A physics-based approach to oversample multi-satellite, multispecies observations to a common grid
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Published:2018-12-18
Issue:12
Volume:11
Page:6679-6701
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ISSN:1867-8548
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Container-title:Atmospheric Measurement Techniques
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language:en
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Short-container-title:Atmos. Meas. Tech.
Author:
Sun KangORCID, Zhu LeiORCID, Cady-Pereira Karen, Chan Miller Christopher, Chance KellyORCID, Clarisse LievenORCID, Coheur Pierre-François, González Abad GonzaloORCID, Huang GuanyuORCID, Liu Xiong, Van Damme MartinORCID, Yang KaiORCID, Zondlo Mark
Abstract
Abstract. 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 NO2 products and IASI NH3 products. There is no appreciable difference in the computational time
when using the physical oversampling versus other oversampling methods.
Publisher
Copernicus GmbH
Subject
Atmospheric Science
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