Solar Activity and Cosmic Ray Variations in September 2017


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The results are presented from an analysis of data on solar activity and cosmic ray variations observed in September 2017. This period is characterized by a sharp increase in the solar flare activity in the active region AR 12673 during the late descending phase of the 24th solar activity cycle. Solar protons are recorded by the particle instruments aboard the GOES-13 satellite, in the atmosphere, and by the ground-based neutron monitor network. A moderate Forbush decrease in the cosmic ray flux during September 6–10 is also recorded by a number of neutron monitors. Several solar proton energy spectra during September 10, 2017, (GLE72 event) are evaluated using the results from satellite measurements, balloon observations, and neutron monitor records.

作者简介

V. Makhmutov

Lebedev Physical Institute, Russian Academy of Sciences

编辑信件的主要联系方式.
Email: makhmutv@sci.lebedev.ru
俄罗斯联邦, Moscow, 119333

G. Bazilevskaya

Lebedev Physical Institute, Russian Academy of Sciences

Email: makhmutv@sci.lebedev.ru
俄罗斯联邦, Moscow, 119333

Y. Stozhkov

Lebedev Physical Institute, Russian Academy of Sciences

Email: makhmutv@sci.lebedev.ru
俄罗斯联邦, Moscow, 119333

M. Philippov

Lebedev Physical Institute, Russian Academy of Sciences

Email: makhmutv@sci.lebedev.ru
俄罗斯联邦, Moscow, 119333

E. Kalinin

Lebedev Physical Institute, Russian Academy of Sciences

Email: makhmutv@sci.lebedev.ru
俄罗斯联邦, Moscow, 119333

A. Morzabaev

Gumilyov Eurasian National University

Email: makhmutv@sci.lebedev.ru
哈萨克斯坦, Astana, 010000

V. Erkhov

Gumilyov Eurasian National University

Email: makhmutv@sci.lebedev.ru
哈萨克斯坦, Astana, 010000

S. Giniyatova

Gumilyov Eurasian National University

Email: makhmutv@sci.lebedev.ru
哈萨克斯坦, Astana, 010000

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