Determination of the accelerometer metrological characteristics on board the METRIC mission

A. Valmorbida, G. Anese, R. Peron, E. Lorenzini
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Abstract

METRIC is a proposed mission that aims to improve the knowledge of atmospheric density, general relativity and geodesy. The mission foresees a small spherical satellite placed in a polar eccentric orbit, with the apogee at 1200 km of altitude and perigee at 400–450 km. The spacecraft will be tracked from ground and space and have an on-board 3-axis accelerometer. The accelerometer will measure non-gravitational accelerations (due mainly to neutral drag and solar radiation pressure). A dynamical simulator has been implemented with known models (e.g. higher-harmonics gravity field, upper atmosphere density, solar pressure) in order to estimate the non-gravitational accelerations acting on the satellite. These are then analyzed in order to extract their main characteristics: intensity and frequency spectrum. Consequently, an envelope for the accelerometer features - dynamic range, required accuracy and frequency bandwidth - can be set. The data collected by the accelerometer will be used, in combination with tracking data from GNSS and SLR, to improve the atmospheric density knowledge over a wide range of altitudes, to perform an accurate measurement of the orbital precessions predicted by general relativity and implement a space-based tie of geodetic reference frames.
米制任务上加速度计计量特性的测定
METRIC是一个被提议的任务,旨在提高对大气密度、广义相对论和大地测量学的认识。该任务预计将在极地偏心轨道上放置一颗小型球形卫星,远地点高度为1200公里,近地点高度为400-450公里。该航天器将从地面和太空进行跟踪,并有一个机载三轴加速度计。加速度计将测量非重力加速度(主要是由于中性阻力和太阳辐射压力)。利用已知的模型(如高次重力场、高层大气密度、太阳压力)实现了一个动态模拟器,以估计作用在卫星上的非重力加速度。然后对它们进行分析,以提取它们的主要特征:强度和频谱。因此,可以设置加速度计特性的包络线——动态范围、所需精度和频率带宽。加速度计收集的数据将与GNSS和SLR的跟踪数据结合使用,以提高在大高度范围内的大气密度知识,对广义相对论预测的轨道进动进行精确测量,并实现基于空间的大地测量参考框架。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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