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利用环境等离子体测量校准带电粒子传感器的静电偏转

Calibrating Electrostatic Deflection of Charged Particle Sensors Using Ambient Plasma Measurements.

作者信息

Barrie Alexander C, Schiff Conrad, Gershman Daniel J, Giles Barbara L, Rand David

机构信息

Aurora Engineering Orono ME USA.

NASA Goddard Space Flight Center Greenbelt MD USA.

出版信息

J Geophys Res Space Phys. 2021 Jul;126(7):e2021JA029149. doi: 10.1029/2021JA029149. Epub 2021 Jul 8.

DOI:10.1029/2021JA029149
PMID:35860602
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9285780/
Abstract

As space-based charged particle measurement pushes the technical envelope, resolution, both spatially and temporally, is ever improving. As such, the knowledge of the associated error must also improve. We present a method for correlating data collected from multiple sensors at different times in order to estimate the pointing error of each sensor. The method is demonstrated using flight data from the Dual Ion Spectrometer suite, part of the Fast Plasma Investigation on the NASA's Magnetospheric Multiscale mission. By looking at signals with sharp features in the direction of spacecraft spin, the relative error in look direction between sensors can be estimated with sub-degree precision, roughly 20 times better than the native resolution in the azimuthal (spin) direction. These sharp features appear in nature often enough that a sufficiently large sample size can be identified, using an automated filter of routine science data, to calibrate the system, or post correct measured data. The relative pointing error can then be trended over time to monitor the evolution/aging of the measurement system. These data inform calibration/correction methods, should the error grow to a point where science quality is adversely affected.

摘要

随着天基带电粒子测量不断突破技术极限,空间和时间分辨率都在不断提高。因此,对相关误差的了解也必须不断完善。我们提出了一种方法,用于关联在不同时间从多个传感器收集的数据,以估计每个传感器的指向误差。该方法通过美国国家航空航天局磁层多尺度任务中快速等离子体探测器的双离子光谱仪套件的飞行数据进行了演示。通过观察航天器自旋方向上具有尖锐特征的信号,可以以亚度精度估计传感器之间视向的相对误差,这比方位角(自旋)方向上的原始分辨率大约高20倍。这些尖锐特征在自然界中经常出现,因此可以使用常规科学数据的自动滤波器识别出足够大的样本量,以校准系统或对测量数据进行后期校正。然后,可以随时间推移对相对指向误差进行趋势分析,以监测测量系统的演变/老化情况。如果误差增大到对科学质量产生不利影响的程度,这些数据将为校准/校正方法提供依据。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/26c70ef14037/JGRA-126-0-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/3a789589d8df/JGRA-126-0-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/1f932cb1876c/JGRA-126-0-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/d4de3cc94848/JGRA-126-0-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/e49f01d11a30/JGRA-126-0-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/6e181534fbaa/JGRA-126-0-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/88b031bcb2fb/JGRA-126-0-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/e7483207ddd6/JGRA-126-0-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/26c70ef14037/JGRA-126-0-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/3a789589d8df/JGRA-126-0-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/1f932cb1876c/JGRA-126-0-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/d4de3cc94848/JGRA-126-0-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/e49f01d11a30/JGRA-126-0-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/6e181534fbaa/JGRA-126-0-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/88b031bcb2fb/JGRA-126-0-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/e7483207ddd6/JGRA-126-0-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cee5/9285780/26c70ef14037/JGRA-126-0-g004.jpg

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