MICROSCOPE mission: statistics and impact of glitches on the test of the weak equivalence principle $^{*}$
- Others:
- DPHY, ONERA, Université Paris Saclay [Châtillon] ; ONERA-Université Paris-Saclay
- NASA Goddard Space Flight Center (GSFC)
- Centre National d'Études Spatiales [Toulouse] (CNES)
- Géoazur (GEOAZUR 7329) ; Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Sud])
Description
MICROSCOPE's space test of the weak equivalence principle (WEP) is based on the minute measurement of the difference of accelerations experienced by two test masses as they orbit the Earth. A detection of a violation of the WEP would appear at a well-known frequency f$_{EP}$ depending on the satellite's orbital and spinning frequencies. Consequently, the experiment was optimised to minimise systematic errors at f$_{EP}$. Glitches are short-lived events visible in the test masses' measured acceleration, most likely originating in cracks of the satellite's coating. In this paper, we characterise their shape and time distribution. Although intrinsically random, their time of arrival distribution is modulated by the orbital and spinning periods. They have an impact on the WEP test that must be quantified. However, the data available prevents us from unequivocally tackling this task. We show that glitches affect the test of the WEP, up to an a priori unknown level. Discarding the perturbed data is thus the best way to reduce their effect.
Abstract
International audience
Additional details
- URL
- https://hal.archives-ouvertes.fr/hal-03107980
- URN
- urn:oai:HAL:hal-03107980v1
- Origin repository
- UNICA