Accuracy of meteor positioning from space - and ground-based observations
Accuracy of meteor positioning from space - and ground-based observations
Aims. The knowledge of the orbits and origins derived from meteors is important for the study of meteoroids and of the early solar system. With an increase in nano-satellite projects dedicated to Earth observations or directly to meteor observations (e.g., the Meteorix CubeSat), we investigate the stereoscopic measurement of meteor positions using a pair of cameras, one deployed in space and one on the ground, and aim to understand the accuracy and the main driving factors. This study will reveal the requirements for system setups and the geometry favorable for meteor triangulation. Methods. This Letter presents the principle of the stereoscopic measurement from space and the ground, and an error analysis. Specifically, the impacts of the resolutions of the cameras, the attitude and orbit determination accuracy of the satellite, and the geometry formed by the moving target and observers are investigated. Results. To reach a desirable positioning accuracy of 1 km it is necessary to equip the satellite with high-accuracy sensors (e.g., star tracker and GPS receiver) to perform fine attitude and orbit determination. The best accuracy can occur when the target is at an elevation of 30° with respect to the ground station.
Meteorites, Meteoroids, Meteors, Methods: analytical, Space vehicles, Techniques: photometric
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Rambaux, Nicolas
dbc7fcc9-fe7a-4f22-9288-de9eeabf14e2
Vaubaillon, Jeremie
af4820e9-70d5-4773-9d76-4067fce125d4
9 October 2020
Chen, Hongru
8286469d-afe1-46e5-b107-694017de4d97
Rambaux, Nicolas
dbc7fcc9-fe7a-4f22-9288-de9eeabf14e2
Vaubaillon, Jeremie
af4820e9-70d5-4773-9d76-4067fce125d4
Chen, Hongru, Rambaux, Nicolas and Vaubaillon, Jeremie
(2020)
Accuracy of meteor positioning from space - and ground-based observations.
Astronomy and Astrophysics, 642, [L11].
(doi:10.1051/0004-6361/202039014).
Abstract
Aims. The knowledge of the orbits and origins derived from meteors is important for the study of meteoroids and of the early solar system. With an increase in nano-satellite projects dedicated to Earth observations or directly to meteor observations (e.g., the Meteorix CubeSat), we investigate the stereoscopic measurement of meteor positions using a pair of cameras, one deployed in space and one on the ground, and aim to understand the accuracy and the main driving factors. This study will reveal the requirements for system setups and the geometry favorable for meteor triangulation. Methods. This Letter presents the principle of the stereoscopic measurement from space and the ground, and an error analysis. Specifically, the impacts of the resolutions of the cameras, the attitude and orbit determination accuracy of the satellite, and the geometry formed by the moving target and observers are investigated. Results. To reach a desirable positioning accuracy of 1 km it is necessary to equip the satellite with high-accuracy sensors (e.g., star tracker and GPS receiver) to perform fine attitude and orbit determination. The best accuracy can occur when the target is at an elevation of 30° with respect to the ground station.
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Published date: 9 October 2020
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Publisher Copyright:
© H. Chen et al. 2020.
Keywords:
Meteorites, Meteoroids, Meteors, Methods: analytical, Space vehicles, Techniques: photometric
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Local EPrints ID: 490741
URI: http://eprints.soton.ac.uk/id/eprint/490741
ISSN: 0004-6361
PURE UUID: 1e96b77a-df1d-4621-a85e-3b1c94570ea8
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Date deposited: 04 Jun 2024 17:09
Last modified: 05 Jun 2024 02:10
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Author:
Hongru Chen
Author:
Nicolas Rambaux
Author:
Jeremie Vaubaillon
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