Remote Sensing (Jul 2022)

Hybrid Electrostatic–Atomic Accelerometer for Future Space Gravity Missions

  • Nassim Zahzam,
  • Bruno Christophe,
  • Vincent Lebat,
  • Emilie Hardy,
  • Phuong-Anh Huynh,
  • Noémie Marquet,
  • Cédric Blanchard,
  • Yannick Bidel,
  • Alexandre Bresson,
  • Petro Abrykosov,
  • Thomas Gruber,
  • Roland Pail,
  • Ilias Daras,
  • Olivier Carraz

DOI
https://doi.org/10.3390/rs14143273
Journal volume & issue
Vol. 14, no. 14
p. 3273

Abstract

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Long-term observation of Earth’s temporal gravity field with enhanced temporal and spatial resolution is a major objective for future satellite gravity missions. Improving the performance of the accelerometers present in such missions is one of the main paths to explore. In this context, we propose to study an original concept of a hybrid accelerometer associating a state-of-the-art electrostatic accelerometer (EA) and a promising quantum sensor based on cold atom interferometry. To assess the performance potential of such an instrument, numerical simulations were performed to determine its impact in terms of gravity field retrieval. Taking advantage of the long-term stability of the cold atom interferometer (CAI), it is shown that the reduced drift of the hybrid sensor could lead to improved gravity field retrieval. Nevertheless, this gain vanishes once temporal variations of the gravity field and related aliasing effects are taken into account. Improved de-aliasing models or some specific satellite constellations are then required to maximize the impact of the accelerometer performance gain. To evaluate the achievable acceleration performance in-orbit, a numerical simulator of the hybrid accelerometer was developed and preliminary results are given. The instrument simulator was in part validated by reproducing the performance achieved with a hybrid lab prototype operating on the ground. The problem of satellite rotation impact on the CAI was also investigated both with instrument performance simulations and experimental demonstrations. It is shown that the proposed configuration, where the EA’s proof-mass acts as the reference mirror for the CAI, seems a promising approach to allow the mitigation of satellite rotation. To evaluate the feasibility of such an instrument for space applications, a preliminary design is elaborated along with a preliminary error, mass, volume, and electrical power consumption budget.

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