Abstract

The Atmospheric Infrared Ultraspectral Sounder (AIUS), the first high-resolution (0.02 cm−1) solar occultation sounder, aboard GF5, was launched in May 2018 from China. However, relevant studies about vertical profiles of atmospheric constituents based on its operational data were not conducted until half a year later. Due to an urgent need for Hin-orbit tests, the real spectra (called reference spectra hereafter) were substituted with simulated spectra calculated from the reference forward model (RFM) plus different random noises at different altitudes. In the generation process of the reference spectra for N2O, NO2, and HF species, ACE-FTS (Atmospheric Chemistry Experiment–Fourier Transform Spectrometer instrument on the SCISAT satellite) level 2 products replace corresponding profiles included in the atmospheric background profiles. The optimal estimation method is employed to extract N2O, NO2, and HF profiles in this study. Comparing the retrieved results with ACE-FTS level 2 products, the relative deviations for these three species are calculated. For N2O, the average relative deviation is less than 6% at altitudes below 25 km, while larger deviations are observed in the range of 25–45 km, with the maximum being at ~25%. Additionally, the difference for NO2 is less than 5% in the 20–45 km range, with a larger discrepancy found below 20 km and above 45 km; the maximum deviation reaches ±40%. For HF, the relative deviation is less than 6% for all tangent heights, implying satisfactory retrieval. The vertical resolution, averaging kernel, and number of degrees of freedom are used to assess the retrieval algorithm, which indicate that the retrieved information content is much more attributable to the reference spectra contribution than to the a priori profile. Finally, a large number of retrieval tests are performed for N2O, NO2, and HF in selected areas covering the Arctic region, northern middle latitude, tropics, southern middle latitude, and Antarctic region, and reliable results are obtained. Thus, to a great extent, the algorithm adopted in the AIUS system can process retrievals reliably and precisely.

Highlights

  • The Atmospheric Infrared Ultraspectral Sounder (AIUS) has a high spectral resolution of 0.02 cm−1 while operating over a broad wavenumber range of 2.4–13.3 μm (750–4100 cm−1 )

  • This paper aims to is to test the retrieval performance by using synthetic measurements based on AIUS instrument characteristics for HF, NO2, and Nitrous oxide (N2 O)

  • The retrieval scheme of AIUS is based on the reference forward model (RFM) to simulate infrared atmosphere radiation transmission

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Summary

Introduction

The Atmospheric Infrared Ultraspectral Sounder (AIUS) has a high spectral resolution of 0.02 cm−1 while operating over a broad wavenumber range of 2.4–13.3 μm (750–4100 cm−1 ). AIUS was designed to measure atmospheric absorption spectral sequences. These spectra, detected in the limb viewing geometry tangent heights, are inverted to obtain the vertical profiles of atmospheric constituents [1]. AIUS, which was launched on 9 May 2018, features instrument parameters that are similar to those of ACE-FTS. Three ACE-FTS level 2 profile products were assumed as the true profiles to simulate the spectra of AIUS for HF, NO2 , and N2 O. Its primary instrument is a high-spectral-resolution (0.02 cm−1 ) infrared Fourier transform spectrometer (ACE-FTS), with a wavenumber range of 750–4400 cm−1

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