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MICROSCOPE: systematic errors

delete2022-09-07
delete8
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OA
AI
M
Manuel Rodrigues *
P
Pierre Touboul
A
Alain Robert
O
Océane Dhuicque
J
Joël Bergé
D
Damien Boulanger
R
Ratana Chhun
B
Bruno Christophe
V
Valerio Cipolla
B
Bernard Foulon
P
Pierre-Yves Guidotti
É
Émilie Hardy
P
Phuong-Anh Huynh
V
Vincent Lebat
B
Benjamin Pouilloux
P
Pascal Prieur
S
Serge Reynaud
P
Patrizia Torresi
DOI:10.1088/1361-6382/ac49f6delete
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摘要

摘要

En 中文
The MICROSCOPE mission aims to test the weak equivalence principle (WEP) in orbit with an unprecedented precision of 10(-15) on the Eotvos parameter thanks to electrostatic accelerometers on board a drag-free micro-satellite. The precision of the test is determined by statistical errors, due to the environment and instrument noises, and by systematic errors to which this paper is devoted. Systematic error sources can be divided into three categories: external perturbations, such as the residual atmospheric drag or the gravity gradient at the satellite altitude, perturbations linked to the satellite design, such as thermal or magnetic perturbations, and perturbations from the instrument internal sources. Each systematic error is evaluated or bounded in order to set a reliable upper bound on the WEP parameter estimation uncertainty.
Keyword:
MICROSCOPE
electrostatic accelerometer
in-orbit calibration
drag-free
microsatellite
thermal perturbation
magnetic perturbation

期刊

Classical and Quantum Gravity 封面图
Classical and Quantum Gravity
IF:
3.7
论文数:
1.3W
被引数:
3.0W

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O
observatoire de la cote d'azur
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2.4K
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N
national office for aerospace studies & research (onera)
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1.9K
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U
Universite Paris Saclay
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7.3W
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