Analytical attitude prediction of spin stabilized spacecrafts perturbed by magnetic residual torque


Autoria(s): Zanardi, M. C.; Quirelli, IMP; Kuga, H. K.; Moore, P.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

20/05/2014

20/05/2014

01/01/2005

Resumo

An analytical approach for spin-stabilized spacecraft attitude prediction is presented for the influence of the residual magnetic torques. Assuming an inclined dipole model for the Earth's magnetic field, an analytical averaging method is applied to obtain the mean residual torque every orbital period. The orbit mean anomaly is utilized to compute the average components of residual torque in the spacecraft body frame reference system. The theory is developed for time variations in the orbital elements, and non-circular orbits, giving rise to many curvature integrals. It is observed that the residual magnetic torque does not have component along the spin axis. The inclusion of this torque on the rotational motion differential equations of a spin stabilized spacecraft yields conditions to derive an analytical solution. The solution shows that residual torque does not affect the spin velocity magnitude, contributing only for the precession and the drift of the spin axis of the spacecraft. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.

Formato

460-465

Identificador

http://dx.doi.org/10.1016/j.asr.2005.07.020

Satellite Dynamics In the Era of Intredisciplinary Space Geodesy. Oxford: Elsevier B.V. Ltd, v. 36, n. 3, p. 460-465, 2005.

0273-1177

http://hdl.handle.net/11449/9269

10.1016/j.asr.2005.07.020

WOS:000235247800019

Idioma(s)

eng

Publicador

Elsevier B.V.

Relação

Satellite Dynamics In the Era of Intredisciplinary Space Geodesy

Direitos

closedAccess

Palavras-Chave #attitude propagation #spin stabilized satellite #residual magnetic torque #geomagnetic field
Tipo

info:eu-repo/semantics/article