| Texto completo | |
| Autor(es): |
de Moraes, Rodolpho Vilhena
;
Raimundo, Paula Cristiane P.
;
Kuga, Helio K.
;
Seago, JH
;
Neta, B
;
Eller, TJ
;
Pelletier, FJ
Número total de Autores: 7
|
| Tipo de documento: | Artigo Científico |
| Fonte: | ASTRODYNAMICS 2018, PTS I-IV; v. 130, p. 2-pg., 2008-01-01. |
| Resumo | |
The main target here is to determine the orbit of an artificial satellite, using signals of the GPS constellation and least squares algorithms implemented through sequential Givens rotations as a method of estimation, with the aim of improving the performance of the orbit estimation process and, at the same time, minimizing the computational procedure cost. Geopotential perturbations up to high order and direct solar radiation pressure were taken into account. It was also considered the position of the GPS antenna on the satellite body that, lately, consists of the influence of the satellite attitude motion in the orbit determination process. An application has been done, using real data from the Topex/Poseidon satellite, whose ephemeris is available at Internet. The best accuracy obtained in position was smaller than 5 meters for short period (2 hours) and smaller than 28 meters for long period (24 hours) orbit determination. In both cases, the perturbations mentioned before were taken into consideration and the analysis occurred without selective availability on the signals measurements. (AU) | |
| Processo FAPESP: | 04/11635-8 - Determinacao de orbita via gps considerando modelo de pressao de radiacao solar para o satelite topex/poseidon. |
| Beneficiário: | Paula Cristiane Pinto Mesquita Pardal |
| Modalidade de apoio: | Bolsas no Brasil - Mestrado |