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Research Article

PHiFA-A tool for numerical propagation of high-fidelity astrodynamics

Yang Yang1( )Erik Klein2Changyong He3 Han Cai4Yan Zhang1
School of Aeronautics and Astronautics, Sun Yat-sen University, Shenzhen, 518000, China
Institut for Space Systems, TU Braunschweig, 38108, Braunschweig, Germany
ENSG-Géomatics, Institut national de l'information géographique et forestière (IGN), F-77455, Marne-la-Vallée, France
School of Aerospace Engineering, Beijing Institute of Technology, Beijing, 100081, China
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Abstract

This paper presents a tool for the numerical propagation of high-fidelity astrodynamics, called PHiFA. The coupled orbit-attitude dynamics for space objects are modeled by considering various types of perturbative forces and torques. Two methods have been implemented to calculate the surface forces: the area matrix method and the beam method. The beam method is more precise as it discretizes the source media (e.g., sunlight and aerodynamic wind) and the surface of the target into multiple rays and finite elements, respectively, and then accumulates the effect of each hit. The PHiFA tool was tested and validated using a 3U CubeSat model and the defunct European environment satellite (Envisat) model.

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Astrodynamics
Pages 189-204

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Cite this article:
Yang Y, Klein E, He C, et al. PHiFA-A tool for numerical propagation of high-fidelity astrodynamics. Astrodynamics, 2022, 6(2): 189-204. https://doi.org/10.1007/s42064-021-0113-1

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Received: 12 May 2021
Accepted: 10 September 2021
Published: 29 January 2022
© Tsinghua University Press 2021