Effect of ionospheric drag on atmospheric density estimation and orbit prediction

2019 ◽  
Vol 63 (8) ◽  
pp. 2495-2505 ◽  
Author(s):  
C.J. Capon ◽  
B. Smith ◽  
M. Brown ◽  
R. Abay ◽  
R.R. Boyce
2020 ◽  
Vol 65 (8) ◽  
pp. 1965-1980
Author(s):  
Shaylah Mutschler ◽  
Penina Axelrad ◽  
Tomoko Matsuo

2021 ◽  
Author(s):  
Shunchenqiao Bai ◽  
Guangwei Wen ◽  
Zhaokui Wang

Abstract Atmospheric drag calculation error greatly reduce the low-earth orbit spacecraft trajectory prediction fidelity. To solve the issue, the "correction - prediction" strategy is usually employed. In the method, one parameter is fixed and other parameters are revised by inverting spacecraft orbit data. However, based on a single spacecraft data, the strategy usually performs poorly as parameters in drag force calculation are coupled with each other, which result in convoluted errors. A gravity field recovery and atmospheric density detection satellite, Q-Sat, developed by xxxxx Lab at xxx University, is launched on August 6th, 2020. The satellite is designed to be spherical for a constant drag coefficient regardless of its attitude. An orbit prediction method for low-earth orbit spacecraft with employment of Q-Sat data is proposed in present paper for decoupling atmospheric density and drag coefficient identification process. For the first step, by using a dynamic approach-based inversion, several empirical atmospheric density models are revised based on Q-Sat orbit data. Depends on the performs, one of the revised atmospheric density model would be selected for the next step in which the same inversion is employed for drag coefficient identification for a low-earth orbit operating spacecraft whose orbit needs to be predicted. Finally, orbit forecast is conducted by extrapolation with the dynamic parameters in the previous steps. Tests are carried out for the proposed method by using a GOCE satellite 15-day continuous orbit data. Compared with legacy “correction - prediction” method in which only GOCE data is employed, the accuracy of the 24-hour orbit prediction is improved by about 171m the highest for the proposed method. 14-day averaged 24-hour prediction precision is elevated by approximately 70m.


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