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**Atmospheric Measurement Techniques**
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- Abstract
- Introduction
- Data
- SEVIRI cloud property retrieval algorithm
- Candidate methods for downscaling SEVIRI reflectances
- Example retrievals
- Evaluation of downscaling techniques with MODIS data
- Full downscaling versus VNIR only
- Conclusions
- Code and data availability
- Author contributions
- Competing interests
- Acknowledgements
- Financial support
- Review statement
- References

**Research article**
06 Mar 2020

**Research article** | 06 Mar 2020

Increasing the spatial resolution of cloud property retrievals from Meteosat SEVIRI by use of its high-resolution visible channel: evaluation of candidate approaches with MODIS observations

Increasing the spatial resolution of cloud property retrievals from Meteosat SEVIRI by use of its high-resolution visible channel: evaluation of candidate approaches with MODIS observations
Increasing the spatial resolution of cloud property retrievals from Meteosat SEVIRI by use of...
Frank Werner and Hartwig Deneke

^{1}Leibniz Institute for Tropospheric Research, Permoserstraße 15, 04318 Leipzig, Germany^{a}now at: Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA

^{1}Leibniz Institute for Tropospheric Research, Permoserstraße 15, 04318 Leipzig, Germany^{a}now at: Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA

**Correspondence**: Frank Werner (frank.werner@jpl.nasa.gov)

**Correspondence**: Frank Werner (frank.werner@jpl.nasa.gov)

Abstract

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This study presents and evaluates several candidate approaches for
downscaling observations from the Spinning Enhanced Visible and
Infrared Imager (SEVIRI) in order to increase the horizontal
resolution of subsequent cloud optical thickness (*τ*) and
effective droplet radius (*r*_{eff}) retrievals from the
native $\approx \mathrm{3}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{3}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$ spatial resolution of the
narrowband channels to $\approx \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$. These methods make
use of SEVIRI's coincident broadband
high-resolution visible (HRV) channel. For four example cloud fields,
the reliability of each downscaling algorithm is evaluated by means of
collocated 1 km×1 km MODIS radiances, which are
reprojected to the horizontal grid of the HRV channel and serve as
reference for the evaluation. By using these radiances, smoothed with the
modulation transfer function of the native SEVIRI channels, as retrieval
input, the accuracy at the SEVIRI standard resolution can be evaluated
and an objective comparison of the accuracy of the different
downscaling algorithms can be made. For the example scenes considered
in this study, it is shown that neglecting high-frequency
variations below the SEVIRI standard resolution results in significant
random absolute deviations of the retrieved *τ* and
*r*_{eff} of up to ≈14 and
≈6 µm, respectively, as well as biases. By error propagation, this
also negatively impacts the reliability of the subsequent calculation
of liquid water path (*W*_{L}) and cloud droplet number
concentration (*N*_{D}), which exhibit deviations of up to
$\approx \mathrm{89}\phantom{\rule{0.125em}{0ex}}\mathrm{g}\phantom{\rule{0.125em}{0ex}}{\mathrm{m}}^{-\mathrm{2}}$ and $\approx \mathrm{177}\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{3}}$, respectively. For *τ*, these deviations can be almost
completely mitigated by the use of the HRV channel as a physical constraint
and by applying most of the presented downscaling schemes. Uncertainties in retrieved *r*_{eff} at the native SEVIRI resolution are smaller, and the improvements from downscaling the observations are less obvious than for *τ*. Nonetheless, the right choice of downscaling scheme yields noticeable improvements in the retrieved *r*_{eff}. Furthermore, the improved reliability in retrieved cloud products results in significantly reduced uncertainties in derived *W*_{L} and *N*_{D}. In particular, one downscaling approach provides clear improvements for all cloud products compared to those obtained from
SEVIRI's standard resolution and is recommended for future downscaling endeavors. This work advances efforts to mitigate impacts of scale mismatches among channels of multiresolution instruments on cloud retrievals.

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Werner, F. and Deneke, H.: Increasing the spatial resolution of cloud property retrievals from Meteosat SEVIRI by use of its high-resolution visible channel: evaluation of candidate approaches with MODIS observations, Atmos. Meas. Tech., 13, 1089–1111, https://doi.org/10.5194/amt-13-1089-2020, 2020.

1 Introduction

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In studies of the role of clouds in the climate system,
the bispectral solar reflective method described by
Twomey and Seton (1980), Nakajima and King (1990), and Nakajima et al. (1991) is widely used to
infer cloud optical and physical properties from satellite-based
sensors. Based on observations of solar reflectance (*r*) from a
channel pair at wavelengths with conservative scattering (usually
around 0.6 or 0.8 µm) and significant
absorption by cloud droplets (common channels are 1.6, 2.2, and 3.7 µm),
respectively, this method simultaneously estimates the cloud
optical depth (*τ*) and effective droplet radius
(*r*_{eff}) of a sampled cloudy pixel. This method however
relies on a number of assumptions which are often violated in nature:
clouds are considered to be horizontally homogeneous and to have a
prescribed vertical structure, which is generally assumed to be
vertically homogeneous or to show a linear increase of liquid water
content as predicted by adiabatic theory (see the discussions in
Brenguier et al., 2000, and Miller et al., 2016). Moreover, the observed cloud
top reflectance field is usually described by one-dimensional (1-D)
plane-parallel radiative transfer, which neglects horizontal photon
transport between neighboring atmospheric columns.

Use of the independent pixel approximation (IPA; see
Cahalan et al., 1994a, b) produces uncertainties in the
retrieved cloud variables that are dependent upon the horizontal
resolution of the observing sensor. For sensors with a high spatial
resolution, the observations resolve the actual cloud heterogeneity,
which are unaccounted for in the IPA approach. This
usually results in an overestimation of both *τ* and
*r*_{eff}, as reported in Barker and Liu (1995),
Chambers et al. (1997), and Marshak et al. (2006). Conversely, for observations with a
low spatial resolution, the actual cloud heterogeneity cannot be
resolved. Moreover, the chances of clear-sky contamination within a cloudy pixel increase
with increasing spatial resolution. As a result, an underestimation (overestimation) of
retrieved *τ* (*r*_{eff}) is usually observed
(Marshak et al., 2006; Zhang and Platnick, 2011; Zhang et al., 2012; Werner et al., 2018b).
These uncertainties are propagated to the liquid water content (*W*_{L}) and the droplet number concentration (*N*_{D}), which can be estimated from retrieved *τ* and
*r*_{eff}. Estimates of *N*_{D} are especially susceptible to uncertainties in *r*_{eff}, which impacts the reliability of aerosol–cloud-interaction studies (Grosvenor et al., 2018).
The analysis in Varnai and Marshak (2001) suggests that a horizontal scale of around
1–2 km minimizes the combined uncertainty from unresolved
and resolved cloud heterogeneity. While strategies to mitigate the
effects of unresolved cloud variability have been recently reported in
Zhang et al. (2016) and Werner et al. (2018a), these techniques become less
successful with lower-resolution sensors like those operated on
geostationary satellites.

Remote sensing from geostationary platforms such as the Meteosat Spinning Enhanced Visible and Infrared Imager (SEVIRI) offers unique capabilities for cloud studies not available from polar-orbiting satellites. These advantages include more frequent temporal sampling of individual regions and the ability to capture the temporal evolution (Bley et al., 2016; Senf and Deneke, 2017) and diurnal cycle of cloud parameters (Stengel et al., 2014; Bley et al., 2016; Martins et al., 2016; Seethala et al., 2018). However, SEVIRI pixels are characterized by a lower spatial resolution of its narrow-band channels compared to other operational remote sensing instrumentation, like the Moderate Resolution Imaging Spectroradiometer (MODIS, Platnick et al., 2003) or the Visible Infrared Imaging Radiometer Suite (VIIRS, Lee et al., 2006). Given the increase in retrieval uncertainty due to the IPA constraints, there is a desire to increase the resolution for geostationary cloud observations.

The aim of this paper is to critically evaluate several candidate approaches for downscaling of the SEVIRI narrow-band reflectances for operational usage and to identify the most promising of these schemes, exploiting the fact that information on small-scale variability is available from its broadband high-resolution visible (HRV) channel. The study by Deneke and Roebeling (2010) presented a statistical downscaling approach of the SEVIRI channels in the visible to near-infrared (VNIR) spectral wavelength range. This method makes use of the fact that SEVIRI's high-resolution channel can be modeled by a linear combination of the 0.6 and 0.8 µm channels with good accuracy (Cros et al., 2006). This study advances these efforts in three ways: (i) it explores other possible downscaling approaches, which might improve upon the statistical downscaling scheme; (ii) it introduces techniques to accurately capture information on the small-scale reflectance variability in the 1.6 µm channel, which predominantly arises from variations in effective droplet radius; and (iii) it studies the impact of the various downscaling techniques on the subsequently retrieved cloud properties.

A critical requirement, formulated at the start of this work, is to maintain a target accuracy for the retrieved effective radius based on the lower-resolution observations, while hoping for further improvements. This goal was set because the error in effective radius will propagate into other cloud products such as vertically integrated liquid or ice water path or the cloud droplet number concentration, thereby potentially corrupting any gains in accuracy obtained from the improved spatial resolution. However, without an independent reference data set, it is impossible to determine whether this target can be met. Thus, higher-resolution reflectance observations from Terra MODIS are remapped to SEVIRI’s HRV and standard-resolution grids here as basis for a thorough evaluation of the accuracy of the retrieved cloud parameters. This allows us to objectively benchmark the accuracy of candidate approaches by comparison of results from a true ≈1 km resolution reflectance data set and processed with an identical retrieval scheme. Note that even the retrieved cloud products from a hypothetically perfect downscaling technique would still be impacted by the effects of resolved and unresolved cloud variability. Therefore, the results of this study will not help to mitigate the uncertainties associated with the retrieval schemes of similar ≈1 km sensors (e.g., clear-sky contamination, plane-parallel albedo bias, three-dimensional radiative effects).

The results of this study are relevant for many other passive satellite sensors, which, like the SEVIRI instrument, feature multiple resolutions for the conservative and absorbing channels. Similar configurations exists for the MODIS instrument (250 m horizontal resolution versus 500 m for the 0.6 and 2.1 µm channels, respectively), VIIRS (375 m versus 750 m), and GOES-R (500 m versus 1 km).

The structure of the paper is as follows: Sect. 2 describes both the SEVIRI and MODIS instruments used as basis for this study, as well as the covered observational domain. A brief overview of the SEVIRI cloud property retrieval algorithm is given in Sect. 3, followed by a description of the different candidate approaches for the downscaling of the narrow-band SEVIRI channel observations in Sect. 4. An example of lower- and higher-resolution cloud property retrievals is presented in Sect. 5. A statistical evaluation of the different downscaling approaches based on remapped MODIS observations follows in Sect. 6 for a limited number of example cloud fields. Finally, a comparison between a full downscaling scheme and a VNIR-only approach (similar to Deneke and Roebeling, 2010) is given in Sect. 7. The paper presents the main conclusions and an outlook in Sect. 8.

2 Data

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This section gives an overview of both the SEVIRI and MODIS instruments in Sect. 2.1 and 2.2. Here, the respective spectral channels of interest for this study are listed. Subsequently, the observational domain is described in Sect. 2.3.

The current version of European geostationary satellites is the
Meteosat Second Generation, which has provided operational data since 2004
(Schmetz et al., 2002). The SEVIRI imager is installed aboard the
Meteosat-8 to Meteosat-11 platforms, which are positioned above
longitudes of 9.5^{∘} E and 0.0^{∘}, respectively. One SEVIRI
instrument samples the full disk of the Earth from 0.0^{∘} longitude with a
temporal resolution of 15 min. However, a backup satellite
positioned at 9.6^{∘} E also scans a northern subregion with a
temporal resolution of 5 min (the so-called Rapid Scan
Service). These samples – in our case from Meteosat-9 – provide the
observational SEVIRI data set for the following analysis.

This study mainly considers observations from SEVIRI's solar
reflectance channels 1–3, as well as from the spectrally broader HRV
band. These channels cover the VNIR and
shortwave-infrared (SWIR) spectral wavelength ranges. The two VNIR
reflectances (*r*_{06} and *r*_{08}) are sampled in
bands 1 and 2, respectively, and are centered around wavelengths
*λ*=0.635 and *λ*=0.810 µm. SWIR reflectances (*r*_{16}) are provided by channel 3
observations, which are centered around *λ*=1.640 µm. The horizontal resolution of the channel 1–3 samples is 3 km×3 km at the subsatellite point and increases with higher sensor zenith angles.
Conversely, the broadband reflectances *r*_{HV} are sampled at SEVIRI's HRV channel at a horizontal
scale of 1 km×1 km at the subsatellite point. These observations cover the
spectral range of 0.4–1.1 µm.

As context for the present study, the reader is reminded that the spatial resolution of geostationary satellites is significantly reduced at higher latitudes due to the oblique viewing geometry. For Germany and Central Europe as considered in this paper, the pixel size is effectively increased by a factor of 2 in the north–south direction as a result. In addition, the distinction between sampling and optical resolution needs to be acknowledged. While the former determines the distance between recorded samples, the latter is given by the effective area of the optical system, which is larger by a factor of 1.6 than the sampling resolution for SEVIRI (Schmetz et al., 2002). The spatial response of optical systems is commonly characterized by their modulation transfer function, which describes the response of the optical system in the frequency domain.

Further information about the spectral width of each SEVIRI channel, as well as the respective spatial response and modulation transfer functions, can be found in Deneke and Roebeling (2010).

The 36-band scanning spectroradiometer MODIS, which was launched aboard NASA’s Earth Observing System satellites Terra and Aqua, has a viewing swath width of 2330 km, yielding global coverage every 2 d. MODIS collects data in the spectral region between 0.415 and 14.235 µm, covering the VNIR to thermal-infrared spectral wavelength range. In general, the spatial resolution at nadir of a MODIS pixel is 1000 m for most channels, although the pixel dimensions increase towards the edges of a MODIS granule. Only observations from the Terra satellite launched in 1999 are used here, due to broken detectors of the 1.64 µm channel of the MODIS instrument on the Aqua satellite. Information on MODIS and its cloud product algorithms is given in Ardanuy et al. (1992), Barnes et al. (1998), and Platnick et al. (2003). The current version of the level 1b radiance and level 2 cloud products used is data collection 6.1 (C6.1).

In this study, data from a subregion of the full SEVIRI disk has been
selected. This region, which is located within the European subregion
described in Deneke and Roebeling (2010), is illustrated by the red borders in
Fig. 1. It is centered around Germany due to its
intended domain of application (thus, from here on it is referred to
as the Germany domain) and comprises the latitude and longitude ranges of
≈44.30–57.77^{∘} and $\approx -\mathrm{0.33}$–21.65^{∘},
respectively. This domain includes 240×400 lower-resolution
pixels (i.e., the native SEVIRI resolution of channels 1–3) and is far away from the edges of the full SEVIRI
disk, ensuring that the observed viewing zenith angles are
$<\mathrm{70}{}^{\circ}$.

Due to the increased sensor zenith angles the spatial resolution of each SEVIRI pixel is degraded. The average pixel size is 6.20 km×3.22 km and 2.06 km×1.07 km for channels 1–3 and the HRV channel, respectively. To avoid confusion, we will use the designations LRES (abbreviation for lower resolution) and HRES (abbreviation for higher resolution) scales to refer to the 3 km×3 km and 1 km×1 km pixel resolutions from here on.

A relatively small domain was chosen, because the number of pixels to be processed will expand by a factor of 3×3, increasing the computational costs of the subsequent cloud property retrievals by roughly 1 order of magnitude. Except for some regional dependencies introduced by changes in the prevalence of specific cloud types, we expect results of our study to also be valid for other domains.

3 SEVIRI cloud property retrieval algorithm

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Retrieved cloud variables in this study are provided by the Cloud
Physical Properties retrieval algorithm (CPP;
Roebeling et al., 2006), which is developed and maintained at the
Royal Netherlands Meteorological Institute (KNMI). It is used as basis for
the CLAAS-1 and CLAAS-2 climate data records (Stengel et al., 2014; Benas et al., 2017) distributed by the Satellite Application Facility on
Climate Monitoring (Schulz et al., 2009). Using a lookup table (LUT) of
reflectances simulated by the Doubling–Adding KNMI (DAK:
, ) radiative transfer model, observed and
simulated reflectances at 0.6 and 1.6 µm are iteratively matched to yield estimates of *τ* and
*r*_{eff}. The CPP retrieval uses the cloud mask and cloud
top height products obtained from the software package developed and
distributed by the satellite application facility of Support to
Nowcasting and Very Short Range Forecasting (NWCSAF), version 2016, as
input (Le Gléau, 2016). The former product identifies cloudy pixels
for the retrieval, while the information on the height of the cloud is
used to account for the effects of gas absorption in the SEVIRI
channels.

4 Candidate methods for downscaling SEVIRI reflectances

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This section describes the necessary steps to convert the
reflectances *r*_{06}, *r*_{08}, and *r*_{16},
available at SEVIRI's native LRES, to reliable estimates of higher-resolution
reflectances ${\widehat{r}}_{\mathrm{06}}$, ${\widehat{r}}_{\mathrm{08}}$, and
${\widehat{r}}_{\mathrm{16}}$, together with matching cloud properties, at the
HRES scale of the HRV channel. This
downscaling process utilizes the high-resolution *r*_{HV}
observations.

As a first step, all reflectances are interpolated to the HRV grid using trigonometric interpolation, implemented based on the discrete Fourier transform and multiplication with the modulation transfer function (see Deneke and Roebeling, 2010, for details). While this step increases the spatial sampling resolution, it does not add any additional high-frequency variability. In fact, after interpolation, the reflectance values of the central pixel of each 3×3 pixel block equal those of the corresponding standard-resolution pixel reflectances. However, the pixels apart from the central one contain information about the large-scale reflectance variability and can be considered as a baseline high-resolution approach. This approach already improves the agreement with true higher-resolution retrievals, as will be shown later in this study.

Three conceptually different downscaling techniques to improve upon
this baseline method are described: (i) a statistical downscaling approach based on globally
determined covariances between the SEVIRI reflectances in Sect. 4.1; (ii) a local method based on
assumptions about the ratio of reflectances at different scales in
Sect. 4.2; and (iii) a technique combining
globally determined covariances between the VNIR reflectances and the
shape of the SEVIRI LUT, while assuming a constant
*r*_{eff} within a standard SEVIRI pixel in order to constrain
the SWIR reflectance in Sect. 4.3. As variations of this last technique, two
additional approaches are considered to improve upon the constant
*r*_{eff} constraint in Sect. 4.4. As will be shown, each of these
approaches has advantages and disadvantages, and the impact on the
cloud property retrievals will be evaluated in Sect. 6
for a number of example scenes by means of collocated MODIS
observations.

As is discussed in Sect. 4.1–4.4, the derived reflectances ${\widehat{r}}_{\mathrm{06}}$ and
${\widehat{r}}_{\mathrm{08}}$, as well as ${\widehat{r}}_{\mathrm{16}}$, include
an estimate of the spectrally dependent, high-frequency variability
of an image and are based on the actually observed
*r*_{HV}. These reflectances are different from those obtained by
trigonometric interpolation of the respective channel observations at the native scale to the horizontal
resolution of the HRV channel (i.e., the baseline approach), which are denoted by
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}$, ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{08}}$, and
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$. While these latter variables also have a
higher horizontal resolution of the HRV channel, they only
capture the low-frequency variability resolved by SEVIRI channels 1–3.

The statistical downscaling algorithm for the two SEVIRI VNIR
reflectances was first reported in Deneke and Roebeling (2010) and assumes a
least-squares linear model that links *r*_{06} and
*r*_{08} to the reflectances in the HRV channel (see
Cros et al., 2006) in the form

$$\begin{array}{}\text{(1)}& \u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a=a\cdot {r}_{\mathrm{06}}+b\cdot {r}_{\mathrm{08}}.\end{array}$$

Here, the HRV channel observations are first smoothed with the
modulation transfer function of the lower-resolution channels, which yields
reflectances ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}$ at the same HRES horizontal resolution, adjusted to the
low-frequency variability at the spatial scale of the channel 1–3
observations. Subsampling the central pixel of each $\mathrm{3}\times \mathrm{3}=\mathrm{9}$
pixel block subsequently yields $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$ at the same LRES horizontal
resolution as *r*_{06} and *r*_{08} (here, the
subsampling of the field is denoted by 〈〉). The variables *a* and *b* are fit coefficients that
are determined empirically by a least-squares linear fit. In order to
derive a statistically significant and stable linear model, the
coefficients *a* and *b* are calculated hourly between
08:00 and 16:00 UTC within 16 d intervals. Results for the time step
08:00 UTC are derived from 5 min SEVIRI rapid-scan data
between 08:00 and 08:25 UTC, while the 16:00 UTC time step is
comprised of SEVIRI observations between 15:30 and 16:00 UTC. For all
time steps in between, data are from all samples after minute 25 of
the prior hour up to minute 25 of the current hour (e.g., fit
coefficients for time step 09:00 UTC are calculated from SEVIRI
observations between 08:30 and 09:25 UTC).

Values of hourly derived fit coefficients for the Germany domain
between 1 April and 31 July 2013 are shown in Fig. 2a and b for *a* and *b*,
respectively. Here, circles represent the respective fit coefficient
for each 16 d interval, which is indicated by the first Julian day
in the time period. Colors highlight the different UTC time steps. It
is obvious that both coefficients *a* and *b* are very stable and show
no noticeable variation from hour to hour, as well as from one 16 d
interval to another. Considering all hourly data and each 16 d interval, the median fit coefficients are 0.63 (for *a*)
and 0.40 (for *b*), with low interquartile ranges (IQR) of
0.03. The only exceptions are the fit coefficients derived for the
first time period of 1–17 April 2013, especially for the morning and
afternoon hours of 08:00–09:00 and 13:00–16:00 UTC. Here, *a* and
*b* deviate significantly from the other results, with values of
≈0.50 and ≈0.52, respectively, likely due to an
abundance of observations with large solar zenith angles of ${\mathit{\theta}}_{\mathrm{0}}>\mathrm{60}{}^{\circ}$ in the eastern part of the domain.

The high-frequency reflectance variations for the SEVIRI HRV channel
(*δ**r*_{HV}) are calculated as the difference between the
observed *r*_{HV} and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}$, which only
resolve the low-frequency variability:

$$\begin{array}{}\text{(2)}& \mathit{\delta}{r}_{\mathrm{HV}}={r}_{\mathrm{HV}}-{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}.\end{array}$$

Following the linear model in Eq. (1), the high-frequency variations of the channel 1 and 2 reflectances (*δ**r*_{06} and *δ**r*_{08}) are linked to *δ**r*_{HV} via

$$\begin{array}{}\text{(3)}& \begin{array}{rl}\mathit{\delta}{r}_{\mathrm{06}}& ={S}_{\mathrm{06}}\cdot \mathit{\delta}{r}_{\mathrm{HV}},\\ \mathit{\delta}{r}_{\mathrm{08}}& ={S}_{\mathrm{08}}\cdot \mathit{\delta}{r}_{\mathrm{HV}}.\end{array}\end{array}$$

The optimal slopes *S*_{06} and *S*_{08}, which minimize the least-squares deviations, can be derived from bivariate statistics:

$$\begin{array}{}\text{(4)}& \begin{array}{rl}{k}_{\mathrm{1}}& =\sqrt{{\displaystyle \frac{{b}^{\mathrm{2}}\cdot \mathrm{var}\left({r}_{\mathrm{08}}\right)}{{a}^{\mathrm{2}}\cdot \mathrm{var}\left({r}_{\mathrm{06}}\right)}}},\\ {S}_{\mathrm{06}}& ={\displaystyle \frac{\mathrm{1}+{k}_{\mathrm{1}}\cdot \mathrm{cor}({r}_{\mathrm{06}},{r}_{\mathrm{08}})}{a\cdot \left[\mathrm{1}+{{k}_{\mathrm{1}}}^{\mathrm{2}}+\mathrm{2}{k}_{\mathrm{1}}\cdot \mathrm{cor}({r}_{\mathrm{06}},{r}_{\mathrm{08}})\right]}},\\ {k}_{\mathrm{2}}& =\sqrt{{\displaystyle \frac{{a}^{\mathrm{2}}\cdot \mathrm{var}\left({r}_{\mathrm{06}}\right)}{{b}^{\mathrm{2}}\cdot \mathrm{var}\left({r}_{\mathrm{08}}\right)}}},\\ {S}_{\mathrm{08}}& ={\displaystyle \frac{\mathrm{1}+{k}_{\mathrm{2}}\cdot \mathrm{cor}({r}_{\mathrm{08}},{r}_{\mathrm{06}})}{b\cdot \left[\mathrm{1}+{{k}_{\mathrm{2}}}^{\mathrm{2}}+\mathrm{2}{k}_{\mathrm{2}}\cdot \mathrm{cor}({r}_{\mathrm{08}},{r}_{\mathrm{06}})\right]}}.\end{array}\end{array}$$

Here, cor(*r*_{06},*r*_{08}) is the linear correlation coefficient
between the channel 1 and 2 reflectances, while
var(*r*_{06}) and
var(*r*_{08}) are the spatial variances of
the respective samples. Note that the sampling resolution of all
reflectances is the LRES scale (i.e., $\approx \mathrm{3}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{3}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$).

As a result, the high-resolution reflectances ${\widehat{r}}_{\mathrm{06}}$ and ${\widehat{r}}_{\mathrm{08}}$, which include the high-frequency variations, can be derived from the interpolated reflectances as

$$\begin{array}{}\text{(5)}& \begin{array}{rl}{\widehat{r}}_{\mathrm{06}}& ={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}+\mathit{\delta}{r}_{\mathrm{06}},\\ {\widehat{r}}_{\mathrm{08}}& ={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{08}}+\mathit{\delta}{r}_{\mathrm{08}}.\end{array}\end{array}$$

Note that only ${\widehat{r}}_{\mathrm{06}}$ is used for the retrieval.

Similar steps can be applied for the calculation of
${\widehat{r}}_{\mathrm{16}}$. Again, a simple linear model is assumed to
connect *r*_{16} to the lower-resolution $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$ at the spatial scales of the channel
1–3 observations:

$$\begin{array}{}\text{(6)}& \u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a=c\cdot {r}_{\mathrm{16}}.\end{array}$$

The symbol *c* is used to denote the respective fit coefficient, which
needs to be determined empirically. Similar to the coefficients *a*
and *b* from the linear model for the VNIR reflectances, *c* is
calculated hourly between 08:00 and 16:00 UTC within 16 d
intervals. It has to be noted, however, that in contrast to the VNIR
reflectances this fit does not have a clear physical motivation, as
there is no spectral overlap with the HRV channel.

The temporal behavior of the fit coefficient *c* for the Germany
domain for the time period between 1 April and 31 July 2013 is shown in
Fig. 2c. In contrast to the
coefficients *a* and *b*, there is a noticeable trend in the data,
both diurnally and during the transition from 1 April to 31 July. For each 16 d interval the variability in the hourly derived *c* values
ranges between IQR=0.05 and 0.15, while the median 16 d
value varies between 1.04 and 1.25. Overall, the median *c* is
1.16, with an IQR of 0.08 (i.e., almost 3 times larger than
the one for the coefficients *a* and *b*). The observed trends and
larger IQR in the *c* data set shown in Fig. 2c illustrate that the linear model in
Eq. (6) is not ideal and is expected to
introduce significant uncertainties in the calculation of
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$. This behavior is expected, as the relationship between VNIR and SWIR reflectance can usually not be described by a linear function (see discussions in Werner et al., 2018a, b, as well as the LUT examples in Fig. 4 later in this study).
For a constant *r*_{eff} there is a linear increase in *r*_{16} with increasing *r*_{06}, as the cloud optical thickness increases. However, the slope of this linear relationship increases with decreasing *r*_{eff}.
For *τ*>10 the relationship between *r*_{16} and *r*_{06} is characterized by a prominent curvature, while for *τ*≫10 the *r*_{16} values become independent of *r*_{06}.
Therefore, the fit coefficients *c* depend on the distribution of cloud optical and microphysical parameters, which varies widely with cloud type, meteorological conditions, and different dynamic processes.

Values of ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$ can be derived similarly to Eqs. (3–5) for the channel 1 and 2 observations:

$$\begin{array}{}\text{(7)}& \begin{array}{rl}\mathit{\delta}{r}_{\mathrm{16}}& ={S}_{\mathrm{16}}\cdot \mathit{\delta}{r}_{\mathrm{HV}},\\ {S}_{\mathrm{16}}& ={\displaystyle \frac{\mathrm{cov}({r}_{\mathrm{16}},\u2329{\stackrel{\mathrm{\u0303}}{\mathrm{r}}}_{\mathrm{HV}}\u232a)}{\mathrm{var}\left({r}_{\mathrm{16}}\right)}},\\ {\widehat{r}}_{\mathrm{16}}& ={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}+\mathit{\delta}{r}_{\mathrm{16}}.\end{array}\end{array}$$

Note that the use of linear models and bivariate statistics means that the downscaling algorithm described in this section is an example of statistical downscaling techniques, which are common in climate science applications (e.g., Benestad, 2011). While for the VNIR channels the spectral overlap with the HRV channel and the spectrally flat properties of clouds provide a sound physical justification for this technique, this is not the case for the SWIR channel.

The reliability of the linear model in Eq. (1)
depends upon the correlation between channel 1 and 2 reflectances (i.e.,
cor(*r*_{06},*r*_{08})), as
well as the stability of the fit coefficients *a* and *b*. The
analysis in Deneke and Roebeling (2010) concludes that the explained variance
in the estimates of ${\widehat{r}}_{\mathrm{06}}$ and
${\widehat{r}}_{\mathrm{08}}$ is close to 1, corresponding to low
residual variances, which indicates that the linear model is
robust. Moreover, the two fit coefficients are found to exhibit very
low variability, as shown in Fig. 2a–b.

To verify the reliability of the linear model with a large SEVIRI data
set, a joint PDF of the actually observed $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$ and the results from
Eq. (1) is shown in Fig. 3a; data are
from all SEVIRI observations within the Germany domain during June 2013. In case of an ideal linear model, as well as a perfect
correlation between the two reflectances, Eq. (1)
would replicate the $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$
observations. Conversely, deviations from these assumptions will yield
different results from the sampled SEVIRI reflectances. It is clear
that the linear model can reliably reproduce $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$, as most of the observations lie
on the 1:1 line, and Pearson's product-moment correlation
coefficient (*R*) is *R*=0.999. While some larger deviations exist,
such occurrences are significantly less likely (i.e., the joint
probability density is several orders of magnitude lower than the
most-frequent occurrences along the 1:1 line). Regarding
*r*_{16}, the assumption of a linear model is evidently flawed,
because the relationship between VNIR and SWIR reflectances depends on
the optical and microphysical cloud properties. As a result, a single
linear slope, which describes the whole relationship between the two
reflectances for all distributions of cloud properties, will introduce significant
uncertainties. This is illustrated in Fig. 3b, where the
joint PDF of $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$ and
the results from the linear model in Eq. (6) are
shown. The comparison between the two data sets reveals a much larger
spread around the 1:1 line and a lower correlation
coefficient. Overall, the relationship resembles the shape of a LUT,
displayed in the form of the well-known diagram introduced by
Nakajima and King (1990), where changes in *r*_{eff} result in a
spread in the observed SWIR reflectances (see, e.g.,
Werner et al., 2016).

To test the impact of changes in *a* and *b* on the derived
${\widehat{r}}_{\mathrm{06}}$ and ${\widehat{r}}_{\mathrm{08}}$, two experiments are
conducted: (i) the fit coefficients are derived only from cloudy
pixels and are compared to the higher-resolution results from *a* and
*b*, which are derived for all pixels; and (ii) the Germany domain is
divided into 100 km×100 km subscenes, and the fit coefficients are derived more locally within each subscene instead of
globally from the full domain. Subsequently, statistics from the
difference between the two data sets are calculated. Data are from 14 June 2013 at 14:05 UTC. For experiment (i), the 1st,
50th, and 99th percentiles of the relative
difference in ${\widehat{r}}_{\mathrm{06}}$ (defined as the difference
between the reflectances from only cloudy data and the full data set,
normalized by the full data set) are −0.08, −0.02, and 0.03 *%*, while for
${\widehat{r}}_{\mathrm{08}}$ the analysis yields −0.04, 0.02, and
0.19 %. Similarly, experiment (ii) yields relative differences of
−0.08, 0.03, and 0.36 *%* and −0.17, 0.00, and 0.19 % for
${\widehat{r}}_{\mathrm{06}}$ and ${\widehat{r}}_{\mathrm{08}}$, respectively. These
deviations are negligible compared to the measurement uncertainty, and
naturally the correlation coefficients between the different data
sets are *R*≈1.00. This confirms the robustness of the linear
model described in Eq. (1). For the derivation of
${\widehat{r}}_{\mathrm{16}}$ from Eq. (6), a slightly
increased sensitivity to the fit coefficient *c* is observed. Here,
experiment (i) yields percentiles of the relative difference of
−0.16, 0.08, and 0.86 %, whereas experiment (ii) results in −0.39,
−0.01, and 0.40 %. While slightly higher deviations are observed compared
to the linear model for the VNIR reflectances, the uncertainty in
${\widehat{r}}_{\mathrm{16}}$ induced by the variability in *c* is still
significantly lower than the measurement uncertainty.

Compared to the downscaling approach in Sect. 4.1, where fit coefficients for a linear
model are derived over a large temporal and spatial domain, this
second method uses local relationships (i.e., on the pixel level)
between the SEVIRI reflectances. The constant reflectance
ratio approach was introduced by Werner et al. (2018b) and is based on
the assumption that the inhomogeneity index of the HRV reflectance
(*H*_{σ,HV}, defined as the ratio of standard deviation
*σ*_{HV} to the average, pixel-level reflectance
$\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$) equals that for
the channel 1 reflectance (*H*_{σ,06}). This implies a spectrally
consistent subpixel reflectance variability. The relationship can be
written as

$$\begin{array}{}\text{(8)}& \begin{array}{rl}{H}_{\mathit{\sigma},\mathrm{06}}& ={H}_{\mathit{\sigma},\mathrm{HV}},\\ {\displaystyle \frac{{\mathit{\sigma}}_{\mathrm{06}}}{{r}_{\mathrm{06}}}}& ={\displaystyle \frac{{\mathit{\sigma}}_{\mathrm{HV}}}{\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a}},\\ & {\displaystyle \frac{\sqrt{\frac{\mathrm{1}}{\mathrm{9}-\mathrm{1}}\cdot {\sum}_{i=\mathrm{1}}^{i=\mathrm{9}}({\widehat{r}}_{\mathrm{06},\mathrm{i}}-{r}_{\mathrm{06}}{)}^{\mathrm{2}}}}{{r}_{\mathrm{06}}}}\\ & ={\displaystyle \frac{\sqrt{\frac{\mathrm{1}}{\mathrm{9}-\mathrm{1}}\cdot {\sum}_{i=\mathrm{1}}^{i=\mathrm{9}}({r}_{\mathrm{HV},\mathrm{i}}-\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a{)}^{\mathrm{2}}}}{\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a}},\end{array}\end{array}$$

where the index $i=\mathrm{1},\mathrm{2},\mathrm{\dots},\mathrm{9}$ indicates any one of the nine available HRES subpixels within a lower-resolution SEVIRI pixel (i.e., at the LRES scale of channels 1–3). This relationship can be further simplified, assuming that this relationship is also true for individual pixels:

$$\begin{array}{}\text{(9)}& \begin{array}{rl}{\displaystyle \frac{{\widehat{r}}_{\mathrm{06},\mathrm{i}}-{r}_{\mathrm{06}}}{{r}_{\mathrm{06}}}}& ={\displaystyle \frac{{r}_{\mathrm{HV},\mathrm{i}}-\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a}{\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a}},\\ {\displaystyle \frac{{\widehat{r}}_{\mathrm{06},\mathrm{i}}}{{r}_{\mathrm{HV},\mathrm{i}}}}& ={\displaystyle \frac{{r}_{\mathrm{06}}}{\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a}}.\end{array}\end{array}$$

The relationship in Eq. (9) suggests that the ratio of channel 1 and HRV reflectances (i.e., narrowband and broadband VNIR reflectances) remains constant for different scales. Thus, this approach is called the constant reflectance ratio approach.

Finally, we can mitigate some of the scale effects by substituting the lower-resolution variables with the higher-resolution reflectances that resolve the low-frequency variability (i.e., ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}$) and solve for ${\widehat{r}}_{\mathrm{06}}$:

$$\begin{array}{}\text{(10)}& {\widehat{r}}_{\mathrm{06}}={r}_{\mathrm{HV}}\cdot {\displaystyle \frac{{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}}{{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}}}.\end{array}$$

Similarly, higher-resolution SWIR reflectances ${\widehat{r}}_{\mathrm{16}}$ can be derived from

$$\begin{array}{}\text{(11)}& {\widehat{r}}_{\mathrm{16}}={r}_{\mathrm{HV}}\cdot {\displaystyle \frac{{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}}{{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}}}.\end{array}$$

As before, the relationship implies that the ratio of VNIR
and SWIR reflectances remains constant for different scales. This
assumption has been shown to be reasonable, at least for optically thin (i.e., *τ*≤10) liquid water
clouds over the ocean (Werner et al., 2018b).

A third method to derive high-resolution cloud property retrievals
for SEVIRI utilizes an iterative approach to determine *δ**r*_{06} and *δ**r*_{16} independently, based on the
shape of the LUT, while constraining the observed *r*_{eff} to
that of the baseline approach (i.e., simple trigonometric interpolation, which yields reflectances ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}$ and
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$ that only resolve the large-scale variability). While the previous approaches can be implemented as a
preprocessor outside the actual retrieval, this method requires
access to the LUT and has thus been implemented through modifications
of the CPP retrieval algorithm.

Again, a simple linear relationship between *δ**r*_{HV},
*δ**r*_{06} and *δ**r*_{08} based on
Eq. (2) is assumed:

$$\begin{array}{}\text{(12)}& \mathit{\delta}{r}_{\mathrm{HV}}=a\cdot \mathit{\delta}{r}_{\mathrm{06}}+b\cdot \mathit{\delta}{r}_{\mathrm{08}},\end{array}$$

where the fit coefficients *a* and *b* are determined from
the same techniques as described in Sect. 4.1. The variation *δ**r*_{HV} of the HRV channel is obtained from the observations
following Eq. (2), while *δ**r*_{08} is
calculated as the difference between *r*_{08} from high- and
low-resolution optical thickness *τ* based on the functional relation ℱ of the reflectances and cloud properties stored in the LUT (which motivates the name of this method). Therefore, *δ**r*_{06} can be derived from

$$\begin{array}{}\text{(13)}& \begin{array}{rl}\mathit{\delta}{r}_{\mathrm{06}}& ={\displaystyle \frac{\mathrm{1}}{a}}\cdot \left(\mathit{\delta}{r}_{\mathrm{HV}}-b\cdot \mathit{\delta}{r}_{\mathrm{08}}\right),\\ {\widehat{r}}_{\mathrm{06}}& ={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}+\mathit{\delta}{r}_{\mathrm{06}},\\ \mathit{\delta}{r}_{\mathrm{08}}& ={\mathcal{F}}_{\mathrm{08}}\left(\widehat{\mathit{\tau}},{\widehat{r}}_{\mathrm{eff}}\right)-{\mathcal{F}}_{\mathrm{08}}\left(\stackrel{\mathrm{\u0303}}{\mathit{\tau}},{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}\right).\end{array}\end{array}$$

Note that the addition of *δ**r*_{08} in the calculation
of *δ**r*_{06} helps to account for the noticeable
increase in surface albedo of vegetation-like surfaces at *λ*>700 nm (i.e., the vegetational step). This should improve the estimation of *δ**r*_{06} for thin clouds (i.e., *τ*<10) and cloud-edge pixels. For the SWIR reflectance,
instead of relying on the imperfect linear model in
Eq. (6) or assumptions about the inhomogeneity
index *H*_{σ,16}, the adjustment *δ**r*_{16} is
determined iteratively to conserve the coarse-resolution, pixel-level
(i.e., LRES scale of channels 1–3) value of the effective droplet
radius. To reduce some of the associated uncertainties, the effective droplet radius based on the reflectances from triangular interpolation can be used instead of the LRES result. If $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ are the cloud properties based on trigonometric interpolation, and $\widehat{\mathit{\tau}}$ and
${\widehat{r}}_{\mathrm{eff}}$ are the higher-resolution retrievals, which
are derived from an inversion of the functional relationship
(ℱ) between the high-resolution reflectances
${\widehat{r}}_{\mathrm{06}}$ and ${\widehat{r}}_{\mathrm{16}}$ following

$$\begin{array}{}\text{(14)}& \left(\widehat{\mathit{\tau}},{\widehat{r}}_{\mathrm{eff}}\right)={\mathcal{F}}^{-\mathrm{1}}\left({\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}+\mathit{\delta}{r}_{\mathrm{06}},{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}+\mathit{\delta}{r}_{\mathrm{16}}\right),\end{array}$$

then *δ**r*_{16} can be determined as

$$\begin{array}{}\text{(15)}& \mathit{\delta}{r}_{\mathrm{16}}={\mathcal{F}}_{\mathrm{16}}\left(\widehat{\mathit{\tau}},{\widehat{r}}_{\mathrm{eff}}={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}\right)-{\mathcal{F}}_{\mathrm{16}}\left(\stackrel{\mathrm{\u0303}}{\mathit{\tau}},{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}\right).\end{array}$$

This implies that a positive or negative *δ**r*_{06} is connected to a positive or negative
*δ**r*_{16} using the LUT to adjust the SWIR subpixel reflectance variations in such a way as to be representative of the respective
standard-resolution ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$. As a result, we do not expect
any improvement for the *r*_{eff} retrieval during the
transition to smaller scales. Instead, we try to find a physically
reasonable constraint for *δ**r*_{16} to achieve a reliable
retrieval of the higher-resolution $\widehat{\mathit{\tau}}$, while retaining the
accuracy of the standard-resolution retrieval of
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$.

The LUT approach is illustrated in Fig. 4a, where an example SEVIRI liquid-phase LUT for a
specific solar zenith angle (${\mathit{\theta}}_{\mathrm{0}}=\mathrm{40}{}^{\circ}$), sensor zenith
angle ($\mathit{\theta}=\mathrm{20}{}^{\circ}$), and relative azimuth angle ($\mathit{\phi}=\mathrm{60}{}^{\circ}$) is shown. Vertical dashed lines and values below the grid
denote fixed $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$, while the horizontal dashed lines and values
to the right of the grid denote fixed ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ in units of
micrometers. The green dot highlighted by the capital letter A
represents an example SEVIRI reflectance pair of approximately
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}=\mathrm{0.33}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}=\mathrm{0.34}$,
which maps to $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}=\mathrm{8}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}=\mathrm{12}\phantom{\rule{0.125em}{0ex}}\mathrm{\mu}\mathrm{m}$ (i.e., the retrieval result for the
high-resolution reflectances from trigonometric interpolation). The
red line highlights the ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}=\mathrm{12}\phantom{\rule{0.125em}{0ex}}\mathrm{\mu}\mathrm{m}$
isoline. The two horizontal blue arrows indicate a positive (*δ**r*_{06,1}) and negative (*δ**r*_{06,2}) adjustment
to ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{06}}$ based on
Eq. (13). Without an adjustment to
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$, these newly derived higher-resolution
${\widehat{r}}_{\mathrm{06}}$ values map to significantly larger and lower effective
droplet radii of about ${\widehat{r}}_{\mathrm{eff}}=\mathrm{29}$ and
${\widehat{r}}_{\mathrm{eff}}=\mathrm{5}\phantom{\rule{0.125em}{0ex}}\mathrm{\mu}\mathrm{m}$, respectively. The
adjustments *δ**r*_{16,1} and *δ**r*_{16,2}
simply assure that the prior effective radius retrieval is preserved
(i.e., ${\widehat{r}}_{\mathrm{eff}}={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$). Due to the curvature of the isolines of fixed ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ given by
the LUT, small deviations of the coarse-resolution average from
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$ can still occur.

Note that the LUT approach requires a prior cloud phase retrieval (either from the lower-resolution or interpolated reflectances) to determine the correct LUT for either liquid water or ice.

In order to improve the estimation of *δ**r*_{16} in the
LUT approach, two modifications to the previous assumption
are introduced in this section. The first one aims to provide a more
realistic estimate of ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ compared to the
coarser LRES result, which subsequently is used to
determine *δ**r*_{16}. The value of
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ is derived from adiabatic theory, which
provides a physically sound relationship between the derived
high-resolution cloud variables:

$$\begin{array}{}\text{(16)}& {\widehat{r}}_{\mathrm{eff}}={\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}\phantom{\rule{0.125em}{0ex}}{\left({\displaystyle \frac{\widehat{\mathit{\tau}}}{\stackrel{\mathrm{\u0303}}{\mathit{\tau}}}}\right)}^{a}.\end{array}$$

Based on observations, the study by Szczodrak et al. (2001) confirmed
the value of *a*≈0.2 predicted by theory for marine stratocumulus,
so this is the value also adopted here. This approach is
illustrated in Fig. 4b, where the
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ retrieval based on the interpolated
reflectances at point A is indicated by the red *r*_{eff} isoline. During the first iteration step *δ**r*_{06} is derived from Eq. (13) and
*δ**r*_{16}=0, which maps to ${\widehat{\mathit{\tau}}}^{\mathrm{1}}$ in the LUT
(the exponent 1 indicates the first iteration step). This value is
highlighted by the vertical blue line. Based on
Eq. (16) the corresponding adiabatic
${\widehat{r}}_{\mathrm{eff}}^{\mathrm{1}}$ is calculated (highlighted by the horizontal
blue line). This value determines the adjustment *δ**r*_{16}. Note that the resulting reflectances at point B do
not exactly map to ${\stackrel{\mathrm{\u0303}}{\mathit{\tau}}}^{\mathrm{1}}$ after the first iteration. As a
result, multiple iterations are necessary to derive the final cloud
properties. It has however been relatively simple to merge this
iteration into the iterative retrieval loop of the CPP retrieval.

A second approach to improve upon the LUT approach again
utilizes the shape of the LUT to derive a local slope $S=\partial {r}_{\mathrm{16}}/\partial {r}_{\mathrm{06}}$ from the simulated LUT
reflectances. The value of *S* is calculated at the position denoted
by $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$. In the iterative CPP
retrieval, this requires that both low- and high-resolution cloud
properties are estimated during each iteration until convergence of
both properties is achieved. This approach is illustrated in Fig. 4c. Again, the initial ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$
retrieval based on the interpolated reflectances at point A1 is
indicated by the red ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ isoline. The slope
*S*_{A1} at this position in the LUT is highlighted by the
solid blue line. Based on the derived slope and
*δ**r*_{06} from Eq. (13) the
corresponding *δ**r*_{16} can be calculated for each
iteration step. Two additional examples for initial starting points
(A2 and A3) and the respective slopes (*S*_{A2} and
*S*_{A3}) are also shown. These examples indicate the change in slope for different parts of the LUT. For small $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$, the slope *S*_{A3} become steeper, which leads to a larger adjustment *δ**r*_{16}. Meanwhile, for large $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}>\mathrm{30}$ (for this specific viewing geometry and LUT) the $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ isolines are nearly orthogonal and both the respective slope *S*_{A2} and *δ**r*_{16} are close to 0.

Both approaches introduced in this section have advantages and
disadvantages but promise to improve on the standard LUT
approach. While physically sound, adiabatic assumptions might not
always be appropriate, especially for highly convective clouds or in
the presence of drizzle. Meanwhile, large *δ**r*_{06} adjustments might map to a point in the LUT where the derived
local slopes at the position of ${\stackrel{\mathrm{\u0303}}{\mathit{\tau}}}^{\mathrm{i}}$ and
${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}^{\mathrm{i}}$ might not be representative
anymore.

5 Example retrievals

Back to toptop
An example of a standard SEVIRI red, green, and blue (RGB) composite and the respective cloud property
retrievals, utilizing the native *r*_{06}
and *r*_{16}, are shown in Fig. 5a–c. In comparison, the retrieval
results using the downscaled ${\widehat{r}}_{\mathrm{06}}$ and
${\widehat{r}}_{\mathrm{16}}$ from the adjusted lookup table
approach, using the LUT slope adjustment, are presented in
Fig. 5d–f for the same cloud
field. The example is a $\approx \mathrm{100}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{100}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$ subscene of
SEVIRI observations of an altocumulus field, which was acquired on 9 June 2013 at 10:55 UTC over ocean within the Germany domain. The three illustrated parameters are an RGB
composite image of SEVIRI channel 3, 2, and 1 reflectances in panels a
and c; the cloud optical thickness *τ* and $\widehat{\mathit{\tau}}$ in
panels b and e; and the effective droplet radius
*r*_{eff} and ${\widehat{r}}_{\mathrm{eff}}$ in panels c
and f. For the cloud variables only liquid-phase pixels are shown. An increase in contrast and resolved cloud structures is
visible in the higher-resolution RGB composite. Regarding the
retrieved cloud properties, the fields of lower-resolution
*τ* and *r*_{eff} are a lot smoother, and
the results exhibit a lower dynamical range than their higher-resolution
counterparts. One obvious example is the bright cloudy part along
54.6^{∘} N, where *τ*>45 are observed. Moreover, the
region of low *r*_{eff} in the northeastern corner of the
scene exhibits more nuanced values in the higher-resolution data
set.

6 Evaluation of downscaling techniques with MODIS data

Back to toptop
This section presents an evaluation of the different downscaling
techniques, which are introduced in Sect. 4, by
means of MODIS observations. MODIS provides reflectances at a horizontal
resolution of $\approx \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$. These observations are
remapped to the higher-resolution grid of the SEVIRI
*r*_{HV}-band samples, thus simulating a hypothetical SEVIRI-like geostationary instrument, where all channels are provided at the HRES scale. This provides the means to derive
reference retrievals of *τ* and *r*_{eff}. Note that even
though these reference retrievals are performed at a higher resolution the
“$\widehat{\phantom{\rule{0.25em}{0ex}}}$” notation is omitted, because these cloud products are
derived from actual observations and are not the estimates
obtained from the various downscaling techniques.

Remapping MODIS reflectances to SEVIRI's LRES grid (i.e., the native resolution of channels 1–3) subsequently provides the means to apply the various
downscaling schemes, as well as the simple triangular interpolation
approach, in order to compare the retrieved cloud products (i.e.,
$\widehat{\mathit{\tau}}$ and ${\widehat{r}}_{\mathrm{eff}}$, as well as
$\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$ and ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$) to the reference
results. Naturally, the ideal downscaling approach would yield results that closely resemble the MODIS-provided HRES observations. Furthermore, the ideal downscaling approach would also represent an improvement upon the simple interpolation technique. The reader is reminded that the latter data are still available at a higher resolution
than the native LRES grid of the SEVIRI
*r*_{06}, *r*_{08}, and *r*_{16} channels but no
longer contain any information about the high-frequency reflectance variability. As the simplest approach to derive higher-resolution cloud products, these results are called the
baseline results.

In addition, a comparison can be made to those cloud variables, which would be obtained from reflectances at SEVIRI's native spatial resolution by setting each 3×3 HRES pixel block to the LRES value.

Figure 6 shows RGB composites of the four example scenes, which comprise the data set for the evaluation of the different downscaling techniques. The scenes are increasingly more heterogeneous, starting with a rather homogeneous altocumulus field in Fig. 6a, two more heterogeneous broken altocumulus examples in Fig. 6b–c, and finally a broken cumulus field in Fig. 6d.

Meanwhile, Table 1 summarizes the different retrieval experiments that form the comparison in this section. For the sake of completeness, the reference data (i.e., the results from the MODIS reflectances, which are remapped to SEVIRI's HRES grid) are also included. Retrievals based on remapped MODIS data to SEVIRI's native 3 km scale are reproduced to each of the 3×3 subpixels to match the horizontal resolution of the reference results. Meanwhile, the cloud products derived from triangular interpolation of the remapped LRES–MODIS samples are referred to as the baseline data set, as this is the easiest approach and any reliable downscaling technique needs to add an improvement on those results. Experiment 1 denotes the statistical downscaling approach from Sect. 4.1, while retrievals based on the constant reflectance ratio approach and the adjusted LUT approach with LUT slope adjustment are indicated as experiments 2 and 3, respectively. Note that we also performed analysis for the standard LUT approach, as well as the adjusted LUT approach with adiabatic adjustment. However, we will only briefly summarize the results of these downscaling schemes where necessary.

First, the collocation and remapping procedure for the native
MODIS reflectances is briefly described. A comparison between the
retrieved cloud products from the LRES resolution–reflectances and those from triangular interpolation, as well as the
different downscaling procedures, and the reference results follows in
Sect. 6.2. These retrievals can be used
to derive estimates of the liquid water content (*W*_{L}, ${\stackrel{\mathrm{\u0303}}{W}}_{\mathrm{L}}$,
and ${\widehat{W}}_{\mathrm{L}}$) and the droplet number concentration (*N*_{D},
${\stackrel{\mathrm{\u0303}}{N}}_{\mathrm{D}}$, and ${\widehat{N}}_{\mathrm{D}}$), which are evaluated in Sect. 6.3.

To obtain a reliable higher-resolution reference data set, MODIS level
1b swath observations (MOD021km) have been projected to the grid of SEVIRI's *r*_{HV} samples, which corresponds to the
geostationary satellite projection at the HRES scale. Initially, the native HRV grid is
oversampled by a factor of 3 in each dimension (i.e., the target grid has a ≈333 m resolution), and nearest-neighbor interpolation
is used for the projection. This oversampled field is subsequently
smoothed with the modulation transfer function of the HRV channel as
given by EUMETSAT (2006), to remove high-frequency variability not resolved by the sensor and, in particular, the artifacts introduced by the
nearest-neighbor interpolation technique. Finally, this field is downsampled, such that only each central pixel of a 3×3 block (each pixel with a horizontal resolution of 333 m) is retained to represent the HRES value.

To perform the subsequent downscaling experiments, a second set of level 1b radiances are generated, where the spatial variability is reduced to match that of the LRES channels of Meteosat SEVIRI. This step again involves the smoothing of the respective reflectance field with the channel-specific modulation transfer function of the lower-resolution SEVIRI channels (EUMETSAT, 2006). This data set represents hypothetical SEVIRI-like observations at the native LRES.

In addition, a band-pass filter has been constructed from the difference between the modulation transfer functions of the HRV and the 0.6 and 0.8 µm channels (weighted by the coefficients of a linear model; see Deneke and Roebeling, 2010). This filter is used to extract the high-frequency signal of the HRV channel.

It should be noted that retrievals based upon these radiances will be different than those based upon the original MODIS C6 radiances or from an absolutely accurate representation of the (hypothetical) truly observed, high-resolution SEVIRI samples. For one, it uses the linear model of Cros et al. (2006) and Deneke and Roebeling (2010) as a proxy for the HRV channel, thereby excluding a potentially significant source of uncertainty. Moreover, MODIS acquires these reflectances under different viewing geometries (note that the true viewing angles are used in the CPP retrieval, so within the limits of plane-parallel radiative transfer, this effect is accounted for), and the spectral characteristics of the MODIS and SEVIRI channels are not entirely comparable. However, the goal of this study is to provide a consistent reference data set for a comparison of different retrieval data sets, which are derived from a single retrieval algorithm core. The actual absolute values of the retrieved cloud products are not important here.

Figure 7a shows a comparison of *τ*
at the native LRES (replicated onto each subpixel) and the reference *τ* at the HRES scale for the example
cloud field in scene 2, which is shown as an RGB composite image in Fig. 6b. A total of over 13 000 cloudy pixels
(liquid phase) are located in this scene. While for small reference
*τ*<20 there is a reasonable agreement between the two data sets,
there is increased scatter around the 1:1 line (indicated by the dashed gray line) for larger values of cloud optical thickness. For
reference *τ*>40, a substantial underestimation of the LRES *τ* is observed, which yields a sizable contribution to the
nRD of 15.8 *%*. Figure 7b–c show
similar scatter plots of *τ* and $\widehat{\mathit{\tau}}$ from both
experiment 2 (constant reflectance ratio approach) and 3 (adjusted LUT approach with LUT slope adjustment), respectively. It is obvious that the results
from these two downscaling techniques improve the agreement with the
reference retrievals significantly. The explained variance (*R*^{2}, which equals the square of Pearson's product-moment
correlation coefficient *R*) between the data
sets is increased, and the nRD is strongly reduced to values of
1.182 *%* (experiment 2) and 1.589 *%* (experiment 3).

A similar comparison between the reference *r*_{eff} at the HRES scale and
*r*_{eff} at native LRES, as well as
${\widehat{r}}_{\mathrm{eff}}$ from the same downscaling experiments, is
presented in Fig. 7d–f. Here, the
native-resolution results show a much better agreement with the
reference retrievals, and, compared to the cloud optical thickness, the
nRD=5.505 *%* is much lower. While experiment 2 exhibits a good
agreement between reference *τ* and $\widehat{\mathit{\tau}}$, the comparison
of retrieved ${\widehat{r}}_{\mathrm{eff}}$ to the reference results is
less favorable. Both the reduced explained variance (*R*^{2}=0.889 versus
*R*^{2}=0.929) and the increased scatter around the 1:1 line (nRD
=6.630 *%*) indicate that the results from experiment 2 are less
reliable than the ones performed at the native LRES. Thus, the elaborate
downscaling procedure actually reduces the accuracy of the ${\widehat{r}}_{\mathrm{eff}}$ retrieval.
In contrast, the retrieved ${\widehat{r}}_{\mathrm{eff}}$ values from experiment
3 improve upon the native-resolution results, with slightly better
values of *R*^{2}=0.953 and nRD =4.402 *%*.

Statistics of the comparison between the reference and native LRES, baseline, and experimental retrievals are presented in Fig. 8a–d for example scenes
1–4, respectively. The parameters which are used to quantify the
individual comparisons are the median of the relative difference (abbreviated
with p50) to indicate the average deviation from the reference
results, the interquartile range (IQR; defined as the relative
difference between the 75th and 25th
percentile of the deviation to the reference retrievals) to indicate
the spread between the different data sets, the nRD as a second
measure of the spread of data points, and the explained variance
*R*^{2} between the different retrievals and
the reference. Values with a green and red background highlight the
respective experiment with the best and worst comparison for the
specific parameter. Yellow backgrounds, meanwhile, indicate all other
experiments in between the two extreme results. The first noteworthy
observation concerns the native and baseline retrievals of
*τ*, which universally exhibit the largest median
deviations and spread to the reference results, as well as the lowest
*R*^{2}. Still, the difference between native and baseline results
indicates that the trigonometric interpolation to the HRES grid has
significantly improved the comparison.

In contrast, each retrieval of $\widehat{\mathit{\tau}}$ that accounts for small-scale reflectance variability yields significant improvements, regardless of the approach. This is especially obvious in the parameters that characterize the spread in the deviations, i.e., IQR and nRD, which are between 2–9 and 2–10 smaller for the various experiments and example scenes, respectively. Experiments 2 and 3 seem to achieve the best agreement with the reference retrievals.

Regarding the effective droplet radius, the agreement between the native LRES and (i) baseline retrievals and (ii) the
reference results is significantly better. It is worth pointing out that, similar to the optical thickness comparison,
the ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ retrieval based on interpolating reflectances to the HRES
grid performs better than the native-resolution *r*_{eff} retrieval for all scenes.
The most reliable
downscaling approach seems to be experiment 3, which performs
noticeably better than experiments 1 (note the increased nRD and
reduced *R*^{2} for scene 3) and 2 (increased spread and overall issues for the
heterogeneous cloud field in scene 4). This indicates that the linear
model in Eq. (6) or assumptions about a constant ratio of VNIR and
SWIR reflectances are not adequate to estimate higher-resolution
${\widehat{r}}_{\mathrm{16}}$, at least not for certain cloud conditions. In
the case of experiment 2 this is understandable, because the technique
was developed for partially cloudy pixels (Werner et al., 2018b). These observations are characterized by a low cloud optical thickness, where the relationship between VNIR and SWIR reflectance can reliably be considered to be linear (see example LUTs in Fig. 4).

There is a notably better performance of experiment
3, the adjusted LUT approach with LUT slope adjustment, compared to the standard LUT approach highlighted in Sect. 4.3.
Of particular note is the ${\widehat{r}}_{\mathrm{eff}}$ retrieval based on the standard LUT scheme, which compares significantly worse to the reference results (*R*^{2} of 0.890, 0.648, 0.751, and 0.581 for cloud scenes 1–4, respectively).
This is somewhat surprising, because the specified goal of the standard LUT approach is to maintain the accuracy of
the baseline ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ retrieval, which has not been
fully reached. We believe that this might be caused by the sensitivity
of the cloud property retrieval to small reflectance perturbations, in
particular for broken clouds. It is also an indication that assuming constant subpixel *r*_{eff} values within each LRES pixel is not sufficient. We plan to investigate this effect
further in future studies. However, the second adjusted LUT approach, which determines SWIR reflectance adjustments based on adiabatic theory, performs even worse
(*R*^{2} of 0.846, 0.579, 0.741, and 0.519 for cloud scenes 1–4, respectively). This suggests that the observed cloud fields do not follow adiabatic theory and the method is not adequate to estimate higher-resolution
${\widehat{r}}_{\mathrm{16}}$.

Retrievals of *τ* and *r*_{eff} (regardless of the
resolution they are derived at) provide the means to infer other
commonly used cloud variables. The *W*_{L}, which describes the amount
of liquid water in a remotely sensed cloud column, can be derived as
the product of retrieved cloud products (Brenguier et al., 2000; Miller et al., 2016):

$$\begin{array}{}\text{(17)}& {W}_{\mathrm{L}}\approx {\displaystyle \frac{\mathrm{2}}{\mathrm{3}}}\cdot {\mathit{\rho}}_{\mathrm{L}}\cdot \mathit{\tau}\cdot {r}_{\mathrm{eff}}.\end{array}$$

Here, *ρ*_{L} is the bulk density of liquid water.
Assuming adiabatic clouds, where the vertical structure of effective droplet radius follows the adiabatic growth model, introduces an extra factor of 5∕6 and the coefficient 2∕3 changes to $\mathrm{5}/\mathrm{6}\cdot \mathrm{2}/\mathrm{3}=\mathrm{5}/\mathrm{9}$.
Meanwhile, *N*_{D} describes the
number of liquid cloud droplets in a cubic centimeter of cloudy
air. Calculating *N*_{D} from remote sensing products requires a number of
assumptions, e.g., about the vertical cloud structure and shape of the droplet number size distribution, which are summarized and discussed in
Brenguier et al. (2000), Schüller et al. (2005), Bennartz (2007),
and Grosvenor et al. (2018). A simplified form of the resulting equation for *N*_{D}
is

$$\begin{array}{}\text{(18)}& {N}_{\mathrm{D}}\approx \mathit{\alpha}\cdot {\mathit{\tau}}^{\mathrm{0.5}}\cdot {r}_{\mathrm{eff}}^{-\mathrm{2.5}},\end{array}$$

with $\mathit{\alpha}=\mathrm{1.37}\cdot {\mathrm{10}}^{-\mathrm{5}}$ (see Quaas et al., 2006). Note that Eqs. (17)–(18) can yield both baseline and downscaled results (i.e., ${\stackrel{\mathrm{\u0303}}{W}}_{\mathrm{L}}$ and ${\stackrel{\mathrm{\u0303}}{N}}_{\mathrm{D}}$, as well as ${\widehat{W}}_{\mathrm{L}}$ and ${\widehat{N}}_{\mathrm{D}}$) when they are derived from the respective cloud optical thicknesses and effective droplet radii.

Similar to the comparison in Sect. 6.2,
scatterplots of the reference *W*_{L}, the native LRES *W*_{L}, and the results from the downscaling experiments 2 and 3
(${\widehat{W}}_{\mathrm{L}}$) are shown in Fig. 9a–c, respectively. As before,
data are provided by example scene 2 sampled on 9 June 2013 at 10:55 UTC. Compared to the native LRES results, a noticeable improvement in the
correlation and nRD is achieved by utilizing the two downscaling
experiments. Not only are retrieved ${\widehat{W}}_{\mathrm{L}}$ values closer to the 1:1 line, but the
significant underestimation of the LRES *W*_{L} values for larger reference
results is mitigated. Especially for experiment 3, the spread is less
than one-third of the value of the LRES results (4.857 *%* versus
15.234 *%*). Regarding the comparison between reference and native *N*_{D}, as well as ${\widehat{N}}_{\mathrm{D}}$, downscaling experiment 2 yields less favorable results. There is a
slight decrease (increase) in *R*^{2} (nRD). This is caused by the large IQR and nRD of the
deviations in the retrieved ${\widehat{r}}_{\mathrm{eff}}$, shown in
Fig. 7e, which are amplified due to
the associated power of 2.5 in Eq. (18). However, the derived values from experiment 3 show a significantly better agreement with
the reference *N*_{D}.

Values of p50, IQR, nRD, and *R*^{2} for the *W*_{L} and *N*_{D} comparison
from the four example scenes are illustrated in Fig. 10a–d. Due to the
large deviations between the native *τ* and the reference retrievals,
*W*_{L} values for the LRES results almost universally show the
largest deviations to the reference values and thus the largest IQR
and nRD, as well as the lowest explained variance. The exception is
the heterogeneous cloud field in the fourth example scene, where the
large deviations between ${\widehat{r}}_{\mathrm{eff}}$ from experiment 2
and the reference retrievals yield the worst comparison for the
respective ${\widehat{W}}_{\mathrm{L}}$. The estimates based on the adjusted
lookup table approach using the LUT slope adjustment (i.e., experiment 3) almost
universally exhibit the best agreement with the reference results of *W*_{L}.

Overall, 27 of the 32 comparisons (four cloud scenes, two cloud variables, and four statistical measures) exhibit the best performance for experiment 3. For the example scenes considered in this analysis, it is obvious that the adjusted lookup table approach with LUT slope adjustment is preferable to the other downscaling techniques and yields more reliable high-resolution cloud variables than the standard LRES results.

As before, we also tested the standard LUT approach highlighted in Sect. 4.3, as well as the second adjusted LUT approach, which determines SWIR reflectance adjustments based on adiabatic theory.
Due to the poor performance of the ${\widehat{r}}_{\mathrm{eff}}$ retrieval, the ${\widehat{N}}_{\mathrm{D}}$ results based on adiabatic assumptions show a similarly poor agreement with the reference results. Meanwhile, the cloud variables based on the standard LUT approach never show the best or worst performance but are almost universally worse than the adjusted
lookup table approach with LUT slope adjustment. This again illustrates that assumptions of adiabatic clouds and constant subpixel *r*_{eff} values within each LRES pixel are not suitable for the cloud scenes analyzed in this study.

7 Full downscaling versus VNIR only

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Apart from the constant reflectance ratio approach, the downscaling of
*r*_{06} for each of the techniques presented in Sect. 4 uses the well-established relationship between
*r*_{06}, *r*_{08}, and the averaged $\u2329{\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{HV}}\u232a$ (see Fig. 3 and the discussion
in Deneke and Roebeling, 2010). In contrast, downscaling of *r*_{16}
is based on different assumptions about the microphysical structure
and cloud heterogeneity, which induces a level of uncertainty in the
subsequent cloud property retrievals. To test whether assumptions
about *r*_{16} actually improve the retrieval of $\widehat{\mathit{\tau}}$
and ${\widehat{r}}_{\mathrm{eff}}$, this section presents retrievals that include the results from the adjusted
lookup table approach with LUT slope adjustment (i.e., experiment 3) for
${\widehat{r}}_{\mathrm{06}}$ but do not include the respective downscaling
schemes for ${\widehat{r}}_{\mathrm{16}}$. Instead, the SWIR reflectance for
each sample is provided by the ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{16}}$ value derived
from trigonometric interpolation.

Figure 11a shows PDFs of the
relative difference (Δ*τ*) between $\stackrel{\mathrm{\u0303}}{\mathit{\tau}}$ from the
baseline test (black), as well as $\widehat{\mathit{\tau}}$ retrieved from
the partial downscaling approach of only ${\widehat{r}}_{\mathrm{06}}$ (blue) and the full downscaling approach (red), and the reference results (i.e.,
distributions of the difference between the data sets, normalized by
the reference *τ*). Data are from example scene 2, shown in Fig. 6b, sampled on 9 June 2013 at 10:55 UTC. The
largest differences to the reference retrievals are observed for the
baseline results, which only account for the large-scale reflectance
variability of the cloud scene. Here, relative differences cover the
range of $-\mathrm{20.44}\phantom{\rule{0.125em}{0ex}}\mathit{\%}<\mathrm{\Delta}\mathit{\tau}<\mathrm{28.22}\phantom{\rule{0.125em}{0ex}}\mathit{\%}$ (these values indicate the
1st and 99th percentile of Δ*τ*,
respectively). The distributions for the full downscaling experiment 3 are noticeably
thinner, and these observed ranges are reduced significantly to
$-\mathrm{2.33}\phantom{\rule{0.125em}{0ex}}\mathit{\%}<\mathrm{\Delta}\mathit{\tau}<\mathrm{3.14}\phantom{\rule{0.125em}{0ex}}\mathit{\%}$. The differences Δ*τ* for
the VNIR-only approach look closer to the one from the full downscaling
experiment. However, the maximum of the distribution around Δ*τ*≈0 is lower and the
1st percentile is actually higher than that from the baseline
retrievals. Clearly, the downscaling of both VNIR and SWIR
reflectances is preferable for the retrieval of $\widehat{\mathit{\tau}}$. For
the effective droplet radius, the experiment comparison looks
significantly different. Both relative differences Δ*r*_{eff} based on the baseline and full downscaling experiment results
exhibit a similar behavior, and the full downscaling approach only
yields small improvements on the retrievals from trigonometric
interpolation. Conversely, Δ*r*_{eff} from partial downscaling yields a noticeably larger spread and the retrievals become less
reliable.

Regarding Δ*W*_{L} and Δ*N*_{D}, the results using the complete
downscaling approach yield the narrowest distributions, with
significantly smaller minimum and maximum deviations (up to a factor
of 5.6) compared to the VNIR-only technique. Compared to
the baseline results the reliability of derived liquid water path is also improved, even though just the VNIR reflectance is downscaled.

A summary of the performance of the partial and full downscaling approach for experiments 1–3 for all four example cloud scenes is given in Table 2. Here, the 1st, 50th, and 99th percentiles of the relative differences between $\widehat{\mathit{\tau}}$ and ${\widehat{r}}_{\mathrm{eff}}$ and the reference retrievals are listed. An almost universal reduction in the biases is observed when both VNIR and SWIR reflectances are downscaled. These results provide strong evidence that simultaneous downscaling of the SWIR reflectances is essential for providing reliable higher-resolution retrievals of $\widehat{\mathit{\tau}}$ and $\widehat{{r}_{\mathrm{eff}}}$, as well as the subsequently calculated ${\widehat{W}}_{\mathrm{L}}$ and ${\widehat{N}}_{\mathrm{D}}$. This confirms the findings in Werner et al. (2018b), who illustrated that SWIR reflectances differ significantly between the pixel level and subpixel scale and that reliable cloud property retrievals should avoid scale mismatches between the reflectances from the VNIR and SWIR channels.

This result is likely also relevant for retrieving cloud properties at
the highest-possible resolution from other multiresolution sensors such
as MODIS, VIIRS, and GOES-R: here, VNIR reflectances are generally
available at the highest spatial resolution, while SWIR reflectances have a 2–4-times-lower sampling resolution. Based on the previous results, smooth
interpolation of the SWIR reflectances to the VNIR resolution cannot
be recommended. Instead, downscaling approaches such as those
presented in Sect. 4 should be adopted to avoid
a scale mismatch in the spatial variability captured by the VNIR and
SWIR channels or, equivalently, a degraded accuracy of the
*r*_{eff} retrieval.

8 Conclusions

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In this work, several candidate approaches to downscale SEVIRI channel 1–3 reflectances are evaluated, which increases their spatial resolution from the native horizontal resolution (3 km×3 km at the subsatellite point) to the 3-times-higher spatial resolution of the narrowband HRV channel observations. The goal is to identify a reliable downscaling approach to provide the means to resolve higher-resolution, subpixel reflectance and cloud property variations, which are only resolved by reflectances from SEVIRI's coincident HRV channel. The higher-resolution reflectances are subsequently used to retrieve cloud optical thickness ($\widehat{\mathit{\tau}}$) and effective droplet radius (${\widehat{r}}_{\mathrm{eff}}$). These subsequently provide the means to derive estimates of the liquid water path (${\widehat{W}}_{\mathrm{L}}$) and droplet number concentration (${\widehat{N}}_{\mathrm{D}}$).

Three different methods are presented and evaluated: (i) a statistical downscaling approach using globally determined fit coefficients based on bivariate statistics; (ii) a local approach that assumes a constant heterogeneity index for different scales (i.e., the constant reflectance ratio approach); and (iii) an iterative approach utilizing both global statistics and the shape of the SEVIRI LUT (which consists of simulated SEVIRI reflectances for different viewing geometries and combinations of cloud properties), while assuming a constant subpixel ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$ (i.e., the LUT approach). For the latter technique, two modifications (by assuming adiabatic cloud conditions or by deriving local slopes within the LUT) are introduced, which avoid the constraint of a fixed ${\stackrel{\mathrm{\u0303}}{r}}_{\mathrm{eff}}$. The different downscaling approaches are evaluated using MODIS observations of four example cloud fields at a horizontal resolution of $\approx \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\times \mathrm{1}\phantom{\rule{0.125em}{0ex}}\mathrm{km}$ (i.e., comparable to SEVIRI's HRV channel), which are remapped onto the higher-resolution SEVIRI grid, followed by smoothing with the modulation transfer functions of SEVIRI.This approach has the benefit of providing a reference data set to which the results from the different downscaling techniques can be objectively compared.

The retrievals based on native-resolution reflectances (at a scale of ≈3 km) are characterized by significant deviations from the reference retrievals, especially for $\widehat{\mathit{\tau}}$ and ${\widehat{W}}_{\mathrm{L}}$. Here, random absolute deviations as large as ≈14 and ≈89 g m^{−2} are observed, respectively (determined from the 1st or 99th percentiles of the absolute deviations between native and reference results for each cloud scene). For ${\widehat{r}}_{\mathrm{eff}}$ and ${\widehat{N}}_{\mathrm{D}}$ deviations of up to ≈6 µm and $\approx \mathrm{177}\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{3}}$ exist, respectively.

Simply applying trigonometric interpolation of the reflectance to the
higher-resolution grid of the HRV channel (i.e., the baseline approach) provides a
significantly improved agreement with the reference data set for *τ* and *r*_{eff} (i.e., the actual higher-resolution retrievals) compared to SEVIRI's
native lower-resolution results. This improvement can be attributed to the use of higher-resolution reflectances, which resolve the large-scale variability of the scene. It is shown that either downscaling
approach, which applies estimates of the unresolved small-scale variability to the reflectance field, yields reliable retrievals of $\widehat{\mathit{\tau}}$ at the horizontal
resolution of the SEVIRI HRV channel. These results compare noticeably
better with the reference retrievals than the ones from the baseline
approach. The improved performance is illustrated by a lower median absolute bias and
spread (factor of 2–10), as well as a higher observed correlation
between the data sets. The reliability
of ${\widehat{r}}_{\mathrm{eff}}$ utilizing the LUT approach with
an adjustment based on the calculation of isoline slopes in the SEVIRI LUT is comparable
to the baseline results and improves upon the retrievals at the native
LRES. The performance of the other downscaling approaches depends on the observed cloud scene. For more heterogeneous cloud
fields the performance of the statistical downscaling
approach and
the constant reflectance ratio approach decreases noticeably.
The former technique relies on large-scale statistical relationships between the reflectances, which might vary with the size of the observed region, prevalence of different cloud types, and viewing geometry. The latter technique, meanwhile, was developed for optically thin clouds, where the relationship between VNIR and SWIR reflectance can be approximated by a linear function (Werner et al., 2018b).
Conversely, for more homogeneous
altocumulus fields the LUT approach with adiabatic adjustment seems inadequate and yields the worst comparison to the reference effective radius. The study by Miller et al. (2016), following similar studies, illustrated that drizzle and cloud top entrainment yield vertical cloud profiles closer to homogeneous assumptions and away from the adiabatic cloud model. Similar processes might affect the retrieval for the presented cloud scenes in this study.

Due to the fact that these variables are derived from retrieved $\widehat{\mathit{\tau}}$ and ${\widehat{r}}_{\mathrm{eff}}$, a similar behavior is observed for the derived ${\widehat{W}}_{\mathrm{L}}$ and ${\widehat{N}}_{\mathrm{D}}$. Again, the adjusted LUT approach in combination with the use of local slopes exhibits the best agreement with the reference results for 27 out of the 32 comparisons (i.e., four example scenes, two cloud variables, and four evaluation parameters). Based on these results, this method seems to be favorable compared to the other downscaling approaches. The results are preferable to those obtained from the standard-resolution SEVIRI narrowband reflectances and pave the way for future higher-resolution cloud products by the MSG-SEVIRI imager. Especially for $\widehat{\mathit{\tau}}$ and ${\widehat{W}}_{\mathrm{L}}$, these improvements are significant, as even the baseline results show deviations from the reference data set of up to ≈11 and $\approx \mathrm{70}\phantom{\rule{0.125em}{0ex}}\mathrm{g}\phantom{\rule{0.125em}{0ex}}{\mathrm{m}}^{-\mathrm{2}}$ for the observed example scenes.

Most of the presented downscaling techniques utilize a well-established relationship between the observed reflectance from SEVIRI channels 1 and 2, as well as the one from the broadband HRV channel. To test the validity of the different assumptions for the downscaling of the SWIR band reflectance, the reliability of VNIR-only downscaling approaches is compared to the corresponding full downscaling procedure. For the former, the higher-resolution SWIR observations are provided by the baseline technique. An almost universally improved reliability of the retrieved cloud products is observed when both VNIR and SWIR reflectances are downscaled. This illustrates that, in order to achieve reliable higher-resolution retrievals, all channels need to capture small-scale cloud heterogeneities at the same scale. These results confirm the findings of Werner et al. (2018b), who compared SWIR reflectances at different spatial scales and demonstrated the need for effective downscaling approaches to match the spatial scale of the VNIR reflectance. This also has implications for other multiresolution sensors, such as MODIS, VIIRS, and GOES-R ABI. To avoid a scale mismatch of resolved variability in the VNIR and SWIR channels, the higher-resolution observations can either be degraded to match the lower-resolution samples (which yields overall lower-resolution cloud property retrievals) or downscaling techniques can be applied to one or both channel reflectances, which yields matching scales and higher-resolution estimates of cloud properties. It is important to note that downscaling might result in increased retrieval uncertainties if the spatial resolution is below the radiative smoothing scale (≈200–400 m; see Davis et al., 1997).

Naturally, these results require more evaluation with a larger data set to validate the reliability of the approach under different observational geometries and cloud situations. If a similarly good agreement with a set of reference retrievals is found for a broad range of different test scenes, a significant step towards higher-resolution SEVIRI cloud observations is achieved. If our results are confirmed, such retrievals would represent a noticeable improvement upon SEVIRI's current standard-resolution retrievals. Meanwhile, more elaborate downscaling schemes could potentially improve upon the methods presented here. As an example, one possible improvement on the adjusted lookup table approach with adiabatic adjustment would be an explicit fit of the relationship in Eq. (16) from the native, lower-resolution variables. This might also reveal valuable insights into the validity of the adiabatic assumption commonly adopted in remote sensing (Merk et al., 2016). In addition, a comprehensive evaluation of the benefits of the higher-resolution SEVIRI cloud products for the subsequent estimation of solar surface irradiance is planned. In particular, a comparison of satellite retrievals based on Greuell et al. (2013) with observations of a dense network of pyranometers following the approach of Deneke et al. (2009) and Madhavan et al. (2017) is planned, which will enable detailed studies of the effects of spatial and temporal resolution of satellite observations.

This work clearly demonstrated that the adjusted LUT approach with LUT slope adjustment yields reliable higher-resolution cloud products. A follow-up study by Deneke et al. (2020) will provide a comprehensive description of the overall retrieval scheme for obtaining cloud properties and solar radiative fluxes from the Meteosat SEVIRI instrument at the spatial resolution of its HRV channel, which will be established based on the findings of this study. That companion paper also includes a statistical comparisons between the operational MODIS C6.1 and SEVIRI results, as well as the new high-resolution SEVIRI products. Moreover, some interesting use cases are demonstrated in that study, which can benefit from an increase in the spatial resolution of the derived SEVIRI cloud parameters. The companion paper also presents an important extension of this approach to the retrieval of solar surface irradiance, based on the schemes presented in Deneke et al. (2008) and Greuell et al. (2013). Satellite products with high temporal and spatial resolution are of particular interest for forecasting the production of solar power.

Code and data availability

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Code and data availability.

The MODIS and MSG radiance data used as input to the CPP retrieval, the Python code used for their generation, the retrieval output, and Python routines to generate the data analysis in the paper are publicly available through the ZENODO data repository https://doi.org/10.5281/zenodo.3632525 (Werner and Deneke, 2020). The retrieval output for other scenes is available from the authors on request. The CPP software is copyrighted by EUMETSAT and is not publicly available.

Author contributions

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Author contributions.

Both authors have shaped the concept of this study and in particular refined the considered downscaling approaches through extensive discussions. HD implemented the processing of the high-resolution processing scheme including the different downscaling approaches. FW carried out the analysis of the output and wrote the initial draft of the manuscript, which was subsequently refined by both authors.

Competing interests

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Competing interests.

The authors declare that they have no conflict of interest.

Acknowledgements

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Acknowledgements.

This study was carried out within the frame of the German collaborative project MetPVNet funded by the German Ministry of Commerce, grant number 0350009E. The use of MODIS data obtained from the Level-1 and Atmosphere Archive and Distribution System (LAADS) Distributed Active Archive Center (DAAC) and the use of SEVIRI data distributed by EUMETSAT and obtained from the TROPOS satellite archive are gratefully acknowledged. The lead author, Frank Werner, is now employed by the Jet Propulsion Laboratory, California Institute of Technology. This work was done as a private venture and not in the author's capacity as an employee of the Jet Propulsion Laboratory, California Institute of Technology. The authors thank Anja Hünerbein, Fabian Senf, Marion Schroedter-Homscheidt, and Michael J. Schwartz for comments on earlier drafts of this paper, which helped to improve the submitted version.

Financial support

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Financial support.

This research has been supported by the German Ministry of Commerce (grant no. 0350009E).

Review statement

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Review statement.

This paper was edited by Sebastian Schmidt and reviewed by two anonymous referees.

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Short summary

The reliability of remotely sensed cloud variables from space depends on the horizontal resolution of the instrument. This study presents and evaluates several candidate approaches for increasing the spatial resolution of observations from the Spinning Enhanced Visible and Infrared Imager (SEVIRI) from the native 3 km scale to a horizontal resolution of 1 km. It is shown that uncertainties in the derived cloud products can be significantly mitigated by applying an appropriate downscaling scheme.

The reliability of remotely sensed cloud variables from space depends on the horizontal...

Atmospheric Measurement Techniques

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