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  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</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/gmd-13-1267-2020</article-id><title-group><article-title>Data assimilation of in situ and satellite remote sensing data to 3D
hydrodynamic lake models: a case study using Delft3D-FLOW v4.03 and OpenDA
v2.4</article-title><alt-title>Data assimilation of hydrodynamic  models</alt-title>
      </title-group><?xmltex \runningtitle{Data assimilation of hydrodynamic  models}?><?xmltex \runningauthor{T.~Baracchini et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Baracchini</surname><given-names>Theo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Chu</surname><given-names>Philip Y.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Šukys</surname><given-names>Jonas</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Lieberherr</surname><given-names>Gian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2066-6868</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Wunderle</surname><given-names>Stefan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff5">
          <name><surname>Wüest</surname><given-names>Alfred</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff5">
          <name><surname>Bouffard</surname><given-names>Damien</given-names></name>
          <email>damien.bouffard@eawag.ch</email>
        <ext-link>https://orcid.org/0000-0002-2005-9718</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Physics of Aquatic Systems Laboratory (APHYS) – Margaretha Kamprad
Chair, ENAC, EPFL, Lausanne, 1015, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Great Lakes Environmental Research Laboratory, NOAA, Ann Arbor, MI
48108, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Eawag, Swiss Federal Institute of Aquatic Science and Technology,
Systems Analysis, <?xmltex \hack{\break}?> Integrated Assessment and Modelling, Dübendorf, 8600,
Switzerland</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Oeschger Centre for Climate Change Research, Institute of Geography,
University of Bern, Bern, 3012, Switzerland</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Eawag, Swiss Federal Institute of Aquatic Science and Technology,
Surface Waters – Research and Management, Kastanienbaum, 6047, Switzerland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Damien Bouffard (damien.bouffard@eawag.ch)</corresp></author-notes><pub-date><day>17</day><month>March</month><year>2020</year></pub-date>
      
      <volume>13</volume>
      <issue>3</issue>
      <fpage>1267</fpage><lpage>1284</lpage>
      <history>
        <date date-type="received"><day>15</day><month>February</month><year>2019</year></date>
           <date date-type="rev-request"><day>21</day><month>March</month><year>2019</year></date>
           <date date-type="rev-recd"><day>10</day><month>December</month><year>2019</year></date>
           <date date-type="accepted"><day>10</day><month>February</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 Theo Baracchini et al.</copyright-statement>
        <copyright-year>2020</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://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020.html">This article is available from https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e164">The understanding of physical dynamics is crucial to
provide scientifically credible information on lake ecosystem management.
We show how the combination of in situ observations, remote sensing data, and
three-dimensional hydrodynamic (3D) numerical simulations is capable of
resolving various spatiotemporal scales involved in lake dynamics. This
combination is achieved through data assimilation (DA) and uncertainty
quantification. In this study, we develop a flexible framework by
incorporating DA into 3D hydrodynamic lake models. Using an ensemble Kalman
filter, our approach accounts for model and observational uncertainties. We
demonstrate the framework by assimilating in situ and satellite remote
sensing temperature data into a 3D hydrodynamic model of Lake Geneva.
Results show that DA effectively improves model performance over a broad
range of spatiotemporal scales and physical processes. Overall, temperature
errors have been reduced by 54 %. With a localization scheme, an ensemble
size of 20 members is found to be sufficient to derive covariance matrices
leading to satisfactory results. The entire framework has been developed
with the goal of near-real-time operational systems (e.g., integration into
meteolakes.ch).</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e176">The management of aquatic systems is a complex challenge including many
stakeholders pursuing sometimes contradictory objectives. This becomes even
more complicated in view of climate change, affecting both watershed
hydrology and lakes physics. There is thereby an urgent need to provide
accurate information on lake hydrodynamics.</p>
      <p id="d1e179">Traditionally, perhaps due to the misleading definition of lakes as lentic
systems, hydrodynamic studies have focused on the one-dimensional vertical
structure of lakes using in situ measurements with limited spatial and
temporal coverage    (Kiefer et al., 2015). Yet, the lentic
definition of lakes is misleading at a short timescale. Dynamical processes
such as wind-induced upwellings, rivers discharges, and gyres strongly
disrupt the spatial homogeneity of the systems and ultimately affect lake
biogeochemistry    (MacIntyre and Melack, 1995). Remote sensing
observations, as well as one- and three-dimensional hydrodynamic models,
have addressed some of the spatial and temporal coverage limitations.</p>
      <p id="d1e182">While three-dimensional (3D) hydrodynamic models are important tools capable
of simulating multi-scale temporal and spatial 3D lake dynamics,
measurements remain essential to properly calibrate and validate models to
improve their<?pagebreak page1268?> accuracy. Indeed, model deviations are unavoidable due to
uncertainties in processes, forcing, and observations (Lahoz et
al., 2010), which have to be taken into account. Remotely sensed
observations provide another essential source of information, with improved
spatial and temporal resolution. However, this information remains
fundamentally 2D. Ultimately, the combination of remote sensing, numerical
simulations, and in situ measurements can overcome the large variations of
spatiotemporal scales involved in lake dynamics and hence provide an
adequate understanding of the system. This combination is achieved by data
assimilation (DA).</p>
      <p id="d1e185">DA is an effective approach to blend observational data into model
simulations (Bannister, 2017; Li et al., 2008). Defined
as the process by which the model of an evolving system is corrected by
incorporating observations of the real system, DA improves both short-term
forecasts and past model reanalysis     (Hawley et al.,
2006). A fundamental property of DA is to take observation (e.g., instrument
accuracy, representativeness) and model (e.g., in processes, forcing, initial
conditions) errors into account (Lahoz et al., 2010) and to
provide the analysis with corrected errors    (Kourzeneva, 2014).
Those are crucial elements for parameter inference, monitoring, and forecast
reliability.</p>
      <p id="d1e189">Multiple methods have been developed for DA, among those the ensemble
Kalman filter (EnKF;    Evensen, 2003). The EnKF has been successfully
applied to numerous applications in oceanography and atmospheric sciences
(Eknes and Evensen, 2002;
Evensen, 1994; Mao et al., 2009; Natvik and Evensen, 2003). It was found to
be an efficient tool for nonlinear problems with high dimensionality
(Crow, 2003; Reichle
et al., 2002a, b) by computing system error statistics based on system
dynamics. But those methods have rarely been applied to lakes, and DA for
inland waters is still in its infancy. The different scales involved, and
considering the sparse observations in combination with the large
heterogeneity found in lake dynamics, limited the direct application of
experiments designed for oceans. For instance,    Zhang et al. (2007) assimilated current measurements into a two-dimensional circulation
model of Lake Michigan, whereby current updates are calculated by kriging
interpolation.    Yeates et al. (2008) used a pycnocline filter
that assimilated thermistor data into a 3D model of a stratified lake to
negate numerical diffusion driving model predictions off course.
Stroud et al. (2009) assimilated satellite images into a
two-dimensional sediment transport model of Lake Michigan using direct
insertion and a kriging-based approach, effectively reducing model forecast
errors. Later on they used an EnKF and smoother (Stroud et
al., 2010) with a similar model and data when a large sediment plume was
observed after a major storm event. The results obtained were better relative to
standard approaches (a static model and a reduced-rank square root Kalman
filter). Finally,    Kourzeneva (2014) used an extended Kalman filter
(EKF) to assimilate lake surface water temperature into a one-dimensional
two-layer freshwater lake model, leading to significant improvements over
the free model run. Overall, to our knowledge, this is the first DA
experiment that blends both in situ observations and remote sensing data
into a three-dimensional hydrodynamic model with high dimensionality.</p>
      <p id="d1e192">The aim of this study is to develop a flexible framework, in a Bayesian
inference setting, capable of updating and improving model states while
taking into account the uncertainty of both the modeled system and
observational data. Here, we present a novel DA experiment with an EnKF
tailored to lakes and observations using an open-source hydrodynamic model
and assimilation platform. This approach uses a new file-based coupling
recently developed for OpenDA and Delft3D-FLOW with <inline-formula><mml:math id="M1" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>-layer support
(Baracchini et al., 2019a). Delft3D-FLOW is an open-source
three-dimensional hydrodynamic simulation software with numerous successful
applications in coastal, river, estuarine, and lake domains. OpenDA is an
open-source generic DA environment (El Serafy et al., 2007)
used in various calibration and DA experiments (El Serafy et
al., 2007;    Weerts et al., 2010;    Kurniawan et
al., 2011), but it has not yet been applied to 3D lake hydrodynamic modeling with DA. Our
methodology is tested on the large French–Swiss Lake Geneva with in situ
temperature measurements and lake surface water temperature (LSWT) retrieved
from satellite data (AVHRR). The choice of testing a first DA of surface
temperature on Lake Geneva was motivated by recent studies concluding that
data from spaceborne medium-resolution radiometers specifically tailored to
Lake Geneva     (Oesch et al., 2005) could potentially be
assimilated to numerical models (Oesch et al., 2008).
Furthermore, Baracchini et al. (2019a) proposed a calibrated model
and framework for Lake Geneva, this first step being an absolute requirement
for DA. Here, LSWT and in situ data are blended into such a model to expand
its monitoring capabilities of physical phenomena. The latter is achieved by
considering the stochasticity of the system and an EnKF algorithm to update
model results. Environmental research and operational monitoring and
forecasting of midsize to large lakes will benefit from this procedure,
with noticeable impacts on a broad diversity of societally important issues.</p>
      <p id="d1e202">The study is organized as follows: Sect. 2, “Data and methods”, describes the
study site, model, tools, and data used. This includes measurement retrieval
and the processing chain as well as the quantification of their uncertainty.
Although part of the methods, the data assimilation algorithm and its
configuration are provided in a different section (Sect. 3) due to their
central role in the study. Noise generation, the number of ensembles, and
the localization scheme are discussed in this section. Sections 4 and 5 consist
of the presentation and discussion of results, respectively. Finally,
perspectives and conclusion are given in the final section.</p>
</sec>
<?pagebreak page1269?><sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
      <p id="d1e213">Here we describe the various components used in the DA experiment, the
challenges associated with high-frequency and high-resolution measurements,
modeling datasets, and their error definitions, which previously hampered
the application of such systems.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Study site</title>
      <p id="d1e223">Lake Geneva (locally known as Le Léman) is a perialpine lake located
between Switzerland and France (46.458<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 6.528<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)
at an altitude of 372 m (Fig. 1). It is the largest freshwater lake in
western Europe (surface area and volume of 580 and 89 km<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>,
respectively), with a retention time of 11.4 years. Due to relatively mild
winter temperatures and its large depth of 309 m, complete deep convective
mixing occurs only every 5 to 10 winters   (Schwefel et al.,
2016). The lake is composed of two parts: the large eastern basin (Grand
Lac), with a maximum depth of 309 m, mean depth of 160 m, and mean width of 10 km
in which gyres are frequently observed, and the Petit Lac, the narrow and
shallow western basin (maximum depth of 70 m, mean width of 4.5 km). The
centers of the two basins are some 30 km apart, which defines the cutoff
distance of the EnKF (more details in Sect. 3). The surrounding topography
is mountainous, mainly in the southeast, hence affecting the wind
circulation above the basin. Lake Geneva is mesotrophic, with strong
variation in turbidity and light penetration depth over the year (ranging
from 3.6 to 14 m).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e255">Lake Geneva locations, computational grid, and bathymetry. Circles
are in situ measurement sites. The triangle indicates the AVHRR validation
station. Squares are selected sampling locations used to generate the wind
fields of the COSMO-E products. Basemap source: Federal Office of Topography
© Swisstopo.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f01.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Model setup</title>
      <p id="d1e274">The primary purpose of a 3D hydrodynamic model is to solve the
time-dependent, nonlinear differential equations of the hydrostatic
free-surface flows in a computational grid. Various modeling suites have
been developed to solve those equations accounting for momentum
(Reynolds-averaged Navier–Stokes – RANS) and fluid mass (continuity), as
well as heat and mass transfer. The open-source Delft3D-FLOW software is
used in this study.</p>
<sec id="Ch1.S2.SS2.SSSx1" specific-use="unnumbered">
  <title>Delft3D-FLOW numerical model</title>
      <p id="d1e282">Delft3D-FLOW is an
open-source hydrodynamic modeling suite developed by Deltares, Netherlands.
Initially designed for coastal regions and estuaries, it has been expanded
to rivers and lakes. A detailed model description of the equations and
numerical schemes (conjugate gradient solver) can be found in the manual
(Deltares, 2015).
We stress again that a fundamental prerequisite for any DA experiment is a
well-calibrated model. Improper physical parameters could lead to strong
discontinuities followed by waves (assimilation shocks), leading to spurious
behaviors    (Anderson et al., 2000). Assimilated variables could
then, for example, go back to their pre-assimilated value. Lake Geneva's
model has been extensively studied and calibrated (explicit optimization
method by residual minimization) in a previous study (Baracchini
et al., 2019a). This model consists of 100 unevenly distributed vertical
layers, with thinner layers at the top (from 20 cm at the surface to several
meters in the hypolimnion). Due to the steep bathymetry of Lake Geneva, we
use the <inline-formula><mml:math id="M5" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>-coordinate system (layers are horizontal) to avoid strong
numerical diffusion and excessive artificial mixing. A computational
time step of 2 min is specified for the 450 m horizontal grid size to
maintain model stability with the <inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="italic">κ</mml:mi></mml:math></inline-formula>-<inline-formula><mml:math id="M7" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> turbulence closure
model. This turbulence closure model accounts for unresolved mixing at
sub-grid scales. As initial conditions, the model is initialized (uniformly
horizontally) from an in situ temperature profile taken at the deepest
location of the lake in January, when the lake is partially mixed. We
consider a simulation period of 1 year, thereby covering the entire range
of seasonal stratification dynamics.</p>
      <p id="d1e306">The dynamics of a lake are mainly driven by interactions with the atmosphere
and dissipation at the bed. As boundary forcing, we use MeteoSwiss COSMO-1
reanalysis products from their atmospheric model tailored to the Alpine
region. They consist of various meteorological variables on a regular 1.1 km
grid with hourly resolution. Seven of those variables are used in this
study: solar radiation, wind direction and velocity, relative humidity,
cloud cover, pressure, and air temperature.</p>
      <p id="d1e309">Lake Geneva is subject to strong variations in turbidity, which affect the
stratification mainly in early summer. Monthly time series of Secchi depth
observations have therefore been used in the forcing.</p>
      <?pagebreak page1270?><p id="d1e312">Finally, a single deterministic 1-year model run for Lake Geneva without
DA requires 3 d of wall-clock computing time on a single Intel Xeon
Broadwell core processor.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Assimilation platform</title>
      <p id="d1e324">OpenDA is an open interface standard. It provides access to a set of
open-source tools, allowing for the integration of arbitrary numerical models and
observations through calibration and data assimilation algorithms. Its goal
is to minimize algorithmic development by promoting the exchange of software
solutions among researchers and users (Deltares, 2019; <uri>http://www.openda.org</uri>, last access: 9 March 2020).</p>
      <p id="d1e330">An OpenDA interface has recently been developed for the <inline-formula><mml:math id="M8" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>-layer Delft3D-FLOW
using the black-box wrapper (file-based) approach (Baracchini et
al., 2019a). This interface has been further expanded for DA in this study.
Additions include extended modifications of the Delft3D-FLOW
model definition file, model forcing files (on an equidistant grid only) for
OpenDA's noise models, and support for localization, which allows users to limit
the area of influence of an observation. The entire source code is available
on GitHub (<uri>https://github.com/OpenDA-Association/OpenDA</uri>, last access: 9 March 2020).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Monitoring data</title>
<sec id="Ch1.S2.SS4.SSS1">
  <label>2.4.1</label><title>Role of data accuracy </title>
      <p id="d1e359">Key in any DA problem is the
observational data and their quality (Madsen, 2003). 3D models require
an especially large amount of data to validate their variability. Remote
sensing observations are therefore considered together with vertical in situ
profiles to constrain the system over the surface and depth. Errors are
present in the system through its initial conditions, physical processes,
approximations, and forcings    (Bárdossy and Singh, 2008).
Observations of the true system also require quantifying their
uncertainties, as measurements are always an imperfect and incomplete
representation  (Bertino et al., 2007). This is
particularly important as it defines how reliable an observation is and
therefore how the model states are corrected. Injecting data with incorrect
measurement error distributions into a good model could depreciate its
relevance to the point at which assimilation estimates are worse than the
non-assimilative solution or the observations. The opposite holds true, and
model forecast would still be unreliable.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <label>2.4.2</label><title>Lake in situ data</title>
      <p id="d1e370">The dataset consists of 31
temperature profiles over the water column at two locations of Lake Geneva
(GE3 and SHL2; Fig. 1) sampled during the year 2017. Profiles are collected on a
monthly (GE3) to bimonthly (SHL2) basis. Uncertainty of in situ
temperature profiles is defined as the maximum value of the instrument
precision (0.1 <inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) and temporal variability at the measurement
location. The reasons for the latter are twofold: first, some in situ profiles
did not have their exact collection time recorded; second, this study does
not focus on reproducing short-term dynamics such as basin-scale internal
waves and thermocline oscillations. The standard deviation of preliminary
modeling results is computed over a time window to account for this
variability. The temporal variability window is defined by the period of
basin-scale internal oscillations (48 h). This procedure allows for the limiting
of physical discontinuities created by the EnKF updates from specific physical
processes (i.e., internal waves), which are not the focus of this study.</p>
      <p id="d1e382">The Buchillon station (Fig. 1), consisting of a mast measuring various
atmospheric and hydrodynamic properties in real time, has been used for the
validation of AVHRR data as detailed below. Of relevance for this study is a
thermistor located at 1 m of water depth, representing the bulk temperature.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS3">
  <label>2.4.3</label><title>AVHRR LSWT</title>
      <p id="d1e393">The spaceborne Advanced Very High
Resolution Radiometer (AVHRR) sensor has been selected for its high temporal
(up to 10 overpasses per day) and moderate spatial (1.1 km in nadir)
resolution. We consider it to be the right trade-off for lakes: between the
high spatial but low temporal resolution of Landsat 8 (100 m every 2 weeks)
and the low spatial but high temporal one of SEVIRI (3 km at the Equator; every
15 min). The access to the AVHRR data was facilitated by a direct downlink
and processing chain from the University of Bern. We describe below, and in
the Appendix, how AVHRR can be used for DA in lakes.</p>
      <p id="d1e396">The AVHRR LSWT retrieval process, with locally adapted split-window
coefficients for Lake Geneva, is described in
Lieberherr and Wunderle (2018) and
Lieberherr et al. (2017). Only pixels with quality levels higher
than 3 (Lieberherr and Wunderle, 2018)
are considered for the next sections.</p>
      <p id="d1e399">An extensive description of the filtering of the data is available in
Appendix A. Overall, out of the 3372 AVHRR images of Lake Geneva available
for 2017, 124 satisfy the selection criteria (see Appendix A). These data are
relatively evenly spread from February to October, with a maximum frequency
of one image per 24 h. Very few images are available in January,
November, and December due to bad weather conditions or cloud cover. The
average lake coverage of those images is about 51 %.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Data assimilation</title>
      <p id="d1e412">The multiple methods proposed for DA mainly fall into two categories: (i) variational (e.g., 3D-VAR, 4D-VAR) and (ii) sequential methods (e.g., Kalman
filtering, particle filtering). For variational methods, the optimization of
the model states (or parameters) is based on the minimization of a<?pagebreak page1271?> cost
function. Carrassi et al. (2018) have proposed an extensive review of DA
assimilation methods and uses in geophysical sciences. Variational methods
are popular in meteorological forecasting     (Rawlins
et al., 2007). However, the computational burden associated with the
collection and storage of data can be significant. Moreover, the batch
processing of data reduces flexibility and complicates the consideration of
time-varying model parameters.</p>
      <p id="d1e415">Sequential methods are robust techniques for DA in a broad range of
applications. For linear dynamics and measurement processes with Gaussian
error statistics, the Kalman filter (Kalman, 1960) is an optimal
sequential DA algorithm. However, most processes observed in nature, such as
hydrodynamics, are nonlinear. The analytical solution provided by the
Kalman filter therefore cannot be derived in order to compute the posterior
distribution of simulated variables. To overcome this limitation, variants
exist, such as the EKF, which consists of a linearization of the model in
the neighborhood of the current estimate of the state vector. This
linearization can lead to complicated calculations for systems with high
dimensionality, as the integration and propagation of the error covariance
result in a significant computational demand (Gillijns et
al., 2006). Linearization is done using first-order Taylor expansion, which
implies a closure at the second-order moments. For highly nonlinear systems
this can result in an improper estimation of the state vector or covariance
matrices and can therefore lead to quick divergence and instability
(Moradkhani et al., 2005; Nakamura et al., 2006).</p>
      <p id="d1e418">In order to cope with nonlinearities and obtain a full representation of
the posterior distribution, other statistical methods, such as particle
filters, have been developed (Carpenter et al., 1999). The
particle filter is a solution following a Darwinian-like process of survival
of the fittest. It shares properties with an EnKF in the sense that the
particles are the ensemble members. Particle filters do not need any
assumption for the state variable distribution (e.g., Gaussian) and can deal
with nonlinear observation models as well. The updates are applied on
particle weights rather than the state variable, which results in fewer
numerical instabilities for process-based models
(van Leeuwen, 2009; Liu et
al., 2012; Moradkhani et al., 2005). A major drawback is the particle
depletion, which requires complex resampling algorithms. Moreover, it is
less computationally efficient than the EnKF due to the need for a high
number of particles (more particles than EnKF ensembles are often needed, of
the order of tens of thousands). Despite its advantages, the use of the
particle filter as an assimilation method in oceanography and limnology is
limited due to its high computational cost. To address such issues, solutions
are undergoing development   (Šukys and
Kattwinkel, 2018). For its flexibility and affordable computational cost, we
further focus on the EnKF.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Ensemble Kalman filter (EnKF)</title>
      <p id="d1e428">The EnKF is an attractive alternative for nonlinear dynamics and systems
with high dimensionality.         Reichle et
al. (2002a) found that the EnKF is more robust than the EKF while being more
flexible to obtain system covariances, a core element of the DA problem
(Bertino et al., 2007). Indeed, whereas the careful
estimation of covariances often required a lot of effort
(De Lannoy et al., 2007b), in the EnKF they are derived
dynamically from a small ensemble of model trajectories (and therefore take
into account the physics of the model), which grasps   the   essential parts of the
error structure   (Reichle et al., 2002b). The EnKF only
considers a sample of the state variable to represent the processes
modeled. The covariance matrix becomes a sampled covariance matrix, and
predictive probability density functions of the state vectors are
approximated by Monte Carlo simulations    (Nakamura et al., 2006).
It nonlinearly propagates a finite ensemble of model trajectories instead
of using a linearized equation for the error covariance, so no computation of
derivatives is required. The EnKF still considers a linear correction
procedure and assumes Gaussian distributions of the random variables. When
this is not the case, the filter still produces a variance-minimizing
solution, though it is not the optimal estimate
(Bertino et al., 2007).</p>
      <?pagebreak page1272?><p id="d1e431">We develop below the fundamentals behind the algorithm. We first define the
true model state (corresponding to the actual physical state of the lake)
vector <inline-formula><mml:math id="M10" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula> of the system at time <inline-formula><mml:math id="M11" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (in our case temperature for the
entire 3D model grid), <inline-formula><mml:math id="M13" display="inline"><mml:mi mathvariant="script">M</mml:mi></mml:math></inline-formula> the nonlinear lake system operator, <inline-formula><mml:math id="M14" display="inline"><mml:mi mathvariant="italic">η</mml:mi></mml:math></inline-formula>
the process noise, and <inline-formula><mml:math id="M15" display="inline"><mml:mi mathvariant="bold-italic">u</mml:mi></mml:math></inline-formula> the forcing vector (here meteorological forcing) for
a time <inline-formula><mml:math id="M16" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>. The state propagation equation reads
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M17" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="script">M</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">η</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          In this study, the noise is added in the forcing term <inline-formula><mml:math id="M18" display="inline"><mml:mi mathvariant="bold-italic">u</mml:mi></mml:math></inline-formula> and subsequently
dropped in the notation of Eq. (2). The state space vector, noted <inline-formula><mml:math id="M19" display="inline"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula>,
is an approximation (done by the hydrodynamic model Delft3D-FLOW) of the
true state <inline-formula><mml:math id="M20" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula>. The forecast state (the input information for DA at time <inline-formula><mml:math id="M21" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>) is
defined by <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi mathvariant="normal">f</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> and the analysis state obtained after DA
as <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>. The model propagation equation now reads
            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M24" display="block"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="script">M</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          As we do not measure the true state of the system (<inline-formula><mml:math id="M25" display="inline"><mml:mi mathvariant="bold-italic">x</mml:mi></mml:math></inline-formula>), the observation (<inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="bold-italic">y</mml:mi></mml:math></inline-formula>)
equation is defined by the following, with <inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="bold">H</mml:mi></mml:math></inline-formula> an operator relating the system
state to the observation and <inline-formula><mml:math id="M28" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> is some measurement noise:
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M29" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">H</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="italic">ε</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          with the observation prediction given by
            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M30" display="block"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="bold">H</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          Note that in our case, we directly observe what we compute (i.e., surface
temperature and profiles at computed grid points), and therefore in this study <inline-formula><mml:math id="M31" display="inline"><mml:mi mathvariant="bold">H</mml:mi></mml:math></inline-formula> is
an identity matrix. The resulting data assimilation estimate of the state
vector <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi mathvariant="normal">a</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, which will be used in the next cycle as
restart condition, is given by
            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M33" display="block"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>K</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mover accent="true"><mml:mi mathvariant="bold-italic">y</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          That last equation (Eq. 5) is a central concept of DA; it introduces the
weighting factor <inline-formula><mml:math id="M34" display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula>, also referred to as Kalman gain. The Kalman gain can be
viewed as a balance of the model and observation uncertainties, together
with the error correlation of all the elements of the state vector. It aims
to minimize the error covariance of the state estimate during the analysis
time Eq. (5). It is defined as
            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M35" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="bold">K</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msubsup><mml:mi mathvariant="bold">P</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:msubsup><mml:mi mathvariant="bold">H</mml:mi><mml:mi>t</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi mathvariant="bold">H</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:msubsup><mml:mi mathvariant="bold">P</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:msubsup><mml:mi mathvariant="bold">H</mml:mi><mml:mi>t</mml:mi><mml:mi>T</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="bold">R</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          with <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">R</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the measurement error covariance matrix (in this study we assume
no cross-correlation between observation errors, and hence <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">R</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is diagonal
and determined from the uncertainty of the measurements; Sect. 2.4) and
<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="bold">P</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> the a priori state error covariance matrix. Error covariance is a key
component of DA. The EnKF is able to compute a time-varying covariance error
based on the dynamics of the system. This is a critical property when
considering variables with short decorrelation spatiotemporal scales
(Kuragano and Kamachi, 2000). In addition to the probability
density function of the state (when in the presence of process noise),
covariance estimation is achieved considering ensemble members. For an
ensemble of forecasts (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi>j</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>), each subject to a disturbance (e.g., in model
processes, forcing, or initial conditions), <inline-formula><mml:math id="M40" display="inline"><mml:mi mathvariant="bold">P</mml:mi></mml:math></inline-formula> is obtained from
            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M41" display="block"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold">P</mml:mi><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi>N</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfrac></mml:mstyle><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:msubsup><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mrow><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal">¯</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mrow><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:mo>-</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo mathvariant="normal">¯</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msubsup><mml:msup><mml:mo>)</mml:mo><mml:mi>T</mml:mi></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
          From Eq. (7) we can conclude that the error-spreading pattern across the domain
is indeed derived from the ensemble members in a systematic way. This is not
the case for some variational methods such as 3D-VAR, whereby the statistics
are considered isotropic with little variation over time. In the EnKF each
ensemble member is then updated individually (based on Eq. 5). The state
average over the ensemble provides the a posteriori state estimate. Additionally, in
contrast to the extended (or traditional) Kalman filter, there is no need to
propagate the state covariance nor to estimate the initial state covariance
and model error covariance matrices. The EnKF only uses the first and second
moments to construct the probability density functions; it cannot ensure
higher-order statistics by opposition to the particle filter
(Nakamura et al., 2006).</p>
      <p id="d1e1072">The EnKF is widely used for large systems with uncertain initial states, and
variants are still being developed to leverage its limitations
(Hoel et al., 2016). Several authors
(Bertino et al., 2007; Evensen,
1994; Verlaan and Heemink, 2001) found better performance for highly
nonlinear systems in comparison to the EKF. This approach can accommodate
large datasets or missing observations, and it can incorporate correlated
nonlinear and error measurement models. Moreover, the ensembles are easy to
implement in parallel fashion. Models with high dimensionality are well
suited for this type of assimilation, which requires a relatively low number
of ensemble members to produce stable and accurate results (detailed in the
Results section and Discussion section). We used this algorithm for the results
presented in this study.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>System setup</title>
      <p id="d1e1084">The aim of this section is to detail the various properties of the EnKF and
DA setup, which is specific to this study.</p>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Stochasticity and noise</title>
      <p id="d1e1094">The performance of a DA
experiment strongly depends on the characterization of uncertainties
(van Velzen and Verlaan, 2007). The hydrodynamics are modeled with
deterministic equations. Their initial conditions, in the case of Lake
Geneva, play only a limited role in basin-scale dynamics over long periods
of time (months, years). Yet, boundary conditions, especially the air–water
heat and momentum budgets, still contain large uncertainties that decrease
the performance of any theoretically perfectly calibrated model. To overcome
this issue, we added stochasticity to the system by including noise in the
east (<inline-formula><mml:math id="M42" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> direction) and north (<inline-formula><mml:math id="M43" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> direction) components of the wind velocity.
These variables, coming from MeteoSwiss COSMO-1 reanalysis products with DA,
are known to be the most inaccurate and influential boundary forcing over
lakes.</p>
      <?pagebreak page1273?><p id="d1e1111">The addition of stochasticity to the deterministic model is done with
OpenDA's noise model, which adds spatiotemporally correlated noise to the
wind fields. This noise model, distributing the noise based on correlation
scales derived from a distance-dependent function decaying to 0, requires
three quantities (for both the <inline-formula><mml:math id="M44" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M45" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> directions): (i) the wind standard
deviation, (ii) the wind spatial correlation scale, and (iii) the temporal
correlation scale. They are obtained from an analysis of the COSMO-E
(ensemble) products over the entire year of 2017. COSMO-E probabilistic
products are derived from 21-ensemble forecasts on a 2.2 km grid and contain
information on the variability of the computed atmospheric variables. The
wind standard deviation is hence obtained by taking the mean COSMO-E
standard deviation of every pixel over the lake for the studied period. The
spatiotemporal correlation scales are obtained by computing the
cross-correlations of six – fictive – stations around the lake, as shown by
Fig. 1. The cross-correlation of a station with itself provides the temporal
correlation scale, while the cross-correlation among stations allows
for the determination of the spatial correlation scale. Table 1 summarizes the
aforementioned noise model parameters.
<?xmltex \hack{\newpage}?></p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1132">Summary of the noise model parameters.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.9}[.9]?><oasis:tgroup cols="3">
     <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:thead>
       <oasis:row>
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">Description</oasis:entry>
         <oasis:entry colname="col3">Value</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">(<inline-formula><mml:math id="M46" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> direction, <inline-formula><mml:math id="M47" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> direction)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M48" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>  (m s<inline-formula><mml:math id="M49" 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>)</oasis:entry>
         <oasis:entry colname="col2">Wind standard deviation</oasis:entry>
         <oasis:entry colname="col3">1.11, 1.10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (m)</oasis:entry>
         <oasis:entry colname="col2">Wind spatial correlation</oasis:entry>
         <oasis:entry colname="col3">20 000, 30 000</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  (h)</oasis:entry>
         <oasis:entry colname="col2">Wind temporal correlation</oasis:entry>
         <oasis:entry colname="col3">5.67, 6.67</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>State variables</title>
      <p id="d1e1270">OpenDA has recently been updated to
support three Delft3D-FLOW state variables (Baracchini et al.,
2019a), namely water levels, temperatures, and flow velocities. In this
study, only temperatures are updated by the EnKF.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Ensembles</title>
      <p id="d1e1281">The EnKF operates using a statistical
sample of the state of the system. The ensemble size (<inline-formula><mml:math id="M52" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>) is often determined
heuristically and must be a balance between a good representation of the
state space and acceptable computation time. The errors in the solution probability distribution function (PDF)
will approach zero at the rate <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msup><mml:mi>N</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>    (Evensen, 2003). A
preliminary study showed that a satisfying compromise is obtained with 20
ensemble members. The choice for a small number of ensembles is further
motivated by future use for operational purposes. More details and an
ensemble size assessment are presented in the Results section.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <label>3.2.4</label><title>Localization scheme</title>
      <p id="d1e1318">As mentioned above (Sect. 3.1),
the covariance matrix links every domain point with the others. Covariances
are derived from the ensemble members. A limitation of a small ensemble size
is possible spurious correlations    (Evensen, 2009), resulting in
artifacts over long distances from the observation location. In such cases,
when the model spatial extent is large, a localization scheme has to be applied
(an observation usually only influences its near vicinity, and it has limited
influence for greater spatial extensions; Stanev et al.,
2011). Such a scheme has therefore been implemented in OpenDA, which
collaterally also aims to reduce the computational cost of the analysis time.
This localization allows users to define a cutoff distance based on a
Gaspari–Cohn isotropic distance-based function (decaying to 0 at a defined
cutoff distance) to limit the area of influence of an observation. This
function ensures a smooth transition between a full and non-update for
better model stability. Effectively, this removes long-range spurious
correlations by scaling the size of the observation covariance matrix.</p>
      <p id="d1e1321">In this study, a cutoff distance of 15 km is defined. This distance is
based on the spacing of the two in situ stations and the radius of their associated
basin gyres (Petit Lac and Grand Lac; Fig. 1). This is further motivated by
the fact that such a distance allows users to cover the entire interior of the
basin by an update of in situ data. Due to the significant depth of the
lake, dynamics at deeper locations are less variable, and hence their
correlations at longer distances are easier to estimate. Regarding the LSWT,
as it is partly the result of surface heat fluxes, its spatial structure is
also expected to be correlated, to some extent, at relatively large spatial
scales. Finally, as a result of the coarse vertical resolution of the
in situ profiles, we did not define a different localization scheme in the
vertical compared to the horizontal direction.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
      <p id="d1e1334">In this section, we present both quantitative and qualitative results of the
DA experiment. As mentioned in Sect. 2.4, the DA run consisted of the
assimilation of 128 AVHRR LSWT datasets and 31 in situ profiles over the
entire year of 2017. Mean absolute error (MAE), root mean square error
(RMSE), and a Taylor diagram    (Taylor, 2001) are used as benchmark
indicators. Direct model comparisons with satellite images and in situ
profiles are provided to visualize the benefits of the approach for both
surface and deepwater dynamics. Implications of the DA for physical
phenomena are presented.</p>
      <p id="d1e1337">Table 2, providing MAEs and RMSEs before and after
DA, indicates significant improvements over the baseline simulation. RMSE
and MAE values are reduced by 54 % and 60 %, respectively. The discrepancy
between the two indicate some occasional large data–model mismatch, which
affects the RMSE more heavily. The Taylor diagram (Fig. 2), displays large
improvements in centered root mean square difference (RMSD), correlation, and
standard deviation.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1343">Summary of the data assimilation performance (MAE and RMSE).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Control</oasis:entry>
         <oasis:entry colname="col3">DA</oasis:entry>
         <oasis:entry colname="col4">Improvement</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">run</oasis:entry>
         <oasis:entry colname="col3">run</oasis:entry>
         <oasis:entry colname="col4">(%)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">MAE (<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C)</oasis:entry>
         <oasis:entry colname="col2">1.49</oasis:entry>
         <oasis:entry colname="col3">0.60</oasis:entry>
         <oasis:entry colname="col4">60</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RMSE (<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C)</oasis:entry>
         <oasis:entry colname="col2">2.07</oasis:entry>
         <oasis:entry colname="col3">0.95</oasis:entry>
         <oasis:entry colname="col4">54</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1445">Taylor diagram of Lake Geneva temperature data assimilation. The
dots correspond to the observations (black), the control run without DA
(blue), and the DA run (red). The radial distance from the observations is
the centered root mean square difference; the radial distance from the
origin defines the standard deviation, and the azimuthal position is the
correlation coefficient.</p></caption>
        <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f02.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Surface assimilation and physical processes </title>
      <p id="d1e1461">The benefit of DA is shown with four examples in Fig. 3, comparing LSWT from
AVHRR measurements with LSWT from the control run model and DA experiment.
We first highlight (top panels) the fact that DA assimilation can perform correctly
even in the case of missing observations over the lake surface. The state
covariance matrix could update the model in areas where no data were
available. Model accuracy is thereby improved at the basin scale rather than at
observation locations. This is particularly relevant as large lakes are
often partly cloudy. The second example demonstrates the potential of DA to
correct the state variable – a cold bias in the present case – while
maintaining the<?pagebreak page1274?> coherent structure of the complex spatial thermal gradient
(Fig. 3, second row). The third example shows gyre-like flow structures.
Such rotating structures are difficult to observe from AVHRR LSWT data
(third row of Fig. 3), partly due to their limited spatial resolution and
weak signature at the surface. However, a gyre created by a NNE wind on
12 August is better visible in the model results (clockwise in the
western part of the main basin and counterclockwise in the center). In
that case, the DA updated the LSWT while keeping the physical structure and
flow spatial coherence of the control run. Finally, the lowest panels in
Fig. 3 show how DA improves observations and the future quantification of
transient upwelling. While the upwelling in the Petit Lac was partially
already caught by the control run, the DA allowed for a much better adjustment of its
intensity and extent. Another similar case is presented in Appendix B.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1466">Surface temperature comparison of the AVHRR observations (left
column), control run (central column), and DA run (right column) at selected
analysis times (four rows) in 2017. The first row highlights the
assimilation of sporadic data and the second row of complex surface
patterns. The third row is an example for gyre phenomena and the fourth row
of an upwelling event.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1477">Time series of the LSWT in the center of the lake. The red line
corresponds to the mean of the ensemble and the red shaded area to the
ensemble spread, while the blue line marks the control run and the black
dots the AVHRR observations. </p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f04.png"/>

        </fig>

      <p id="d1e1487">The benefit from DA is also evident when looking at the temporal evolution
of LSWT (Figs. 4 and 5). In Figs. 4 and 5, the AVHRR LSWT is again compared
at two locations with the simulations with and without DA. The observed
strong summer temporal variability with biweekly temperature variations
exceeding 5 <inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C is not well resolved in the control run (Fig. 4);
however, it is much better reproduced by applying DA. The warming phase also
benefits significantly from the assimilation. The control run surface
temperature started to increase in the second part of March, while the
warming occurred in early March in the observations and DA. Both models are in
good agreement during the cooling phase after August. While few observations
were available during this late period, not much improvement is obtained
for the baseline, which was already accurate. Overall, every point of the DA
run is close to or at least within the <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
uncertainty of the AVHRR observations (see Sect. 2.4 for more information
on uncertainty).</p>
      <p id="d1e1518">Similar conclusions arise from Fig. 5, which provides a close-up of
time series of the summer period in the western basin (Petit Lac). Ensemble
spread is smaller during the period of strongest stratification from late
July to late August. Overall, the model uncertainty arising from perturbed
wind fields reaches 2 <inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in the summer, when it is the highest
and 1 <inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C on average. Major upwellings in June and July are caught
by both model runs, although the intensity is too weak in the control run.
Again, data–model discrepancies and temperature variability are largest from
late May to early August. Starting in August, the models with and without DA
exhibit similar dynamics, both close to observations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e1541">Zoomed time series of LSWT in the center of the western basin
(Petit Lac). The red line corresponds to the mean of the ensemble, the red
shaded area to the ensemble spread, the blue line to the control run, and
the black dots to AVHRR observations.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f05.png"/>

        </fig>

      <p id="d1e1550">We further compared the upwelling of 15 September with river
temperature data with a model surface grid point located 3 km away (Fig. 6).
The upwelling has indeed been observed in the lake outflow, dropping from 21
to 12 <inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in 6 d. The figure shows that the
control run underestimated the upwelling by 5 <inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while the DA
run underestimated it by <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The AVHRR
observation was 1.5 <inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warmer than the river temperature. Figure 6
also confirms that the model does not suffer from spurious behavior after an
assimilation. Model shocks are not observed and numerical equilibrium is
reached in a sub-daily period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e1601">Close-up of the upwelling event in mid-September. River
temperature from the lake outlet in Geneva is added as a comparison. The AVHRR
data (black dots), control run (blue), and DA run (red) correspond to a
surface pixel 3 km from the outflow.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Deepwater assimilation</title>
      <p id="d1e1618">We investigated how the
vertical structure and subsurface dynamics are affected by the
DA. Figure 7 provides a comparison of the DA performance
over depth with in situ data instead of AVHRR measurements. Overall, for
both stations significant improvements are obtained over the entire water
column and throughout the year. Major improvements are observed at the
thermocline depth, correctly represented in the DA experiment. Its strong
vertical gradient significantly benefited from the assimilation of
temperature profiles. The warm bias between 5 and 25 m of depth, resulting in
an overestimation of the mixed layer depth in the control run, is
effectively eliminated.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e1623">Evolution of the deepwater temperature without and with DA. <bold>(a, c)</bold> The
differences of control runs minus in situ
observations; <bold>(b, d)</bold> the differences of DA runs minus
in situ observations. Panels <bold>(a–b)</bold> correspond to the center of the main basin
(SHL2; Fig. 1), and panels <bold>(c–d)</bold> correspond to Petit Lac (GE3; Fig. 1).</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Ensemble member size</title>
      <p id="d1e1652">Finally, we evaluated the
EnKF ensemble size needed by a convergence analysis. A period of 1.5 months,
from June to mid-July with a spin-up time of 2 weeks (without DA), is
selected for assessment. This period of weak spring thermal stratification
has been selected, as it is the time of the year with the most complex and
broadest range of dynamics (Fig. 4).</p>
      <p id="d1e1655">The results indicate that for an increasing number of ensembles (<inline-formula><mml:math id="M66" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>) the
analysis error decreases. Figure 8 provides RMSEs and MAEs for different
ensemble sizes, also differentiating between assimilated data sources. We
conclude that major gains are achieved with 10 ensemble members.<?pagebreak page1275?> For
in situ data only, 20 ensembles seem to be the sweet spot. Due to the much
larger number of AVHRR observations (i.e., one image provides thousands of
observations since it covers the entire spatial extent of the computational
grid), the red (AVHRR) and black (all measurements) lines are confounded.
Finally, assessment of the ensemble spread showed that few gains in
second-order moments were found with larger ensemble sizes. Indeed, in the
scope of this study, the additional benefits for <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> are
limited. At this stage, the 1 <inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C uncertainty of the AVHRR LSWT
data might become a limiting factor hindering further improvements.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e1688">Data assimilation performance as a function of ensemble size. The
dashed blue line corresponds to the error with respect to in situ
observations only; the red line is the same with respect to LSWT only, and the
black squares show the model error with respect to both observation sources.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f08.png"/>

        </fig>

      <p id="d1e1698">With a vision towards DA for operational lake forecasting systems and the
computational constraints associated with real-time hydrodynamics, we
conclude that 20 members provide a satisfactory compromise for the system
considered in this study.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
      <p id="d1e1711">The DA framework has brought significant improvements to the hydrodynamics
of Lake Geneva. It demonstrated its effectiveness to improve various
model-forecasted mesoscale to large-scale thermal features. The combination of
both in situ measurements and remote sensing observations allowed
for constraining the 3D thermal structure of the model throughout the water
column.</p>
      <p id="d1e1714">Surface time series (Fig. 4) indicated that spring–early summer
observations play a key role in improving the model performance during the
warming period    (Kourzeneva, 2014).<?pagebreak page1276?> This allows for an adequate
modeling of the lake warming, with significant implications expected for
water quality models and the typical spring phytoplankton blooms. Later in
the year, in late spring and summer, the AVHRR data revealed high-variability
temperature dynamics (e.g., upwellings), which are not reproduced by the
control run. It is the time when the largest ensemble spread is observed,
which indicates that the summer LSWT is sensitive to changes in wind
patterns. Additionally, ensemble spread stemming from spatiotemporally
correlated noise applied to the wind fields indicates that the model is
sensitive to changes in this forcing function. The effects on model outputs
are correctly described, and the uncertainty arising from this perturbation
ranged from 1 <inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C on average, with peak values at 2 <inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p>
      <p id="d1e1735">A similar conclusion can be drawn for subsurface thermal dynamics. Figure 7
indicates that data–model mismatches in the mixed layer appeared as the lake
started to warm and the thermocline formed. Compared to the control run, the
DA run exhibited both a more accurate warming phase and vertical
temperature gradient during the stratified period.</p>
      <p id="d1e1738">Overall, the performance of the EnKF has been notable in a broad range of
scenarios. Even with complex observational patterns, filter updates were
performed with different amplitudes at each spatial location (Fig. 3).
Those spatially varying updates are often in agreement with the physical
processes governing the hydrodynamics of the lake. Also, in the case of
incomplete or sporadic data, the EnKF updates behaved well, and good
combinations of data and system dynamics were found. Some authors
(De Lannoy et al., 2007b) found that when the update is
performed through the covariance propagation (in the case of missing
observations), the a posteriori state might not be correct and counteract the updates in
the surrounding locations. This behavior has not been observed in the
presented hydrodynamics of Lake Geneva. This indicates that the covariance
matrices were well estimated from the ensemble members and their physical
dynamics. The non-static covariance matrix derived from the EnKF allows for
longer-term studies, such as over the entire year, with complex changes in
the thermal structure of the water body. Time-varying covariance error
estimates for 3D models are complex tasks in DA. Analysis updates were not
intense or frequent enough to cause model shocks or solver failure. This
would have a minimal impact on the surface layers, since such corrections
would not be persistent due to the variable nature of surface layers and
sensitivity to atmospheric forcing. However, more issues would arise from
model shocks in<?pagebreak page1277?> the deep water, which could trigger movements of large water
volumes. Since in situ profiles have a much lower uncertainty than AVHRR
observations (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C vs. 1 <inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; Sect. 2.4),
intense state updates are more likely; however, they have not been observed
in this study and no model solver failure arose from the EnKF updates. After
significant updates, the model generally recovered over a sub-daily period.
Increasing the observational frequency (here limited to one satellite
observation per day) would increase the likelihood of encountering model
shocks, as equilibrium adjustment may not be reached between updates. Higher
computational costs also weigh into the data quality–quantity compromise,
particularly when considering near-real-time systems. Detailed discussions
regarding model error formulation are provided by Akella and Navon (2009)
and Daescu and Navon (2013) for variational data assimilation.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Physical processes</title>
      <p id="d1e1777">Figure 3 shows that various physical
processes, such as upwellings and gyres, are better resolved with the use of
EnKF. Upwellings typically occur more prominently at the beginning or end of
the season, when stratification is weaker. The better identification of such
processes is of prime importance for various water quality aspects (e.g.,
heat extraction, wastewater discharge,
water intakes; Gaudard et al., 2019). Yet the magnitude of such events has rarely been
quantified due to difficulties with their large-scale identification.
Through the combination of remote sensing observations and 3D hydrodynamic
modeling, we open new possibilities for monitoring and predicting such
phenomena. In this study we found that upwellings are better reproduced in
both intensity and spatial extent. Comparing temperature measurements with a
surface model grid point 3 km away from the outflow showed good agreements
after DA. An underestimation of the upwelling of 2.5 <inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C after DA
is observed (compared to 5 <inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C with the control run). Most of this
remaining difference can be attributed to the satellite underestimating the
event as well (by 1.5 <inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, with an uncertainty of 1 <inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C)
and the remoteness and depth (surface) of the pixel compared. For Lake
Geneva, this is of particular interest when an upwelling occurs in the
western basin (Petit Lac), dropping the outflow temperature for millions of
downstream residents. In terms of gyres, those structures are repeatedly
observed in Lake Geneva     (Bouffard et al., 2018;
Kiefer et al.,<?pagebreak page1278?> 2015). Because of the Coriolis force, subsequent strong
uplifts to down-lifts of the thermocline occur, which structure the lateral
dispersion of primary productivity    (Soomets et al., 2019).</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Ensemble size</title>
      <p id="d1e1824">Among the various ensemble
sizes assessed for this study (Fig. 8), we found that relatively small
ensemble sizes (<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula>) are enough to derive suitable
time-varying covariances and error-spreading patterns. This is particularly
important in the presence of variables with short decorrelation time and
spatial scales. Studies indicated that relatively small ensembles fail to
accurately estimate the small correlation patterns of remote observations
(Houtekamer and Mitchell, 2001). The localization scheme
implemented (Sect. 3.1), defining a cutoff radius around each
observation, allows users to circumvent this limitation.
Houtekamer and Mitchell (2001) found that for an increasing
ensemble size, the optimal cutoff value increases as well. Larger ensemble
sizes not only restrain the underestimation of ensemble spread and accuracy,
but also allow for the use of more remote observations. For DA experiments with
limited data, larger ensemble sizes may be a requirement to maximize
observational coverage.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Limitations and perspectives</title>
      <p id="d1e1845">A main limitation
of the EnKF is the Gaussian assumption, which in the case of large
data–model mismatches could have led to artifacts and unrealistic a posteriori state
values. This has not been observed in this analysis with the provided noise
definition and observational stochastic setup. Furthermore, while we did not
systematically study the physics after each analysis step, we think the
method can still be used for the study of physical processes, provided the
user assesses the intensity of those physical discontinuities. Out of the
152 assimilations, only 8 created some numerical instabilities in the
model, though they were small enough to prevent solver failure. The existence of an
upper limit to the amount of information assimilated was not investigated
here, as the aim of this work is to provide an operational system with data
assimilation in lakes.</p>
      <p id="d1e1848">Other difficulties arise in the presence of bias, whereby Kalman filtering
performs suboptimal corrections (Dee and Da Silva, 1998), as
observations and the model are assumed unbiased. Solutions for dealing with
biases in EnKF may become necessary     (De Lannoy et al.,
2007a). In the present approach, however, occasionally occurring model
biases have been effectively handled by the update. The DA model did not
drift back to its biased or control run state. We believe that this is a
result of the adequate initial parameterization of the model
(Baracchini et al., 2019a). This further highlights the crucial
importance of accurate model calibration and formulation before applying DA
experiments. It is worth noting that the EnKF is able to also provide updates
to parameters and forcing conditions, which in some cases may provide
more persistent improvements (for example, when time-varying parameters are
needed).</p>
      <p id="d1e1851">This DA experiment is time-consuming from a computational aspect. For
example, it took nearly 1 month to compute the present setup on a dual
Intel Xeon E5-2697v4 processor with 256 GB of memory, generating
close to a terabyte of data. While the analysis time for in situ data has
been reasonable (<inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> h), the immense number of observations
generated by an AVHRR image (entire coverage of the surface layer of the
computational grid) brought the analysis time up to 3 h for a single
image. This is largely due to the current lack of multi-core support for the
analysis step. A multi-core local analysis has been implemented in the scope
of this study for multi-variable (e.g., temperature with water levels and/or
flow velocities) assimilations, but gains can further be achieved from a
local analysis based on the observation localization scheme.</p>
</sec>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d1e1873">For managerial and scientific purposes, new monitoring and forecasting
tools covering wide ranges of spatiotemporal scales are of great
interest. The coverage of such scale breadth of inland waters is achieved by
combining three information sources, namely (i) in situ measurements, (ii) remote sensing observations, and (iii) model simulations. With data
assimilation (DA), optimal combinations can be achieved and valorized.</p>
      <p id="d1e1876">For several decades, DA has been applied in oceanography and atmospheric
sciences, yet its applications in limnology has remained limited. In this study,
we developed a flexible framework and tools to blend real-time data into
model simulations tailored to lakes. We applied this method to Lake Geneva
using large datasets consisting of a three-dimensional hydrodynamic model,
AVHRR lake surface water temperature, and in situ profiles over an entire
year. Results demonstrated the effectiveness of DA as significant gains were
obtained for both the surface and deepwater dynamics over a well-calibrated
baseline. We showed that both data types (in situ and remote sensing) are
important to constrain the entire spatial extent (horizontal and vertical)
of the model. Results also indicate that AVHRR data are a valid remote sensing (RS) data source
for DA into lake hydrodynamics, provided that observational error and
uncertainties are well defined.</p>
      <p id="d1e1879">In that regard, the use of an ensemble Kalman filter (EnKF) allowed us to
handle non-static covariance estimation, a key element of any DA problem.
Additionally, it is able to account for the uncertainties of each data
source. Those are essential elements influencing DA performance
(Qi et al., 2014). We found that the ensemble size played an
important role in reducing model errors. To keep their number limited, a
localization scheme has been implemented,<?pagebreak page1279?> hence circumventing the estimation
of improper small correlations at large distances
(Houtekamer and Mitchell, 2001). In that regard, while the
EnKF adds computational cost to the problem, it is capable of dynamically estimating
the stochastic model based on the physical properties of the
system. This is well encompassed by the paradox defined by
Bertino et al. (2007), stating that simple DA methods
become complex engineering tasks when the inconsistency between the
stochastic and the physical model becomes relevant. Due to the flexibility
of the tools developed and used, we that expect this procedure can be transferred
to other lake and hydrodynamic models with relatively minor modifications
(Baracchini et al., 2019b).</p>
      <p id="d1e1882">To conclude, this method has been designed with the vision of future near-real-time applications. Implications of DA in the operational context are
significant to provide robust and timely short-term forecasts, accurate
reanalysis products, and uncertainties for reliable water management. Over
the last decades, the number of remote sensing products has grown rapidly;
however, they have hardly been used in the operational context in an optimal
way    (de Rosnay et al., 2013). The timely retrieval and
processing of RS products requires interdisciplinary efforts to ensure
robustness and the proper error definition of the data, which hinders the
development of such operational systems    (van Velzen and Verlaan,
2007). In this study, we provided an example of how the entire chain, from
the satellite to assimilation into the model, can be performed with limited
field infrastructure. More concretely, we expect the findings of this study
to be directly applicable to existing lake forecasting platforms, such as
the one for Lake Geneva (<uri>http://meteolakes.ch</uri>, last access: 9 March 2020). Impacts of such an
implementation are expected at a scientific, governmental, and public level.</p><?xmltex \hack{\clearpage}?>
</sec>

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

<?pagebreak page1280?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>AVHRR validation</title>
<sec id="App1.Ch1.S1.SSx1" specific-use="unnumbered">
  <title>Validation</title>
      <p id="d1e1905">AVHRR data were validated for Lake Geneva by
comparing in situ data from the Buchillon station to the remote-sensing-derived skin temperature. Analysis of the data and comparison with
both radiometric and in situ observations at Buchillon showed that quality
flags are not a sufficient measure to reliably quantify the accuracy of the
AVHRR images but to improve the quality, avoiding errors (e.g., cloud-contaminated pixels). Indeed, we observed strong fluctuations of up to
<inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M81" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C between skin and bulk temperature, especially during
daytime when a micro-stratification establishes in the surface layer
(Gentemann et al., 2003). Skin and bulk temperature becomes similar
under windy or convective conditions. Skin-to-bulk corrections were
developed in oceanography as a function of the wind intensity
(Minnett et al., 2011). Yet, lakes are a much more calm
environment and parameterization should also take into account convective
processes    (Bouffard and Wüest, 2019). Such parameterization is
unfortunately lacking for Lake Geneva and we initially selected
nighttime to early morning images in which surface convective cooling reduces the
skin-to-bulk difference. However, comparison with field data showed that
this is still not reliable enough. The discrepancy is indeed strongly linked
to day–night cycles, but those are also season-dependent. Therefore, no
specific satellite overpass can be selected for the entire computational
time (1 year). To determine that images portray an accurate representation
of the lake bulk LSWT, the thermistor at 1 m of depth (recording at 1 h
intervals) has been used for a direct comparison with the spaceborne AVHRR
data. Considering that the Buchillon station is close (80 m) to the shore,
its position has been shifted 2 km south to avoid land boundary
contamination. Finally, the average of a <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> pixel window of the satellite
image centered on the south-shifted Buchillon station coordinates is used as
a comparison point with the field data. Only images with an absolute deviation
with respect to the bulk water lower than 1 <inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C are retained for
further assimilation. The 1 <inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C threshold will also define the
AVHRR observational uncertainty needed for the EnKF. Outlier pixel values
colder than 4 <inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and warmer than 28 <inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C are removed.
Finally, to avoid assimilating observations at a frequency that is too high (or too
close in time), which can result in physical discontinuities and the destruction
of model processes (model not reaching equilibrium between assimilations),
the maximum frequency of satellite images is limited to one per 24 h.
The screened images are then mapped to the computational grid.</p>
      <?pagebreak page1281?><p id="d1e1976">This procedure aims to bypass the skin-to-bulk temperature effect, while
ensuring the best data quality for assimilation. This procedure assumes
horizontal uniformity over the lake area (i.e., atmospheric effects are
assumed to be the same over the entire domain) and may be sensitive to
local cloud patches.
<?xmltex \hack{\clearpage}?></p>
</sec>
</app>

<app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><title>Additional results</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F9"><?xmltex \currentcnt{B1}?><label>Figure B1</label><caption><p id="d1e1991">Surface temperature comparison of the AVHRR observations (left
column), control run (central column), and DA run (right column) at selected
analysis times (four rows) in 2017. The first row highlights the
assimilation of sporadic data and the second row of complex surface
patterns. The third row is an example of upwelling phenomena and the fourth
row of gyre-like structures.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/13/1267/2020/gmd-13-1267-2020-f09.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e2008">The source code and documentation of the numerical model (Delft3D-FLOW) and
data assimilation platform (OpenDA) developed in and for this study can be
accessed and downloaded on their online repositories at: <uri>https://oss.deltares.nl/web/delft3d/source-code</uri> (last access: 9 March 2020) and <uri>https://github.com/OpenDA-Association/OpenDA</uri> (Barrachini, 2020).</p>

      <p id="d1e2017">The authors are grateful to the following institutions that provided the
data used in this paper: the Federal Office of Meteorology and Climatology
(MeteoSwiss) for meteorological data, the Département de
l'environnement, des transports et de l'agriculture (DETA) du Canton de
Genève for in situ data on Lake Geneva at GE3, and the Federal Office of the
Environment (FOEN) for the river data temperature in the outlet of Lake
Geneva. In situ data at SHL2 as well as Secchi disk measurements in Lake
Geneva were provided by the Commission International pour la Protection des Eaux du Leman (CIPEL) and the Information System of the
SOERE OLA (<uri>http://si-ola.inra.fr</uri>, last access: 5 June 2019), INRA, Thonon-les-Bains. These data cannot be
published as they belong to their aforementioned owners and are not the
property of the authors of this study. They can nonetheless be requested by
contacting the respective institution. Any other data used in this study are the
property of the Physics of Aquatic Systems Laboratory at EPFL and can be
obtained by contacting Alfred Johny Wüest (alfred.wueest@epfl.ch).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2026">TB, DB, AW, and PYC designed the procedure, and TB carried it out. PYC and JS
helped TB in the data assimilation implementation, and GL and SW retrieved and
processed the raw AVHRR data to generate LSWT. TB prepared the paper
with contributions from all coauthors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2032">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2038">The authors would like to thank Stef Hummel (Deltares) and Martin Verlaan
(TU Delft/Deltares) for their help implementing the coupling between
Delft3D-FLOW and OpenDA. This project was supported by the European Space
Agency's Scientific Exploitation of Operational Missions element (CORESIM
contract no. AO/1-8216/15/I-SBo).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2043">This research has been supported by the European Space Agency (grant no. AO/1-8216/15/I-SBo).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2049">This paper was edited by Adrian Sandu and reviewed by two anonymous referees.</p>
  </notes><?xmltex \hack{\newpage}?><ref-list>
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<abstract-html><p>The understanding of physical dynamics is crucial to
provide scientifically credible information on lake ecosystem management.
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size of 20 members is found to be sufficient to derive covariance matrices
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