First Galileo Single-Frequency Occultation Process and Precision Analysis of FengYun3E

Author:

Yang Ming1234,Meng Xiangguang1234ORCID,Tian Haoran1234,Sun Yueqiang1234,Du Qifei1234,Bai Weihua1234,Wang Bowen1234ORCID,Wang Xianyi1234ORCID,Hu Peng1234,Tan Guangyuan134

Affiliation:

1. National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China

2. School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China

3. Beijing Key Laboratory of Space Environment Exploration, Chinese Academy of Sciences, Beijing 100190, China

4. Key Laboratory of Science and Technology on Space Environment Situational Awareness, Chinese Academy of Sciences, Beijing 100190, China

Abstract

This article proposes a single-frequency occultation method whose core is the reconstruction of a second frequency measurement. We process the actual received Galileo E1 single-frequency occultation observation data of FengYun3E to meet the urgent need for single-frequency Galileo occultation inversion of FengYun3 E/F/G/H satellites. Galileo single-frequency occultation events are globally distributed evenly and have stable quantities. The refractive index products and dry temperature products inverted from the single-frequency occultation data are reliable at altitudes of 5–30 km. The Galileo E1 single-frequency occultation process can effectively improve the output of FengYun3E/GNOS occultation products. These results validate the feasibility and correctness of using FengYun3/GNOS for the actual Galileo single-frequency occultation process. The atmospheric occultation products of Galileo single-frequency occultation increase the quantity of global occultation products and serve as a beneficial supplement to global numerical weather prediction data sources.

Funder

National Natural Science Foundation of China

Youth Cross Team Scientific Research Project of the Chinese Academy of Sciences

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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