**Research article**
18 Dec 2018

**Research article** | 18 Dec 2018

# A physics-based approach to oversample multi-satellite, multispecies observations to a common grid

Kang Sun Lei Zhu Karen Cady-Pereira Christopher Chan Miller Kelly Chance Lieven Clarisse Pierre-François Coheur Gonzalo González Abad Guanyu Huang Xiong Liu Martin Van Damme Kai Yang and Mark Zondlo

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**Kang Sun et al.**Kang Sun Lei Zhu Karen Cady-Pereira Christopher Chan Miller Kelly Chance Lieven Clarisse Pierre-François Coheur Gonzalo González Abad Guanyu Huang Xiong Liu Martin Van Damme Kai Yang and Mark Zondlo

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^{1}Research and Education in Energy, Environment and Water Institute, University at Buffalo, Buffalo, NY, USA^{2}School of Engineering and Applied Sciences, Harvard University, Cambridge, MA, USA^{3}Atmospheric and Environmental Research, Lexington, MA, USA^{4}Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA^{5}Atmospheric Spectroscopy, Service de Chimie Quantique et Photophysique, Université libre de Bruxelles (ULB), Brussels, Belgium^{6}Department of Environmental and Health Sciences, Spelman College, Atlanta, GA, USA^{7}Department of Atmospheric and Oceanic Science, University of Maryland, College Park, MD, USA^{8}Department of Civil and Environmental Engineering, Princeton University, Princeton, NJ, USA

^{1}Research and Education in Energy, Environment and Water Institute, University at Buffalo, Buffalo, NY, USA^{2}School of Engineering and Applied Sciences, Harvard University, Cambridge, MA, USA^{3}Atmospheric and Environmental Research, Lexington, MA, USA^{4}Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA^{5}Atmospheric Spectroscopy, Service de Chimie Quantique et Photophysique, Université libre de Bruxelles (ULB), Brussels, Belgium^{6}Department of Environmental and Health Sciences, Spelman College, Atlanta, GA, USA^{7}Department of Atmospheric and Oceanic Science, University of Maryland, College Park, MD, USA^{8}Department of Civil and Environmental Engineering, Princeton University, Princeton, NJ, USA

**Correspondence**: Kang Sun (kangsun@buffalo.edu)

**Correspondence**: Kang Sun (kangsun@buffalo.edu)

Received: 28 Jul 2018 – Discussion started: 23 Aug 2018 – Revised: 03 Dec 2018 – Accepted: 04 Dec 2018 – Published: 18 Dec 2018

Satellite remote sensing of the Earth's atmospheric composition usually
samples irregularly in space and time, and many applications require
spatially and temporally averaging the satellite observations (level 2) to a
regular grid (level 3). When averaging level 2 data over a long period to a
target level 3 grid that is significantly finer than the sizes of level 2
pixels, this process is referred to as “oversampling”. An agile,
physics-based oversampling approach is developed to represent each satellite
observation as a sensitivity distribution on the ground, instead of a point
or a polygon as assumed in previous methods. This sensitivity distribution
can be determined by the spatial response function of each satellite sensor.
A generalized 2-D super Gaussian function is proposed to characterize the
spatial response functions of both imaging grating spectrometers (e.g., OMI,
OMPS, and TROPOMI) and scanning Fourier transform spectrometers (e.g., GOSAT,
IASI, and CrIS). Synthetic OMI and IASI observations were generated to
compare the errors due to simplifying satellite fields of view (FOVs) as
polygons (tessellation error) and the errors due to discretizing the smooth
spatial response function on a finite grid (discretization error). The
balance between these two error sources depends on the target grid size, the
ground size of the FOV, and the smoothness of spatial response functions.
Explicit consideration of the spatial response function is favorable for
fine-grid oversampling and smoother spatial response. For OMI, it is
beneficial to oversample using the spatial response functions for grids finer
than ∼16 km. The generalized 2-D super Gaussian function also enables
smoothing of the level 3 results by decreasing the shape-determining
exponents, which is useful for a high noise level or sparse satellite datasets. This
physical oversampling approach is especially advantageous during smaller
temporal windows and shows substantially improved visualization of trace gas
distribution and local gradients when applied to OMI NO_{2} products and IASI NH_{3} products. There is no appreciable difference in the computational time
when using the physical oversampling versus other oversampling methods.

Since the launch of the ESA Global Ozone Monitoring Experiment (GOME) in
1995, satellite observations have tremendously advanced our understanding of
the processes governing the atmospheric composition, greenhouse gas
emissions, and air
quality (Jacob et al., 2016; Martin, 2008; Streets et al., 2013). Global
distributions of atmospheric species that play critical roles in atmospheric
chemistry and air pollution, such as ozone (Bak et al., 2017),
NO_{2} (Krotkov et al., 2017), SO_{2} (Li et al., 2017a),
formaldehyde (González Abad et al., 2015), glyoxal (Chan Miller et al., 2014), and BrO (Suleiman et al., 2018), have been
retrieved from the backscattered solar UV–visible spectra observed by
generations of polar-orbiting satellite sensors, including
GOME (Burrows et al., 1999), SCIAMACHY (Bovensmann et al., 1999),
OMI (Levelt et al., 2018), GOME-2 (Munro et al., 2016),
OMPS (Rodriguez et al., 2003), and TROPOMI (Veefkind et al., 2012). A
constellation of geostationary satellites will provide hourly measurements of
these species over North America, Europe, and Asia in the near
future (Zoogman et al., 2017). Observations of the backscattered
shortwave infrared solar spectra also enable the retrieval of CO_{2}, CH_{4},
and/or CO from SCIAMACHY (Buchwitz et al., 2005),
GOSAT (Yoshida et al., 2011), OCO-2 (Eldering et al., 2017), and
TROPOMI (Borsdorff et al., 2018; Hu et al., 2018). Moreover, many atmospheric species have
strong spectroscopic signatures in the mid-infrared and can be retrieved from
the Earth's thermal emission spectra collected by satellite sensors such as
MOPITT (Drummond et al., 2010), AIRS (Aumann et al., 2003), TES (Bowman et al., 2006),
IASI (Clerbaux et al., 2009), and CrIS (Han et al., 2013). One species of
particular significance to tropospheric chemistry and air quality is
NH_{3} (Baek et al., 2004; Paulot and Jacob, 2014), which has been successfully
retrieved from TES (Shephard et al., 2011; Sun et al., 2015a),
AIRS (Warner et al., 2016),
IASI (Clarisse et al., 2010; Van Damme et al., 2017; Whitburn et al., 2016a), and
CrIS (Dammers et al., 2017; Shephard and Cady-Pereira, 2015).

The retrieval results from satellite sensors are usually total or partial (e.g., tropospheric or planetary boundary layer, PBL) column density at individual satellite pixels, i.e., the level 2 product. However, the pixel geometry may vary significantly even for the same sensor (see Fig. 1 for example), and data quality screening (by cloud coverage, solar zenith angle, surface albedo, thermal contrast, etc.) often leaves only small and patchy fractions of useful level 2 pixels for any given orbit. As such, the level 2 data over many orbits are often projected to a regular spatial grid to better represent the spatiotemporal variations of the target species through a gridding algorithm. These “level 3” products help to average out the observational noise that can be significant for individual level 2 retrieval and make satellite data more accessible for scientific studies and the general public. These products may also lead to additional discoveries, such as emission and lifetime estimates (Beirle et al., 2011; Fioletov et al., 2017, 2015; Liu et al., 2016; Valin et al., 2013; Whitburn et al., 2015, 2016b; Zhu et al., 2014; de Foy et al., 2015), source identification (Kort et al., 2014; McLinden et al., 2012, 2016), trend analyses (Duncan et al., 2016; Lamsal et al., 2015; Russell et al., 2012; Warner et al., 2017; Zhu et al., 2017b), assessment of environmental exposure for public health (Geddes et al., 2016; Zhu et al., 2017a), and satellite data validation (Zhu et al., 2016).

The operational level 3 products are typically provided at grid sizes of $\mathrm{0.25}{}^{\circ}\times \mathrm{0.25}{}^{\circ}$ or even $\mathrm{1}{}^{\circ}\times \mathrm{1}{}^{\circ}$, which are too coarse for regional heterogeneous emission sources (e.g., urban areas), especially for species with short lifetimes. These level 3 products are provided at fixed temporal intervals (e.g., daily, monthly, and annually). To customize the temporal and spatial sampling intervals, one often needs to regrid the level 2 data.

Various gridding algorithms have been developed to generate level 3 maps at
a regional scale with much finer grids (0.05–0.01^{∘}) than the
sizes of level 2 pixels, and this process is generally referred to as
“oversampling” (Russell et al., 2010; de Foy et al., 2009). In this work, we present
an agile, physics-based oversampling approach that represents each level 2
satellite pixel as a sensitivity distribution on the Earth's surface (e.g.,
the spatial response function), instead of a point or a polygon as assumed in
previous methods. A generalized 2-D super Gaussian function is used to
characterize the spatial response functions of both imaging grating
spectrometers (e.g., OMI, OMPS, and TROPOMI) and scanning Fourier transform
spectrometers (FTSs; e.g., GOSAT, IASI and CrIS). Applications to multiple
existing satellite datasets are also highlighted.

## 2.1 OMI

The OMI instrument aboard the Aura satellite launched in 2004 is a push-broom
UV–visible imaging grating spectrometer. It has a daytime equatorial crossing
at ∼13:42 LT (local time). During normal global observation mode, the
backscattered sunlight from the Earth is imaged by a telescope onto a
rectangular entrance slit perpendicular to the flight direction. The light
coming through the slit, which corresponds to an across-track angle of
115^{∘}, or 2600 km on the ground, is dispersed by optical gratings and
mapped on two 2D CCD detectors. Each detector image is aggregated
across-track (along the length of the slit) into 60 spectra, corresponding to
60 across-track spatial pixels for the UV2 (307–383 nm) and visible
(349–504 nm) bands, as shown by Fig. 1. Although the spatial
response functions of OMI pixels are
nonuniform (Sihler et al., 2017; de Graaf et al., 2016), the OMI pixels are widely
characterized as quadrilateral polygons defined by 75 % of the energy in the
along-track field of view (FOV) and the halfway points of the across-track
FOV (Kurosu and Celarier, 2010).
These OMI pixel polygons are close to rectangles, ranging from 14 km×26 km
at nadir (or 13 km×24 km if assuming nonoverlapping pixels)
to 28 km×160 km at the swath edges. Alternatively, OMI pixels can be
represented as tiled polygons with no overlap between adjacent pixels. These
tiled pixels produce a seamless swath image but are less accurate,
especially in the along-track direction. OMI is a highly successful mission
with long data records, and most of the successor missions follow a similar
design (Levelt et al., 2018). The oversampling technique demonstrated here can
be readily adopted for a range of OMI products and OMI's successor missions,
such as OMPS, TROPOMI, and TEMPO.

## 2.2 IASI

The IASI instrument is an FTS with an across-track scanning range of 2200 km (Fig. 1). It has a daytime equatorial crossing time of ∼09:30 LT. The first IASI instrument (IASI-A) was launched aboard the MetOp-A satellite in 2006, with the launch of IASI-B following in 2012 and IASI-C in 2018. IASI scans across the track with 30 mirror positions, or fields of regard (FORs), and each FOR is composed of a 2×2 array of pixels, or FOV. Each FOV projected on ground is a 12 km diameter circular footprint at nadir and elongates to ellipses towards the swath edges (Clerbaux et al., 2009). To simplify the ground pixel calculation, we represent each pixel as an ellipse with the major and minor axes and rotation angle interpolated from a lookup table based on latitude and FOR and FOV number.

We use the most recent neural network (NN) IASI NH_{3} retrieval based on
calculation of a hyperspectral range index (HRI) and subsequent conversion to
NH_{3} columns via a neural
network (Van Damme et al., 2017; Whitburn et al., 2016a). The IASI NH_{3} datasets
are publicly available for both IASI-A and IASI-B, with the version
2 (Van Damme et al., 2017) presenting significant improvements over version
1 (Whitburn et al., 2016a), including the negative values that are
crucial for observational error averaging near the detection limit.

## 2.3 CrIS

The CrIS instrument, which is aboard the Suomi NPP satellite and the series of JPSS satellites, is a step-scan FTS with 2200 km across-track width (Fig. 1). It has a daytime equatorial crossing time of ∼13:30 LT. It has the same number of FORs as IASI, but each FOR contains 9 FOVs (3×3 array), providing a better spatial coverage. Each CrIS FOV is 14 km at nadir, slightly larger than IASI. Due to the mounting angle of the scanning mirror, the FOR rotates differently at each scanning angle. Similar to IASI, each CrIS pixel is represented as a rotated ellipse.

The CrIS fast physical retrieval (CFPR) NH_{3} retrieval product is based on the
TES optimal estimation approach that minimizes the differences between
spectral radiances and a simulated fast forward line-by-line
model (Shephard and Cady-Pereira, 2015).

This section reviews existing gridding methods that map level 2 pixels to level 3 grids. Oversampling conventionally refers to the cases where level 3 grid is much finer than the level 2 pixel size.

## 3.1 Spatial interpolation

The spatial interpolation methods generate continuous data fields from
observations made at discrete locations. The main difference between
interpolation and the point- and polygon-based oversampling approaches
discussed in Sect. 3.2 and 3.3 is that
the values at grid cells that are not covered by satellite observations can
be estimated. Therefore, the spatial interpolation methods are more commonly
used for satellite datasets with significant spatial gaps or requiring
additional smoothing. Common spatial interpolation methods include nearest
neighbors, piecewise 2-D linear interpolation, spline interpolation, and
various kriging methods. The moving window block kriging method has been
proposed to generate global level 3 products for satellite observations of
long-lived species, such as CH_{4} and
CO_{2} (Tadić et al., 2015, 2017). A comprehensive review of
available spatial interpolation methods for environmental variables is
provided by Li and Heap (2014). There are relatively few
applications of spatial interpolation methods to regional
fine-grid oversampling, where each target grid cell usually receives a large number of
overlapping satellite observations. Kuhlmann et al. (2014)
proposed an interpolative gridding algorithm that reconstructs the trace gas
distribution by a continuous parabolic spline surface, defined on the lattice
of tiled satellite pixels. This approach produces smooth regional level 3
maps for the OMI NO_{2} products with specifically tuned smoothing
parameters but has not been tested in non-tiled observations with
significant numbers of missing values (e.g., IASI and CrIS).

## 3.2 Satellite observations as points

The simple “drop-in-the-box” gridding method can be classified into this
category, as each satellite observation is assumed to be a point on the
surface. The value for each target grid cell is the average of all screened
satellite observations with the center of the FOV falling inside the grid cell
boundaries. A conventional oversampling approach has been developed based on
the drop-in-the-box method; instead of only averaging “in the box”, it
includes satellite observations within a certain radius (much larger than the
grid size) from the center of each grid cell. This averaging radius is chosen
to balance the smoothing and noise but is also somewhat arbitrary. For
example, McLinden et al. (2012) used a radius of 8 km to oversample the OMI
NO_{2} tropospheric columns and a larger radius of 24 km to oversample the
OMI SO_{2} total columns near the Canadian oil sands region;
Fioletov et al. (2011) used 12 km to oversample the OMI SO_{2} total
columns over the US; and Zhu et al. (2014) used 24 km to oversample the
HCHO total columns near Houston, TX. This oversampling approach is referred
to as “point oversampling” hereafter, as the pixel geometry is not
considered. The pixel-specific observational errors are also not taken into
account.

Figure 2 reconstructs a point oversampling process for an
arbitrary target grid point (red star) located near Denver, CO. OMI NO_{2}
data (Krotkov et al., 2017) over the year 2005 are used in this demonstration.
Pixels with a cloud fraction ≥30 % or a solar zenith angle ≥75^{∘} are screened out. Only across-track positions with relatively
small pixel areas (6–55 out of 1–60) are included, a common practice to
oversample OMI data. Adding pixels at the swath edges would induce more
“false negative” cases, as shown below. The screened satellite pixel
centers that fall within a 12 km radius (dashed circle) are plotted as black
points and red triangles. The red triangles are “false positive”
observations because the corresponding pixel quadrilaterals, provided by the
OMPIXCOR product, do not cover the target grid point. The pixel geometry of
an extreme false positive case is illustrated by the pixel quadrilateral,
featuring the largest separation between its boundary and the target grid
point. Likewise, the false negative observations are plotted as purple
squares, whose pixel centers fall outside the averaging circle (and hence not
averaged), but these pixels cover the target grid point. An extreme case of
the false negatives is also illustrated. For this example, there are 243
pixels within the 12 km radius, of which 54 are false positives (22 %). There
are 92 false negatives (38 %) not included in the point oversampling.
Typically, false positives are pixels closer to nadir, whereas false
negatives are pixels away from nadir. In combination, the oversampled value
at this grid location has contributions from a much different set of
satellite observations than what should be represented. A larger averaging
radius will decrease the occurrence of false negative cases but increase
that of false positive cases. Because the OMI pixel dimension is larger at
the across-track direction, these sampling biases differ in direction;
observations in the across-track direction of the target grid point are more
likely to become false negatives, and observations in the along-track
direction are more likely to become false positives.

In reality, the OMI ground pixel footprints are not as sharp as quadrilateral boundaries (de Graaf et al., 2016), so the false positive and negative cases are not as well defined as in Fig. 2. This will be discussed in Sect. 4.1.

## 3.3 Satellite observations as polygons (i.e., tessellation)

This approach assumes that each satellite observation footprint is a polygon on the surface, and calculates the areal proportions of grid cells inside each polygon. Because calculating these overlapping areas requires filling irregular satellite footprint polygons with rectangular grid cells, it is also known as the “tessellation” approach. The contribution of each satellite observation to a given grid cell is weighted by the overlapping area and inversely weighted by the total pixel polygon area and the observational uncertainty, as shown by the following equations (Zhu et al., 2017a):

where

In the equations above, *C*(*j*) is the oversampled result for destination grid
cell *j*; Ω(*i*) is the variable to be oversampled (e.g., total column)
associated with the satellite pixel *i*; *S*(*i*,*j*) is the overlapping area
between pixel *i* and grid cell *j*, and hence ${\sum}_{j}S(i,j)$ is the total
area of pixel *i*, assuming that the grid extends beyond all pixel
boundaries. When the destination grid is regular with constant grid cell
area, it is convenient to normalize *S*(*i*,*j*) by the grid cell area, leading
to overlapping fractions. We will follow this convention hereafter, and hence
*S*(*i*,*j*) is always a dimensionless number. These equations take into account
the extent of a pixel and give more weight to a nadir observation than to an
observation at the edges of the satellite swath, where the information is
more smeared out. The variable *σ*(*i*)^{p} is the uncertainty term, and the power *p*
has been assumed to be 1 (Zhu et al., 2017a) or
2 (Spurr, 2003; Van Damme et al., 2014) by different studies. If we assume
each observation Ω(*i*) is a measurement of a constant true value with
Gaussian random error *σ*(*i*), *p*=2 yields the maximum likelihood
estimate of the true value. However, the true measurement and sampling errors
often show heavier tails than a Gaussian distribution. In this study we adopt
*p*=1, following Zhu et al. (2017a). The oversampled results are generally
similar for both cases. Unlike the point oversampling discussed in
Sect. 3.2 where *C*(*j*) is simply the average of Ω(*i*)
within a circle, the tessellation approach fully utilizes the geometry and
error information for each satellite observation. It has been adopted by many
operational level 3 products and oversampling
studies (Duncan et al., 2016; Kim et al., 2016; Krotkov, 2013; Li et al., 2017b; Liu et al., 2006; Van Damme et al., 2014; Wenig et al., 2008; Zhu et al., 2017a; de Foy et al., 2015).

It is sometimes convenient to define

to quantify the total number of overlapping pixel polygons used in averaging
for grid cell *j*. Unlike the point oversampling, this number does not have
to be an integer due to the consideration of partial overlaps. Because the
location and size of these pixels vary day by day, averaging a large number
of pixels reveals spatial patterns at scales finer than the satellite pixel
scales, if these patterns are consistent through the averaging time period.

Figure 3 illustrates the tessellation process for OMI (a)
and IASI (b) pixels, where the elliptical IASI pixel is represented by a
100-vertex polygon calculated from its minor/major axes and rotational
angle lookup tables. The destination grid size is 5 km × 5 km, and the
overlapping areas are normalized by the grid cell area (25 km^{2}), as
labeled in each grid cell.

## 4.1 Satellite observations as sensitivity distributions

The tessellation approach discussed in Sect. 3.3 inherently assumes that the satellite observation is uniformly sensitive to the scene inside the pixel polygon and has no sensitivity outside it. However, depending on target grid size and the spatial response function of specific satellite observations, this may be too strong of an assumption. For example, Schreier et al. (2010) characterized the complex spatial response function of the AIRS instrument and used it to improve the comparison of radiances measured by AIRS and MODIS. de Graaf et al. (2016) and Sihler et al. (2017) derived an in-flight spatial response function of OMI using collocated MODIS radiance. The operational Sentinel-5 Precursor, Sentinel-5, and Sentinel-4 cloud processors also rely on the spatial response functions of the imaging grating spectrometers to accurately calculate the cloud coverage within each FOV using collocated high-resolution cloud imagers (Siddans, 2017).

For imaging grating spectrometers like OMI, the spatial response function depends on the diffraction of the fore optics, the instantaneous field of view (i.e., the instantaneous projection of the slit on the ground from the point of view of a native detector pixel), the numbers of across- and along-track bins, and the along-track movement of subsatellite point during the integration time. The satellite movement only affects the along-track direction, generally making the spatial response in the along-track direction smoother than that in the across-track direction. de Graaf et al. (2016) and Sihler et al. (2017) fitted the OMI spatial response function using a 2-D super Gaussian function to parameterize the different smoothness in the along- and across-track directions. To standardize the representation of spatial response functions for diverse satellite sensors, we generalize the 2-D super Gaussian function as

where

In these equations, *x* and *y* are distances to the center of ground FOV in
orthogonal directions, usually transformed by geometric projections of the
across- and along-track directions. FWHM_{x} and FWHM_{y} are full widths at
half maximum of the spatial response function, *S*(*x*,*y*), in the directions of
*x* and *y*. The three exponential terms, *k*_{1}, *k*_{2}, and *k*_{3}, control
the distribution of spatial response, as illustrated by Fig. 4.
When *k*_{3}=1 (Fig. 4a and c), Eq. (5) becomes the 2-D
super Gaussian function used by de Graaf et al. (2016) and Sihler et al. (2017) to
characterize the OMI spatial response:

For OMI, *k*_{1}∼4 and *k*_{2}∼2 (de Graaf et al., 2016).

For FTS systems with stop-and-stare sampling, like IASI and CrIS, the spatial
response function (also known as point spread function by the community) is
more simply defined by the circular aperture and some diffraction around the
edge. The nadir FOV is circular with no difference between across- and
along-track directions, and hence the spatial response function can be
characterized by a 1-D super Gaussian function rotating around the nadir
point. This rotating super Gaussian function is another special case of the
generalized 2-D super Gaussian (Eq. 5) with ${k}_{\mathrm{1}}={k}_{\mathrm{2}}=\mathrm{2}$ and
*w*_{x}=*w*_{y}:

The smoothness of the rotating super Gaussian is controlled by only one
exponent, which equals to 2×*k*_{3}. The elongated spatial response
functions for off-nadir angles can be readily characterized by different
values for *w*_{x} and *w*_{y} (Fig. 4a–b). The spatial response
function of IASI is rather sharp at the edge with little variation at the
top, close to a super Gaussian with an exponent of ∼18 (CNES, 2015).
The spatial response function of CrIS is relatively smoother at the edge,
best fit by a super Gaussian with an exponent of ∼8 (Wang et al., 2013).
Details on the spatial response functions of IASI and CrIS can be found in
Appendix A.

In the generalized 2-D super Gaussian function (Eq. 5), *k*_{1}×*k*_{3} and *k*_{2}×*k*_{3} are the exponents in the *x* and *y*
directions, respectively, and determine the sharpness of the spatial response
in the corresponding direction. An exponent of 2 leads to a standard Gaussian
function; the larger exponents produce a top-hat shape, converging to a
boxcar shape when the exponent approaches
infinity (Beirle et al., 2017). Redistributing the contributions
from *k*_{1}/*k*_{2} and *k*_{3} makes hybrid spatial response functions that may
have sharp edges in sensitivity but rounded corners in space, as in the case
of OMPS (Glen Jaross, personal communication, 2017). The difference between this
hybrid case and conventional 2-D super Gaussian is illustrated by
Fig. 4c–d.

The projection of a rectangular FOV for imaging grating spectrometers like OMI
on the surface at large viewing angles leads to distorted quadrilateral
footprints, as shown by the polygon ABCD in Fig. 5a. To
account for this effect, a geometric transformation function is determined by
the OMI pixel corner points (ABCD in Fig. 5a) and the
corresponding rectangle (A^{′}B^{′}C^{′}D^{′} in Fig. 5b) defined by
the distances between the middle points of opposing edges of the OMI pixel
quadrilateral. The spatial response function is first calculated according to
Eq. (5) with FWHM_{x} =$\left|{\mathrm{A}}^{\prime}{\mathrm{D}}^{\prime}\right|$ and FWHM_{y} =$\left|{\mathrm{A}}^{\prime}{\mathrm{B}}^{\prime}\right|$ as shown in
Fig. 5b and then projected to match the OMI pixel corners
ABCD (Fig. 5a) using the geometric transformation function.
This algorithm is implemented using both the OpenCV library in Python and the
Image Processing Toolbox in MATLAB.

The proposed oversampling approach represents each satellite observation as a
sensitive distribution, instead of a point or a polygon. If the true
satellite spatial response function is used as the sensitive distribution,
this approach is the theoretically optimal solution to the oversampling
problem, and is hence referred to as “physical oversampling” hereafter. It
follows the same equations as the tessellation approach as in
Eqs. (1)–(4), except that the fractional overlapping area
*S*(*i*,*j*) is generalized to the integration of the spatial response function
of satellite observation *i*, $S(x,y|i)$, over the grid cell *j*:

where the denominator is the grid cell area. Similar to the tessellation
approach, *S*(*i*,*j*) is always a dimensionless number between 0 and 1. By
normalizing the grid cell area, this accurate form of *S*(*i*,*j*) can be
directly replaced by approximating values such as $S(x,y|i)$ evaluated at the
grid center. $S(i,j)/{\sum}_{j}S(i,j)$ is just the normalized spatial response
function for observation *i* so that its spatial integration is unity. If the
spatial response is uniform inside the pixel polygon and zero outside the
polygon, this integration of the spatial response function within the grid cell
is equivalent to the fractional overlapping area used in the tessellation
approach. As such, the tessellation is just the extreme case where the
spatial response function is a perfect 2-D boxcar. This corresponds to ${k}_{\mathrm{1}}\times {k}_{\mathrm{3}}\to \mathrm{\infty}$ and ${k}_{\mathrm{2}}\times {k}_{\mathrm{3}}\to \mathrm{\infty}$ in
Eq. (5).

This physical oversampling approach can also be considered as a spatial interpolation method as discussed in Sect. 3.1 because the spatial response function can be defined beyond the satellite pixel boundaries and theoretically on the entire 2-D space. Moreover, instead of the exact form of spatial response function, the satellite observations can be represented by similar (with the same FWHM) but smoother sensitivity distributions to enhance the quality of the oversampling results. This possibility will be demonstrated in Sect. 5.2.

## 4.2 Balancing the errors from tessellation and discretization of spatial response

The tessellation approach is perfect if the spatial response of satellite
observation is a boxcar, but otherwise it will introduce some error in the
oversampled results (referred to as “tessellation error” hereafter). When
the satellite spatial response function is smooth (instead of a boxcar), the
exact solution is to calculate *S*(*i*,*j*) as the integration of the spatial
response of satellite observation *i* over the area covered by the target
grid cell *j* (Eq. 10). It is computationally demanding to
numerically integrate the spatial response of all satellite pixels over each
grid cell. To simplify it, one may discretize the spatial response function
to the target oversampling grid and use the spatial response value at the
grid center to approximate the integration. As such, the spatial response
function only needs to be evaluated once per pixel per grid cell. To improve
this simple discretization scheme, we calculate a weighted average of the
spatial response values at the grid center and grid corners (Yang and Wolfe, 2001). Because the grid corners are shared
by neighboring grid cells, this approach only doubles the spatial response
calculation but significantly reduces the error induced by discretization
(“discretization error” hereafter). Appendix B gives a detailed comparison
of different discretization schemes.

The satellite sensors have very different spatial responses. The target grid
size for level 3 data ranges from 0.25^{∘} (∼25 km) for many global
operational products to 0.01^{∘} (∼1 km) for regional oversampling.
The discretization error decreases as the size of the target grid cells
becomes finer and the spatial response of satellite observations becomes
better resolved. At any fixed target grid size, spatial response functions
with smoother edges are better approximated by the discretization scheme. As
such, it is essential to balance the tessellation and discretization errors based
on the target grid cell size and the smoothness of the satellite spatial
response so that the most accurate and efficient approximating method can be
chosen.

Figure 6 compares the tessellation and discretization
errors when oversampling synthetic OMI observations to a grid of 1 km
(∼0.01^{∘}). A checkerboard pattern is used as the “true”
concentration distribution (alternating values of zeros and ones with a spatial
period of 20 km × 20 km, as shown in Fig. 6a; it also
shows OMI pixel polygons at across-track position no. 1 in red and across-track
position no. 30 in cyan). Synthetic OMI observations are generated by sampling
the checkerboard pattern using the OMI spatial response function, simplified
using Eq. (8) with *k*_{1}=4, *k*_{2}=2 and discretized at a very fine
grid (0.05 km, or ∼0.0005^{∘}) so that the spatial response
distribution is always fully resolved. The locations of OMI observations are
from the real OMI NO_{2} products (Krotkov et al., 2017), filtered by cloud
fraction <25 % and solar zenith angle <75^{∘} for 2005–2006. Instead
of NO_{2} columns, the synthetic OMI observations at these locations are
oversampled. The oversampled area is in the north midlatitude
(∼40^{∘}Ṅ). In Fig. 6b, the oversampling is
conducted at a native grid size (0.05 km), and then the result is
block-averaged to the 1 km target grid size to represent ideal OMI
observations, as in Eq. (10). One should note that this
discretization at 0.05 km is used to get the true map of OMI observation
where the discretization error is negligible. It is unnecessary to oversample
at this fine grid in general. Figure 6c and e show the
results for tessellation and discretization of the spatial response at
1 km
grid, where *S*(*i*,*j*) is approximated by fractional overlapping area and the
discretization scheme, respectively. They both reproduce the checkerboard
pattern in general, but the tessellation method generates errors up to 40 %
(Fig. 6d) relative to the peak-to-trough value of the
ideal observation because the OMI spatial response is smooth
(Fig. 5) instead of boxcar. In contrast, the discretization
error is much smaller (Fig. 6f) because of the small
size of the target grid cells (1 km).

The analysis for Fig. 6 is repeated for a range of
target grid sizes (1–50 km, or about 0.01–0.5^{∘}) and different
smoothness of the spatial response functions using the same OMI observation
locations. The spatial response function is assumed to be 2-D super Gaussian
(Eq. 8). The exponent in the along-track direction (*k*_{2}) is
tuned from 2 to 64, whereas the exponent in the across-track direction
(*k*_{1}) is set to be 2×*k*_{2}. Figure 7a shows, for
satellite observations with a quadrilateral FOV, the contour of the ratio
between the discretization error and the tessellation error, calculated as
the root-mean-squares of the differences between the ideal observation and
the simplifications using tessellation and spatial response discretization,
respectively. The contour line of unity divides the regimes where
tessellation and discretization errors are dominant: discretization of the
spatial response is more accurate for fine-grid oversampling of satellite
observations with smooth spatial responses (small *k*_{1} and *k*_{2});
tessellation is more accurate for coarser target grids and sharper spatial
responses. Tessellation is perfect if *k*_{1} and *k*_{2} both approach infinity.
The case of OMI (*k*_{1}=4, *k*_{2}=2) lies at the left edge (red vertical
dashed line in Fig. 7a), and its intersect with the unity
contour line is located at the target grid size of ∼16 km. In other words,
it is beneficial to explicitly consider the spatial response of OMI
observation for target oversampling grids finer than ∼16 km (about
0.15^{∘}).

Similarly, Fig. 7b shows the ratios between
discretization and tessellation errors for satellite observations with
circular FOVs. The pixel dimensions and locations of IASI observations for
2015–2016 are used with standard data screening, and the spatial response
function is assumed to be a rotating super Gaussian
(Eq. 9). The exponential term (equal to 2×*k*_{3})
varies from 2 to 64. When characterizing the IASI spatial response as a
rotating super Gaussian function, the exponent is about 18, intersecting the
unity contour line at the target grid size of ∼2 km. If the IASI
instrument had the same spatial response as CrIS (the exponent is about 8),
the intersect would be at the target grid size of ∼4 km. The results
would be very similar when using the CrIS observation locations instead of
IASI because the exact locations of any observations are averaged out and
the IASI and CrIS pixel sizes are similar.

As shown by Fig. 7, the balance between tessellation and
discretization errors depends on both the target grid size and the deviation
of satellite spatial response function from an ideal 2-D boxcar shape. The
uncertainty in the knowledge of the spatial response functions is not
considered here, but the spatial response function can be characterized
prelaunch and validated
on orbit (Schreier et al., 2010; Sihler et al., 2017; de Graaf et al., 2016). For all three
cases, the tessellation error significantly outweighs the discretization
error at 1 km oversampling grid size by a factor of 4 for IASI and over 200
for OMI. Therefore, we recommend discretization of the spatial response
function at a 1 km (or 0.01^{∘}) grid for regional scale oversampling of
OMI, IASI, and CrIS data and then co-adding to coarser grids if necessary. The
threshold grid size where tessellation and discretization errors balance also
depends on the ground size of satellite FOV. For the OMI successor missions
with significantly smaller pixels (e.g., TROPOMI, TEMPO), the threshold grid
size is expected to be finer.

## 4.3 Spatial resolution and spatial sampling

The difference between resolution and sampling density for 1-D spectral data has been thoroughly discussed in the literature (Chance et al., 2005). However, for 2-D, spatially resolved data, it is common to refer to both the sizes of the level 2 pixels and the size of the level 3 grid as the spatial “resolution” of the data. To avoid confusion, it is emphasized here that the true spatial resolution is limited by the sizes of level 2 pixels. The size of level 3 grid only determines the density of spatial sampling, which does little to enhance the true resolving power of the data after reaching a certain point. For example, the oversampling results using synthetic OMI data at 1 vs. 0.05 km grids are very similar (Fig. 6). Nonetheless, it is still beneficial to oversample, i.e., make level 3 grid size significantly smaller than level 2 pixel sizes, as demonstrated by Fig. 8. As the ground truth, an array of 2-D Gaussian functions are generated with FWHM ranging from 1 to 16 km (the second column of Fig. 8) and peak height of unity, and this true field of concentration is measured by an imaginary sensor whose spatial response function is a 2-D super Gaussian (Eq. 8) with FWHM = 10 km and ${k}_{\mathrm{1}}={k}_{\mathrm{2}}=\mathrm{8}$ (the first column and the white boxes inserted in the third column). The third column shows the oversampling results using 10 000 randomly located observations. The fine structures in the ground truth are clearly smoothed, limited by the spatial resolution that is inherent to the level 2 pixel sizes (10 km). However, by oversampling at a fine grid (0.2 km for the first row vs. 5 km for the second row), the spatial gradients are better recovered, and spatial features finer than individual level 2 pixels can be identified. Additionally, the details in the spatial response function is better resolved with a finer target grid, which is particularly beneficial when collocating with higher resolution measurements (e.g., a cloud imager). As such, although the spatial resolving power is ultimately determined by the spatial extent of satellite pixels, the physical oversampling approach helps in enhancing the visualization of spatial gradient and the identification of emission sources.

## 5.1 Physical oversampling using OMI data

Figure 9 compares the drop-in-the-box method, point
oversampling, tessellation, and physical oversampling using OMI NO_{2}
tropospheric vertical column density (TVCD) within a 200 km × 200 km square
centered around a power plant in Arizona. The first column shows the simple
drop-in-the-box method on a 10 km grid. The second column averages OMI
observations within a 12 km radius of each grid center. These two approaches
assume OMI observations as points without consideration of pixel geometry and
retrieval uncertainties. The third column shows results using the
tessellation approach, and the fourth column shows the physical oversampling
using the OMI spatial response functions as a 2-D super Gaussian function with
*k*_{1}=4 and *k*_{2}=2. The target grid size is 1 km for the last three
approaches. The first and third rows show the oversampled results (*C*(*j*) in
Eq. 1) using 5 days (1–5 July 2005) and 5 months (May–September 2005)
of data, respectively. The second and fourth rows show the
corresponding numbers of pixels included in the averaging for each grid cell
(*D*(*j*) in Eq. 4). For the drop-in-the-box approach, the total
number of satellite observations included for each grid cell is much smaller
and shown with a different color scale for the 5-month averaging.

The drop-in-the-box approach shows significant data gaps (5-day averaging)
and high level of noise (5-month averaging), even when its target grid is 10
times coarser than the other oversampling approaches. There are two gaps
where no observation is available for point oversampling over the 5 days
(column 2, rows 1–2 in Fig. 9), which is an example of
false negatives as these gaps are actually covered by OMI pixels (column 3,
rows 1–2 in Fig. 9). The physical oversampling in the
fourth column consistently shows the smoothest results with clear
identification of the point source at the center of the domain, because the
spatial response function of OMI is properly incorporated. The oversampled
NO_{2} TVCD is biased high for the point oversampling approach because all
observations within the averaging radius are averaged equally, but larger
observation values generally are associated with larger uncertainties. The
results from tessellation become increasingly similar to those from physical
oversampling for longer averaging times, because the tessellation error is
randomly distributed and will eventually be averaged out. The physical
oversampling also does not require more computational resources than point
oversampling and tessellation, making it suitable for a wide range of spatial
scales and target grids.

## 5.2 Physical oversampling using IASI data with smoother spatial sensitivity distributions

Although the physical oversampling using the true satellite spatial response
functions produces the optimal estimation, the result is sometimes noisy and
even unphysical, especially when the observations are noisy and sparse. In
these cases, some spatial interpolation or smoothing methods are often
needed. In addition to the specialized interpolation and smoothing methods
discussed in Sect. 3.1, some smoothing can be applied
within the oversampling framework. For example, the level of smoothing can be
adjusted by the averaging radius in the point oversampling approach.
Barkley et al. (2017) used a Gaussian filter to smooth tessellation results
for OMI HCHO and CHOCHO products. When using the generalized 2-D super
Gaussian function to characterize the satellite spatial response function
(Eq. 5), it is also simple to tune the exponents (*k*_{3} in the
cases of circular FOVs such as IASI and CrIS and *k*_{1} and *k*_{2} in the cases of
quadrilateral FOVs such as OMI) so that the assumed satellite spatial
sensitivity distribution is smoother than the true spatial response function.
This often leads to better visualization and identification of local hot
spots, especially for products with a high noise level or sparse spatial
sampling. The advantage of this approach is that the smoothing is applied at
the satellite pixel level (level 2) instead of grid level (level 3), so the
geometry and error information for each satellite observation are preserved.

Figure 10 shows similar oversampling results as
Fig. 9, but using IASI NH_{3} total column density
data (Van Damme et al., 2017) for 2015 in eastern Colorado, centered around a
large cattle feedlot. The drop-in-the-box approach is not shown for IASI. The
results from point oversampling, tessellation, and physical oversampling to a
1 km grid are presented in the first three columns. The true IASI spatial
response functions have rather sharp edges (see Appendix A), so the physical
oversampling shown in the third column of Fig. 10 is very
similar to tessellation shown in the second column. Although this is the
optimal estimation based on the physics of IASI observation, the spatial
gradients are hard to identify for 5-day averaging and noisy for 5-month
averaging. Instead of applying smoothing after the oversampling process, the
fourth column uses a smooth spatial sensitivity distribution of a 2-D
standard Gaussian function (2*k*_{3}=2, rather than the true IASI spatial
response function with 2*k*_{3}∼18). As illustrated by the first row in
Fig. 10, the physical oversampling using smoother spatial
sensitivity distributions provides the best results by clearly identifying the
central point source using only sparse (5-day) data. The third row in
Fig. 10 demonstrates that with 5 months of averaging, the
local NH_{3} gradients are well resolved. The point oversampling using a
12 km radius overly smooths the results, making the central hot spot
artificially larger, whereas the general spatial gradients are still noisy
(column 1, row 3). The overall number of IASI observations used in point
oversampling is also significantly higher than tessellation and physical
oversampling, as shown by the fourth row. This is because the
12 km
averaging circle is much larger than most IASI footprints, and hence many
IASI observations are double counted as false positives. The smoothing based
on physical oversampling is much more effective in suppressing the noise, and
the spatial gradients are adequately preserved (column 4, row 3). This is
because each satellite FOV keeps the same FWHM and overall weight, and only
the distribution of sensitivity becomes more spread out.

Oversampling based on Eqs. (1)–(3) also provides a flexible way
to categorize the results according to environmental and temporal variables.
The conventional way is to save the averaging weights for each level 2
observation (i.e., the level 2G product, where level 2 pixels are assigned to
points of the latitude and longitude grid), but the averaging weights can only be
defined for a specific grid. When representing each level 2 observation as a
spatial sensitivity distribution (the actual instrument spatial response
function or a smoother version of it), *A*(*j*) and *B*(*j*) can be calculated at
fine spatial and temporal grids and then aggregated spatially and/or
temporally. The level 3 map *C*(*j*) is just the grid-by-grid ratio of the
aggregated *A*(*j*) and *B*(*j*). Similarly, *A*(*j*) and *B*(*j*) can be calculated
according to environmental variables such as wind and temperature at fine
intervals and binned to coarser categories as needed.
Figure 11 shows the physical oversampling of NH_{3} total
column under southerly winds (meridional wind component >0, panels a and c) and
northerly winds (meridional wind component <0, panels b and d) and high PBL
temperature (>15 ^{∘}C, panels a and b) and low PBL temperature (<15 ^{∘}C,
panels c and d). Here the PBL temperature is the average air temperature from
the surface to the top of the PBL, weighted by pressure. The average wind speed
and wind direction under each category are labeled in the corresponding
panels. IASI-A daytime data from 2008 to 2017 over northeastern Colorado are
included in the oversampling, and a 2-D standard Gaussian is used as the
spatial sensitivity distribution to smooth the results. The 3-D wind field,
atmospheric temperature, surface pressure, and PBL height are interpolated
from the North American Regional Reanalysis (Mesinger et al., 2006) from their native resolutions of 32 km
and 3 h to
the IASI pixel locations and overpass time. Using the concentrated animal
feeding operation (CAFO) locations (colored dots; data courtesy of Daniel Bon, Colorado Department of Public Health and Environment) as a spatial
reference, the downwind dispersion of the total NH_{3} column under different
wind directions is clearly seen. The close match between large cattle CAFOs
and the NH_{3} hot spots seen from space confirms that they are the dominant
source of atmospheric NH_{3} in this region. The overall abundance of NH_{3}
is significantly higher at warmer temperatures, in agreement with the
previous in situ quantification of CAFO NH_{3} emissions in the same
region (Sun et al., 2015b).

A physics-based approach is developed to oversample diverse satellite observational products to high-resolution destination grids. It represents each FOV as a sensitivity distribution on the ground, which is physically a more realistic representation of satellite observations. This sensitivity distribution can be determined by the spatial response function of each satellite sensor. We propose a generalized 2-D super Gaussian function that can standardize the spatial response functions of many satellite sensors with distinct observation mechanisms and viewing geometries. This generalized 2-D super Gaussian function can be reduced to a rotating super Gaussian to characterize the circular FOV of IASI and CrIS or a 2-D super Gaussian to characterize the quadrilateral FOV of OMI and its successors. It can also represent hybrid cases where the FOV is quadrilateral but with rounded corners. When the shape-determining exponents in the generalized 2-D super Gaussian function approach infinity, the FOV is equivalent to a polygon, as assumed in the tessellation approach.

Synthetic OMI and IASI observations were generated assuming the spatial
response functions are perfectly known to compare the tessellation error and
the discretization error. The balance between these two error sources depends
on the target grid size, the ground size of FOV, and the smoothness of
spatial response functions. The proposed oversampling approach is generally
more accurate for fine-grid oversampling of satellite observations with
smooth spatial responses, whereas tessellation is more accurate for coarse
grids and sharper spatial responses. For OMI, CrIS, and IASI, the threshold
target grid size where both errors are equal are at ∼16, ∼4, and
∼2 km, respectively. Therefore, it is recommended to oversample to 1 km
(0.01^{∘}) and then co-add to coarser grids if necessary for regional
studies. The tessellation may be more desirable for generating global level 3
products with coarse grids. The generalized 2-D super Gaussian function also
enables smoothing of the level 3 results by decreasing the shape-determining
exponents, useful for high noise levels or sparse satellite datasets. This
smoothing performed at each observation is more physically realistic than
arbitrarily tuning the averaging radius and the spatial filtering of the
level 3 map as the weightings of level 2 pixels are unchanged.

The new physical oversampling approach is applied to OMI NO_{2} products and
IASI NH_{3} products, showing substantially improved visualization of trace
gas distribution and local gradients. With proper consideration of the
spatial response functions, this approach can be applied to multiple
previous, current, and future satellite datasets, which will help to create
long-term consistent data records for atmospheric composition.

A MATLAB implementation of the physical oversampling is available at https://github.com/Kang-Sun-CfA/Oversampling_matlab/, last access: 5 December 2018 (Sun, 2018).

The spatial response functions of IASI are tabulated at https://iasi.cnes.fr/en/IASI/A_caract_instr.htm, last access: 10 December 2017, for each of its four detector pixels. They are very close to ideal circular FOV with some smoothing at the edge and weak non-homogeneity at the top response, as shown by Fig. A1.

Figure A2 shows a rotating super Gaussian function (Eq. 9) fitted to the tabulated spatial response function at detector pixel no. 2 and the fitting residual. With only two parameters (the width and exponent of the super Gaussian), the spatial response function can be well reconstructed by the rotating super Gaussian function.

Figure A3a shows the fitting of the across-track cross
section of the spatial response function of IASI detector pixel no. 2 using a
1-D super Gaussian function. The FWHM is 11.6 km on the ground and the
exponent is ∼18. The detailed information on the spatial response of
CrIS detectors is proprietary, but Wang et al. (2013) provides the spatial
response values at a few angles; i.e., the angles of 1.2380,
1.1000, 0.9420, and 0.8735^{∘} correspond to 3 %, 10 %,
50 %, and 70 % of the peak response. Based on this information, a 1-D super
Gaussian can be fitted with FWHM=13.6 km on the ground and an exponent of
7.93, as shown by Fig. A3b. The CrIS orbit height is
assumed to be 824 km above the ground.

To compare different discretization schemes, we first construct an ideal
spatial response function using OMI pixel boundaries but sharper edges (*k*_{1}=12, *k*_{2}=6, see Fig. B2a) and zoom in to a
single grid cell of 5 km × 5 km (Fig. B1a).
The true value of *S*(*i*,*j*) should be the integration of the spatial response
function over the grid cell area as in Eq. (10). A simple
discretization scheme is to use the spatial response value at the grid
center, C (Fig. B1b):

where *S*(C) denotes the evaluation of continuous spatial response function
*S*(*x*,*y*) at the coordinates of the grid center C. A more advanced
discretization scheme is to calculate the spatial response values at both the
grid center and the grid corners ABDE
(Fig. B1c) and approximate the integration as
the sum of the volumes of four triangular prisms (i.e., ABC, BDC, DEC,
and EAC):

Hence it is a weighted average with the weight for grid center twice that of the
weight for grid corners. For completeness, the assumption of tessellation is
also shown in Fig. B1d, where spatial response
is assumed to be unity inside the pixel boundary and zero outside. *S*(*i*,*j*)
is calculated as the fractional area covered by the portion of pixel polygon
within the grid cell.

In Fig. B2, both discretization schemes and
tessellation are applied to calculate *S*(*i*,*j*) for all grid cells near the
satellite FOV. Figure B2b–d shows the
distribution of errors from these three approximation methods, where the true
*S*(*i*,*j*) is the numerical integration of the high-resolution spatial response
function shown in Fig. B2a. The errors in both
discretization schemes (discretization only at grid center,
Fig. B2b, and weighted averaging of grid center
and grid corners, Fig. B2c) and the tessellation
error are shown as the root-mean-square of the error distribution. The
discretization scheme using both grid center and grid corner values
significantly reduces the error, which in this case is also lower than the
tessellation error. For a realistic OMI spatial response function (*k*_{1}=4,
*k*_{2}=2), the discretization errors in both cases are significantly lower
than the tessellation error at this grid size (5 km).

KS, LZ, KY, and GH developed and implemented the oversampling algorithms. KCP provided expertise on the CrIS instrument and products. CCM, KC, GGA, and XL provided expertise on the OMI instrument and products. LC, PFC, MVD, and MZ provided expertise on the IASI instrument and products. KS collected the data, analyzed the results, and wrote the manuscript. All authors contributed to interpretations and edited the manuscript.

The authors declare that they have no conflict of interest.

We acknowledge support from NASA (sponsor contract numbers NNX14AF16G and NNX14AF56G), the RENEW
Institute and School of Engineering and Applied Science at the University at
Buffalo, and Smithsonian Institution subaward SV8-8802. We thank John Houck
at the SAO; Thomas Kurosu at JPL; Holger Sihler at MPI-C; Glen Jaross at
NASA; Rui Wang, Xuehui Guo, and Da Pan at Princeton University; and Likun Wang
at University of Maryland for helpful discussions. We thank the OMI
science team for making the OMI NO_{2} data available at
https://disc.gsfc.nasa.gov/datasets/OMNO2_V003/summary, last access: 1 July 2018, and the IASI science
team for making the IASI NH_{3} retrieval available at
http://iasi.aeris-data.fr/NH3, last access: 1 October 2018. Lieven Clarisse is a research associate with
the Belgian F.R.S-FNRS and acknowledges the support.

Edited by: Jun Wang

Reviewed by: two anonymous referees

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- Abstract
- Introduction
- Satellite observations
- Existing gridding methods
- Proposed method
- Applications to satellite datasets
- Conclusions
- Code availability
- Appendix A: Spatial response functions of IASI and CrIS as rotating super Gaussian functions
- Appendix B: Comparison of discretization schemes
- Author contributions
- Competing interests
- Acknowledgements
- References

- Abstract
- Introduction
- Satellite observations
- Existing gridding methods
- Proposed method
- Applications to satellite datasets
- Conclusions
- Code availability
- Appendix A: Spatial response functions of IASI and CrIS as rotating super Gaussian functions
- Appendix B: Comparison of discretization schemes
- Author contributions
- Competing interests
- Acknowledgements
- References