A background correction algorithm for Van Allen Probes MagEIS electron flux measurements

被引:92
作者
Claudepierre, S. G. [1 ]
O'Brien, T. P. [1 ]
Blake, J. B. [1 ]
Fennell, J. F. [1 ]
Roeder, J. L. [1 ]
Clemmons, J. H. [1 ]
Looper, M. D. [1 ]
Mazur, J. E. [1 ]
Mulligan, T. M. [1 ]
Spence, H. E. [2 ]
Reeves, G. D. [3 ]
Friedel, R. H. W. [3 ]
Henderson, M. G. [3 ]
Larsen, B. A. [3 ]
机构
[1] Aerosp Corp, Dept Space Sci, El Segundo, CA 90245 USA
[2] Univ New Hampshire, Inst Study Earth Oceans & Space, Durham, NH 03824 USA
[3] Los Alamos Natl Lab, Space & Atmospher Sci Grp, Los Alamos, NM USA
关键词
radiation belt; inner radiation belt; background contamination; spacecraft engineering; outer radiation belt; particle measurements; RELATIVISTIC ELECTRONS; ENERGETIC PARTICLE; RADIATION BELT; ENVIRONMENT;
D O I
10.1002/2015JA021171
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe an automated computer algorithm designed to remove background contamination from the Van Allen Probes Magnetic Electron Ion Spectrometer (MagEIS) electron flux measurements. We provide a detailed description of the algorithm with illustrative examples from on-orbit data. We find two primary sources of background contamination in the MagEIS electron data: inner zone protons and bremsstrahlung X-rays generated by energetic electrons interacting with the spacecraft material. Bremsstrahlung X-rays primarily produce contamination in the lower energy MagEIS electron channels (approximate to 30-500keV) and in regions of geospace where multi-MeV electrons are present. Inner zone protons produce contamination in all MagEIS energy channels at roughly L < 2.5. The background-corrected MagEIS electron data produce a more accurate measurement of the electron radiation belts, as most earlier measurements suffer from unquantifiable and uncorrectable contamination in this harsh region of the near-Earth space environment. These background-corrected data will also be useful for spacecraft engineering purposes, providing ground truth for the near-Earth electron environment and informing the next generation of spacecraft design models (e.g., AE9).
引用
收藏
页码:5703 / 5727
页数:25
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