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A Parametric Model to Reproduce the Background of the Insight-HXMT/HE Blind Detector

  • Authors: Yuan You, Jin-Yuan Liao, Shuang-Nan Zhang, Shu Zhang, Xue-Feng Lu, Juan Zhang, Gang Li, Zhi Chang, Yu-Peng Chen, Ming-Yu Ge, Cheng-Cheng Guo, Rui Huang, Yue Huang, Jing Jin, Xiao-Bo Li, Xu-Fang Li, Zheng-Wei Li, Cong-Zhan Liu, Fang-Jun Lu, Jian-Yin Nie, Li-Ming Song, Si-Fan Wang, Yi-Fei Zhang, and Hai-Sheng Zhao

2021 The Astrophysical Journal Supplement Series 256 47.

  • Provider: AAS Journals

Caption: Figure 8.

Relationship between the proton flux p and intersection angle φ between the direction of the geomagnetic field and the orientation of the satellite in the SAA region according to SEM data. The flux of protons is normalized by their mean flux in the SAA region in each corresponding energy band. This relationship is recorded as a function f(φ).

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