Geomagnetism and Aeronomy ( IF 0.7 ) Pub Date : 2020-10-22 , DOI: 10.1134/s0016793220050072 E. A. Ginzburg , A. A. Krivolutsky , A. A. Kukoleva , I. N. Myagkova
Abstract—
The results of a comparative analysis of the fluxes and spectra of solar protons measured in September 2017 by satellites at different orbits (ELECTRO-L No. 2, GOES 13, and METEOR-3 No. 2) and the results of modeling of the ionization rate in the polar atmosphere based on data from these experiments are presented. It is found based on data from Russian and US satellites that the proton spectra are sufficiently close to each other and are exponential. Calculations of the ionization rate in the polar atmosphere based on data from the three experiments showed close results, except for those at low altitudes.
中文翻译:
质子事件期间极地大气中的电离率的计算
摘要—
2017年9月由不同轨道的卫星(ELECTRO-L 2号,GOES 13和METEOR-3 2号)测量的太阳质子通量和光谱的比较分析结果和电离建模结果根据这些实验的数据,给出了极地大气中的速率。根据俄罗斯和美国卫星的数据发现,质子谱彼此足够接近且呈指数关系。根据来自三个实验的数据计算出的极地大气中的电离速率显示出接近的结果,除了低海拔地区的结果。