, quantiles or pdfs for future
streamflows will be derived for each single forecast time step. Whereas
quantile regression (QR) methods (<xref ref-type="bibr" rid="bib1.bibx25" id="altparen.20"/>) and modifications of
them will lead to predictions of quantiles, a predictive pdf can be derived
for example by the recently developed waveVARX method (<xref ref-type="bibr" rid="bib1.bibx7" id="altparen.21"/>)
directly. For more details of these post-processing methods, the reader is
referred to <xref ref-type="bibr" rid="bib1.bibx8" id="normal.22"/>, whereas the objective of this paper will be the
analysis of combination methods of forecasts. In the next section the three
combination methods and the applied verification measures will be described.
After the presentation of the data and the results, the outcome of the
comparison will be discussed and summarized in the conclusions.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
      <p>Three different combination methods have been applied to the flood
forecasting system for the Sihl River at station Zurich (Switzerland), where
two meteorological forecasts, the 16-member COSMO-LEPS (<xref ref-type="bibr" rid="bib1.bibx32" id="altparen.23"/>)
and the deterministic C7 system (produced at MeteoSwiss with <inline-formula><mml:math id="M1" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 7 km
resolution) are implemented (a detailed description can be found in
<xref ref-type="bibr" rid="bib1.bibx2" id="altparen.24"/>, <xref ref-type="bibr" rid="bib1.bibx38" id="altparen.25"/>, and <xref ref-type="bibr" rid="bib1.bibx29" id="altparen.26"/>).</p>
      <p>In a first step the hydrological modelling errors of all these forecasts will
be minimized, using a QR method in combination with neural networks (QRNN,
<xref ref-type="bibr" rid="bib1.bibx41 bib1.bibx11" id="altparen.27"/>). This will result in direct estimates of the
inverse cumulative density function (i.e. the quantile function), which in
turn allows the derivation of the predictive uncertainty (see for example
<xref ref-type="bibr" rid="bib1.bibx50" id="altparen.28"/>, <xref ref-type="bibr" rid="bib1.bibx30" id="altparen.29"/>, and <xref ref-type="bibr" rid="bib1.bibx15" id="altparen.30"/>, where the
application of the QR in order to estimate predictive uncertainties (PUs) is
outlined). If the number of estimated quantiles within the domain <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:mo mathvariant="italic">{</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula> is sufficiently large, the resulting distribution could be considered
to be continuous. In this study the number of quantiles is set to nine with
probability levels <inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.75</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.9</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0.99</mml:mn></mml:mrow></mml:math></inline-formula>. In <xref ref-type="bibr" rid="bib1.bibx33" id="text.31"/> the cdf or pdf is constructed by combining step
interpolation of probability densities for specified <inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>-quantiles with
exponential lower and upper tails, which will be called the empirical method
(EMP). Alternatively the pdf could be constructed by monotone re-arranging of
the <inline-formula><mml:math id="M5" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>-quantiles and estimating a log-normal distribution (LN) to these
quantiles for each lead time <inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:math></inline-formula>. The advantage of the quantile
re-arranging and the distribution fitting is 2-fold and efficiently prevents
known problems occurring with QR: firstly it eliminates the problem of
crossing of different quantiles (i.e. the unrealistic but possible outcome of
the non-linear optimization problem yielding lower quantiles for higher
streamflow values – <xref ref-type="bibr" rid="bib1.bibx12" id="altparen.32"/> – e.g. the value of the 0.90
quantile is higher than the value of the 0.95 quantile), and secondly it
permits the extrapolation to extremes not included in the training sample
(<xref ref-type="bibr" rid="bib1.bibx10" id="altparen.33"/>).</p>
      <p>This QRNN method will be applied to each ensemble member of the COSMO-LEPS
forecasts, resulting in 16 forecasts of quantiles, and to the
C7  forecasts. <xref ref-type="bibr" rid="bib1.bibx28" id="normal.34"/> have
examined averaging quantiles of continuous distributions given by multiple
information sources rather than averaging probabilities. Both approaches of
probability and quantile averaging have been applied in this paper for
averaging the post-processed ensemble prediction system (EPS) based
streamflow forecasts in order to get one predictive pdf or quantile forecast.
Before applying the probability averaging approach, a pdf has been
constructed by the LN method, i.e. a log-normal distribution has been fitted
to the re-arranged <inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>-quantiles.</p>
      <p>Thus, in total there are five different forecasts available after
post-processing, two based on the application of the QRNN method for the
COSMO-LEPS with probability averaging (p.aver.) or quantile averaging
(q.aver.), two post-processed C7 forecasts based on QRNN with the EMP and the
LN approach, and one forecast based on the waveVARX method. Additionally the
raw COSMO-LEPS forecast will be included in the following combination
procedures as well (see Fig. <xref ref-type="fig" rid="Ch1.F1"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p>Set of six different forecast models available for combination, five
post-processed plus one raw forecast. For the quantile averaging (M1) and the
probability averaging (M2) method, an example of averaging two ensemble
members is indicated.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f01.png"/>

      </fig>

      <p>Three different methods will be tested for optimally combining these six
forecast models (M1, <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="normal">…</mml:mi></mml:math></inline-formula>, M6), which allow us to assign different
weights to the raw and five post-processed forecasts. For the application of
the first two methods, BMA and NGR, the streamflow values have been
transformed to the normal space by the help of the normal quantile
transformation (<xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx45 bib1.bibx46" id="altparen.35"/>).</p>
<sec id="Ch1.S2.SS1">
  <title>Bayesian model averaging (BMA)</title>
      <p>If the combination is calculated within a Bayesian framework by using weights
corresponding to the posterior model probabilities, it is usually referred to
as BMA and follows from direct application of Bayes' theorem as explained in
e.g. <xref ref-type="bibr" rid="bib1.bibx31" id="normal.36"/> and <xref ref-type="bibr" rid="bib1.bibx36" id="normal.37"/>.</p>
      <p>In <xref ref-type="bibr" rid="bib1.bibx35" id="normal.38"/> the statistical BMA model is extended to dynamical forecast
models, where each forecast and/or ensemble member is represented by a
probabilistic distribution for which a weight is assigned based on the past
performance of each individual forecast. These weights are used to combine
all distributions into one single mixture distribution. Therefore the BMA
predictive model of the quantity of interest <inline-formula><mml:math id="M9" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> is given by
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M10" display="block"><mml:mrow><mml:mi>p</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>|</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi>h</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>g</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>|</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msub><mml:mi>h</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the posterior probability (i.e. weight) of forecast <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the
best forecast derived from its performance in the training period, and the
conditional pdf of <inline-formula><mml:math id="M13" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> on <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>g</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>|</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, given that <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the best
forecast in the ensemble with <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:mi>M</mml:mi></mml:mrow></mml:math></inline-formula> members, or models. The
transformation of the streamflow values to the normal space beforehand allows
the application of the BMA method based on mixtures of univariate normal
distributions. In the work of <xref ref-type="bibr" rid="bib1.bibx49" id="text.39"/> and <xref ref-type="bibr" rid="bib1.bibx39" id="text.40"/> variants
of the BMA method have been applied, which allow the direct usage of the cdfs
for estimating the weighting parameters. However, in this study these BMA
approaches have not been implemented, and the estimated medians (<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>) from the five post-processing methods and from the raw COSMO-LEPS are
taken as input only in order to allow better comparison with the following
NGR approach.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Non-homogeneous Gaussian regression (NGR)</title>
      <p>Another possibility to address underdispersion and forecast bias is the use
of the NGR method, also known as EMOS, and is based on multiple linear
regression for linear variables, such as temperature or streamflows, and
logistic regression for binary variables, such as precipitation occurrence or
freezing. More information about the MOS technique can be found for example
in <xref ref-type="bibr" rid="bib1.bibx18" id="normal.41"/> and <xref ref-type="bibr" rid="bib1.bibx51" id="normal.42"/>. Its extension for ensembles is
explained in <xref ref-type="bibr" rid="bib1.bibx21" id="normal.43"/> and a brief summary of this method is given
hereafter. Let <inline-formula><mml:math id="M19" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> denote again the variable of interest (e.g. streamflow)
and let <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> be the corresponding forecast of the <inline-formula><mml:math id="M21" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>
ensemble members or models. If <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> denotes a
Gaussian density with mean <inline-formula><mml:math id="M23" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> and variance <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, the NGR predictive
distribution is given by

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M25" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>y</mml:mi><mml:mi mathvariant="normal">|</mml:mi><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:msub><mml:mi>k</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtext>where</mml:mtext><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msup><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>M</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msup><mml:mfenced open="(" close=")"><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>M</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi>k</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>Thus the predictive mean is equal to the regression estimates with
coefficients <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and forms a bias-corrected
weighted average of the different forecasts (ensemble members), whereas the
predictive variance depends linearly on the variance of the forecast models
(ensemble members). Although modifications for the NGR exist for non-normal
distributed variates (see for example <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx5" id="altparen.44"/>), the
streamflow values have been transformed to the normal space for comparison
reasons and the medians (<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>) from the five post-processing methods
and from the raw COSMO-LEPS are taken as input as in the BMA method.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Beta-transformed linear pool (BLP)</title>
      <p>In <xref ref-type="bibr" rid="bib1.bibx37" id="normal.45"/> it has been stated that any non-trivially weighted average
of distinct probability forecasts will be uncalibrated and lack sharpness,
even when the individual forecasts have been calibrated. Hence they suggested
a composite of the traditional linear pool with a beta transform. The
aggregation method introduced by <xref ref-type="bibr" rid="bib1.bibx37" id="normal.46"/> and <xref ref-type="bibr" rid="bib1.bibx20" id="normal.47"/>
considers the BLP for a set of predictive cdfs <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math id="M30" display="block"><mml:mrow><mml:mi>F</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>B</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mi>y</mml:mi></mml:mfenced></mml:mfenced></mml:mrow></mml:math></disp-formula>
          for <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>∈</mml:mo><mml:mi>R</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi>B</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> denotes the cdf of the standard
Beta distribution with parameters <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are non-negative weights that sum to 1. The BLP density
forecast for the component densities <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> then is
            <disp-formula id="Ch1.E4" content-type="numbered"><mml:math id="M37" display="block"><mml:mrow><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced open="(" close=")"><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mi>y</mml:mi></mml:mfenced></mml:mfenced><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mi>y</mml:mi></mml:mfenced></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          with parameters <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> of the Beta density function
<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. For <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> the BLP corresponds to the
traditional linear opinion pool.</p>
      <p>Thus <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>B</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> can be interpreted as a parametric calibration
function for combining <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with mixture weights <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi mathvariant="italic">ω</mml:mi><mml:mo>∈</mml:mo><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which assign relative importance to the individual
predictive distributions. The parameters <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and the
weights <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>M</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are estimated with the maximum
likelihood method. The log-likelihood function for the BLP model
(Eq. <xref ref-type="disp-formula" rid="Ch1.E4"/>) is

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M48" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">ℓ</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>M</mml:mi></mml:msub><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>J</mml:mi></mml:munderover><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>J</mml:mi></mml:munderover><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>J</mml:mi></mml:munderover><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mfenced></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>J</mml:mi></mml:munderover><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>J</mml:mi></mml:munderover><mml:mfenced open="(" close=""><mml:mo>(</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced close=")" open="("><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mfenced></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mspace width="1em" linebreak="nobreak"/><mml:mfenced close=")" open="."><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>m</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>M</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">ω</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>F</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:msub><mml:mi>y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mfenced></mml:mfenced></mml:mfenced><mml:mo>+</mml:mo><mml:mi>J</mml:mi><mml:mi>log⁡</mml:mi><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M49" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> is the classical Beta function.</p>
      <p>This BLP approach has been applied now to combine the different forecast
systems. The quantiles resulting from the QRNN method (models M1, M4, and M5)
forecasts have been converted to pdfs by applying the LN method (by fitting a
log-normal distribution to the re-arranged <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> quantiles).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Verification</title>
      <p>Although probability and quantile forecasts are both probabilistic products,
the former is expressed in terms of a probability (e.g. that a certain
threshold will be exceeded) and the latter is given by a quantile for a
particular probability level of interest (<xref ref-type="bibr" rid="bib1.bibx9" id="altparen.48"/>). Since the
outputs of the QRNN model are quantiles, it is reasonable to evaluate the
performance with a skill score which has been developed for predictive
quantiles (<xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx17" id="altparen.49"/>), known as the quantile score (QS). It
is based on an asymmetric piecewise linear function, the so-called check
function, <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mfenced></mml:mrow></mml:math></inline-formula>, which is a function of the
probability level <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the error between the observation
<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the quantile forecast <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:mi>N</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M56" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>
is the sample size. The check function is defined as
            <disp-formula id="Ch1.E6" content-type="numbered"><mml:math id="M57" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mfenced><mml:mo>=</mml:mo><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mfenced close=")" open="("><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∀</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mfenced close=")" open="("><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mfenced><mml:mfenced close=")" open="("><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>∀</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>
          and the QS results as the mean of the check function with penalties <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M59" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> for under- and over-forecasting (see <xref ref-type="bibr" rid="bib1.bibx9" id="altparen.50"/>):
            <disp-formula id="Ch1.E7" content-type="numbered"><mml:math id="M60" display="block"><mml:mrow><mml:mi mathvariant="normal">QS</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>:</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>&lt;</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:munder><mml:mo>(</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>:</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:munder><mml:mo>(</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>q</mml:mi><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>The CRPS compares the forecast probability distribution with the observation
and both are represented as cdfs. If <inline-formula><mml:math id="M61" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> is the predictive cdf and <inline-formula><mml:math id="M62" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> is the
verifying observation, <xref ref-type="bibr" rid="bib1.bibx19" id="normal.51"/> showed that the CRPS can be defined
equivalently as a standard form,

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M63" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E8"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">CRPS</mml:mi><mml:mo>(</mml:mo><mml:mi>F</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">∞</mml:mi></mml:mrow><mml:mi mathvariant="normal">∞</mml:mi></mml:munderover><mml:msup><mml:mfenced open="(" close=")"><mml:mi>F</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>I</mml:mi><mml:mo mathvariant="italic">{</mml:mo><mml:mi>y</mml:mi><mml:mo>≤</mml:mo><mml:mi>t</mml:mi><mml:mo mathvariant="italic">}</mml:mo></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mtext>and as</mml:mtext></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E9"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mn mathvariant="normal">1</mml:mn></mml:munderover><mml:mfenced open="(" close=")"><mml:mi>I</mml:mi><mml:mfenced open="{" close="}"><mml:mi>y</mml:mi><mml:mo>&lt;</mml:mo><mml:msup><mml:mi>F</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo></mml:mfenced><mml:mo>-</mml:mo><mml:mi mathvariant="italic">τ</mml:mi></mml:mfenced><mml:mfenced close=")" open="("><mml:msup><mml:mi>F</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>Thus, in the standard form (Eq. <xref ref-type="disp-formula" rid="Ch1.E8"/>) an ensemble of predictions can
be converted into a piecewise constant cdf with jumps at the different models
(ensemble members), and <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi>I</mml:mi><mml:mo mathvariant="italic">{</mml:mo><mml:mo>.</mml:mo><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula> is a Heaviside step function, with a single
step from 0 to 1 at the observed value of the variable. The equivalence of
Eqs. (<xref ref-type="disp-formula" rid="Ch1.E8"/>)–(<xref ref-type="disp-formula" rid="Ch1.E9"/>) was noted by <xref ref-type="bibr" rid="bib1.bibx27" id="normal.52"/>. For the
quantile forecast <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>q</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mi>F</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the integrand in
Eq. (<xref ref-type="disp-formula" rid="Ch1.E9"/>) equals the quantile score, i.e. the mean of the check
function (Eq. <xref ref-type="disp-formula" rid="Ch1.E6"/>). That means the CRPS corresponds to the integral of
the QS over all thresholds, or likewise the integral of the QS over all
probability levels (<xref ref-type="bibr" rid="bib1.bibx27" id="altparen.53"/> and <xref ref-type="bibr" rid="bib1.bibx19" id="altparen.54"/>). Hence, the CRPS
averages over the complete range of forecast thresholds and probability
levels, whereas the QS looks at specific <inline-formula><mml:math id="M66" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>-quantiles; thus, it is more
efficient in revealing deficiencies in different parts of the distributions,
especially with respect to the tails of the distribution. Both verification
measures are negatively oriented, meaning the smaller the better.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
      <p>COSMO-LEPS and C7 forecasts are available from 24 February 2010 to
27 April 2016 once a day with hourly time resolution, which have been
post-processed in order to derive predictive distributions and quantile
forecasts. To calibrate and validate the post-processing parameters (QRNN and
waveVARX), the data sets of available hourly observations and corresponding
simulations have been split into two halves (calibration period: 2010–2012;
validation period: 2013–2016). The results of the validation, which are not
shown due to lack of space, highlight the improvements of the QRNN method
(similar to the results shown in <xref ref-type="bibr" rid="bib1.bibx8" id="altparen.55"/>).</p>
      <p>The weighting parameters of the combination methods are estimated by applying
a moving window with a size of 7 days (168 h) for optimization. Different
window sizes have been tested as well, but 7 days was chosen finally as a
trade-off between computing time and efficiency. In Fig. <xref ref-type="fig" rid="Ch1.F2"/> an
example of the temporal evolution of the hourly weights for a lead time of
48 h for the three combination methods is shown.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Hourly weights of the BMA <bold>(a)</bold>, NGR <bold>(b)</bold>, and
BLP <bold>(c)</bold> methods estimated for a lead time of 48 h. The six
forecasts are the QRNN method for the COSMO-LEPS with quantile averaging
(QRNN-CL-q.) – M1, probability averaging (QRNN-CL-p.) – M2, the
waveVARX(-CL) method – M3, the raw COSMO-LEPS (CL) forecast – M4, the
two post-processed C7 forecasts based on QRNN with the EMP – M5, and the
LN approach – M6.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f02.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Probability integral transform (PIT) of the raw and three combined
forecasts at a lead time of 48 h.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f03.pdf"/>

      </fig>

      <p>Before the forecast skill of the three combination methods are compared, the
statistical consistency between the predictive cdf and the observations are
analysed with the help of the probability integral transform (PIT) as
proposed by <xref ref-type="bibr" rid="bib1.bibx13" id="text.56"/> (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). In the case of
well-calibrated forecasts, the sequence of PIT values will follow a uniform
distribution <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi>U</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. U-shaped PIT histograms indicate underdispersed
forecasts with too little spread on average, and inverse U-shaped histograms
correspond to overdispersed forecasts (see for example
<xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx27" id="altparen.57"/>).</p>
      <p>The question now is whether there are significant differences between the
three combination methods. Therefore the QS has been applied at first to
highlight possible differences between the combination methods in more
detail.</p>
      <p>In Fig. <xref ref-type="fig" rid="Ch1.F4"/> the results of the QS at four lead times for the raw
COSMO-LEPS (C-L, black line) and for the three combination methods BLP (red
line), NGR (green line), and BMA (blue line) are shown and compared to the QS
results of the raw C-L (black circles). Additionally, a simple quantile
mapping (QM) is applied (cyan diamonds) to the raw C-L forecasts in order to
evaluate the positive effect of using more complex methods. Thereby the cdf
of the raw forecast is matched to the cdf of the observations. As mentioned
in <xref ref-type="bibr" rid="bib1.bibx53" id="normal.58"/>, QM is highly effective for bias correction, but ensemble
spread reliability problems cannot be solved properly.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Quantile score (QS) for various lead times and the three combination
methods in comparison to the raw COMSO-LEPS and a simple quantile mapping
(QM) approach.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f04.pdf"/>

      </fig>

      <p>In Fig. <xref ref-type="fig" rid="Ch1.F5"/> the CRPS results of the six forecast models are shown in
comparison to the BLP in order to demonstrate the motivation of aggregating
these systems. As can be seen clearly, the combined forecast outperforms each
of the individual forecasts in view of the CRPS.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5"><caption><p>CRPS of the six forecast models: COSMO-LEPS with quantile averaging
(QRNN-CL-q.) – M1, probability averaging (QRNN-CL-p.) – M2, the
waveVARX(-CL) method – M3, the raw COSMO-LEPS (CL) forecast – M4, the
two post-processed C7 forecasts based on QRNN with the EMP – M5, and the
LN approach – M6. Additionally, the CRPS of the BLP combined forecast is
shown.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f05.pdf"/>

      </fig>

      <p>The CRPS for the raw C-L, the QM approach and the three combination methods
is shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>CRPS of the raw and combined forecasts.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://hess.copernicus.org/articles/21/5493/2017/hess-21-5493-2017-f06.pdf"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
      <p>So far most of the studies comparing the results of the BMA and the NGR
approach have not found any preference (see for example <xref ref-type="bibr" rid="bib1.bibx52" id="altparen.59"/>). In
this paper these two methods are checked against the BLP, which has not been
used for hydrological purposes until now. In a first step the weights derived
for each individual, raw and post-processed, forecast system are compared.
The pattern of these optimized weights in Fig. <xref ref-type="fig" rid="Ch1.F2"/> shows rather
vague similarities between the three combination methods. The BLP and the NGR
are in general more spiky, with rapid changes between consecutive hours. This
could result from problems in convergence from the optimization algorithm
applied for estimating the parameters (“constrOptim” in R <xref ref-type="bibr" rid="bib1.bibx34" id="altparen.60"/>).</p>
      <p>In general the weights show some periodicity, which indicates that some
models are more appropriate to be used in certain seasons and for certain
flow conditions during a year. However, the limited amount of data does not
allow us to draw clear conclusions.</p>
      <p>The results of the PIT clearly indicate that all three combinations result in
well-calibrated forecasts with close to uniform histograms. In Fig. <xref ref-type="fig" rid="Ch1.F3"/>
the examples for the 48 h forecast are given, highlighting the heavy
underdispersiveness of the raw forecasts. The same behaviour is visible for
almost all lead times; however, the raw COSMO-LEPS forecasts get less
underdispersed with increasing lead time, since the spread and the
uncertainty in the ensemble increase.</p>
      <p>The analysis of the QS (Fig. <xref ref-type="fig" rid="Ch1.F4"/>) shows slightly better results for
the BLP, followed by the NGR and BMA. The raw COSMO-LEPS (C-L) and the QM are
much worse, especially for smaller lead times. It is interesting to see that
the QS of the raw C-L follows a straight line for smaller lead times (6 and
12 h) in the same manner as one would expect from deterministic forecasts,
because of the underdispersiveness of the C-L at the beginning of the
forecast horizon. The slope of this line is an indicator of the size of the
(positive) bias. The QM at a lead time of 6 h is also a straight line,
however, with an opposite but much smaller and negative slope (bias) in
comparison to the raw C-L. With increasing lead times the QS of the raw C-L
and the QM forecasts come closer to the combined forecasts for probability
levels between 0.1 and 0.5. This is most probably caused by the increased
spread of the ensemble. However, for a lead time of 24 and 48 h, the raw C-L
forecasts still show the worst behaviour at higher flows, whereas the QM
method performs at a lead time of 48 h almost as well as the combination
methods, apart from the forecasts around the median.</p>
      <p>As already stated previously, the comparison of the CRPS of the different
post-processed methods and the aggregated ones (e.g. BLP) clearly identifies
the advantage of combination (Fig. <xref ref-type="fig" rid="Ch1.F5"/>). The CRPS, i.e. the integral
of the QS, for the different combination methods (Fig. <xref ref-type="fig" rid="Ch1.F6"/>) confirms
the results of the QS. In general the results of the BLP are slightly better
than the NGR and BMA results. It seems that for those periods of lead times,
where the BLP is not superior (e.g. around 20 h), the optimization routines
had problems on convergence. However, further analysis will be necessary. The
comparison with the QM approach confirmed the results of <xref ref-type="bibr" rid="bib1.bibx53" id="normal.61"/>, since
the forecast quality did not show any improvements at the first lead times
because of the underdispersiveness of the raw C-L. Thus, the more complex
combination by far outperforms the QM method.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Combination is an essential tool for improving the forecast quality. The
different methods are all more or less equally suited. Although the BLP
showed slightly better results, the straightforward application and the low
computational costs of the NGR make this method an equally good alternative,
at least for this case study. The parameter estimation of the BMA and the BLP
could get quite time-consuming and sometimes results in suboptimal solutions,
which could degrade the gain of applying combination methods.</p><?xmltex \hack{\newpage}?>
</sec>

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

      <p>The COSMO-LEPS and C7 raw meteorological forecasts are
properties of MeteoSwiss and have been made available under license agreement
between WSL and MeteoSwiss. The processed streamflow simulations and
forecasts as well as the measured discharge data can be made available upon
request. All calculations of the post-processing and the combination methods
have been implemented in the R statistical software (R Core Team, 2016) using
various packages like QRNN (<xref ref-type="bibr" rid="bib1.bibx11" id="altparen.62"/>) and ensembleBMA
(<xref ref-type="bibr" rid="bib1.bibx35" id="altparen.63"/>).</p>
  </notes><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p>The real-time operational system for the Sihl basin is financed by the Office
of Waste, Water, Energy and Air of the Canton of Zurich. This study was
conducted in the framework of the Swiss Competence Center for Energy Research
– Supply of Electricity (SCCER-SoE) with funding from the Commission for
Technology and Innovation – CTI (grant 2013.0288). MeteoSwiss is greatly
acknowledged for providing all used meteorological data. The Swiss Federal
Office for Environment (FOEN) provided the observed discharge data. The
authors would like to thank especially Vanessa Round for proofreading.
<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Florian
Pappenberger<?xmltex \hack{\newline}?> Reviewed by: two anonymous referees</p></ack><ref-list>
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<abstract-html><p class="p">The enhanced availability of many different hydro-meteorological modelling
and forecasting systems raises the issue of how to optimally combine this
great deal of information. Especially the usage of deterministic and
probabilistic forecasts with sometimes widely divergent predicted future
streamflow values makes it even more complicated for decision makers to sift
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information will be aggregated based on several different predictive
distributions, and quantile forecasts. For this combination the Bayesian
model averaging (BMA) approach, the non-homogeneous Gaussian
regression (NGR), also known as the ensemble model output statistic (EMOS)
techniques, and a novel method called Beta-transformed linear
pooling (BLP) will be applied. By the help of the quantile score (QS) and the
continuous ranked probability score (CRPS), the combination results for the
Sihl River in Switzerland with about 5 years of forecast data will be
compared and the differences between the raw and optimally combined forecasts
will be highlighted. The results demonstrate the importance of applying
proper forecast combination methods for decision makers in the field of flood
and water resource management.</p></abstract-html>
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