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Shorting Factor In-Flight Calibration for the Van Allen Probes DC Electric Field Measurements in the Earth’s Plasmasphere

机译:在地球等离子层中对Van Allen探针进行直流电场测量的空程因子飞行中校准

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摘要

Satellite-based direct electric field measurements deliver crucial information for space science studies. Yet, they require meticulous design and calibration. In-flight calibration of double-probe instruments is usually presented in the most common case of tenuous plasmas, where the presence of an electrostatic structure surrounding the charged spacecraft alters the geophysical electric field measurements. To account for this effect and the uncertainty in the boom length, the measured electric field is multiplied by a parameter called the shorting factor (sf ). In the plasmasphere, the Debye length is very small in comparison with spacecraft dimension and there is no shorting of the electric field measurements (sf = 1). However, the electric field induced by spacecraft motion greatly exceeds any geophysical electric field of interest in the plasmasphere. Thus, the highest level of accuracy in calibration is required.The objective of this work is to discuss the accuracy of the setting Sf =1 and therefore to examine the accuracy of Van Allen Probes electric field measurements below L = 2. We introduce a method to determine the shorting factor near perigee. It relies on the idea that the value of the geophysical electric field measured in the Earth’s rotating frame of reference is independent of whether the spacecraft is approaching perigee or past perigee, i.e. it is independent of spacecraft velocity. We obtain that Sf =0.994 ± 0.001. The resulting margins of errors in individual electric drift measurements are of the order of ± 0.1% of spacecraft velocity (a few meters per second).
机译:基于卫星的直接电场测量为太空科学研究提供了关键信息。但是,它们需要精心设计和校准。双探针仪器的飞行中校准通常是在等离子体最常见的情况下进行的,其中带电航天器周围的静电结构的存在会改变地球物理电场的测量值。为了考虑到这种影响和动臂长度的不确定性,将测得的电场乘以一个称为短路系数(sf)的参数。在等离子层中,与航天器尺寸相比,德拜长度非常小,并且不会缩短电场测量值(sf = 1)。但是,由航天器运动引起的电场大大超过了等离子层中任何感兴趣的地球物理电场。因此,需要在校准中达到最高的精确度。这项工作的目的是讨论设置Sf = 1的精确度,并因此检验L = 2以下的Van Allen Probes电场测量的精确度。我们介绍一种方法确定近地点的短路因素。它依赖于这样一种想法,即在地球旋转参考系中测得的地球物理电场的值与航天器是接近近地点还是过去近地点无关,也就是说,它与航天器速度无关。我们获得Sf = 0.994±0.001。每次电漂移测量中所产生的误差幅度约为航天器速度的±0.1%(每秒几米)。

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  • 期刊名称 other
  • 作者

    Solène Lejosne; F. S. Mozer;

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  • 年(卷),期 -1(6),4
  • 年度 -1
  • 页码 646–654
  • 总页数 16
  • 原文格式 PDF
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