Method for the Identification of Heliospheric Anomalies Based on the Functions of the Characteristic Deviations for the Observation Matrices of the Muon Hodoscope
- Авторы: Chinkin V.E.1,2, Astapov I.I.2,3, Gvishiani A.D.2,4, Getmanov V.G.2,4, Dmitrieva A.N.2,3, Dobrovolsky M.N.2, Kovylyaeva A.A.2,3, Sidorov R.V.2, Soloviev A.A.2,4, Yashin I.I.2,3
-
Учреждения:
- Bauman Moscow State Technical University (BMSTU)
- Geophysical Center of the Russian Academy of Sciences (GC RAS)
- National Research Nuclear University MEPhI (NRNU MEPhI)
- Schmidt Institute of Physics of the Earth of the Russian Academy of Sciences (IPE RAS)
- Выпуск: Том 82, № 6 (2019)
- Страницы: 924-928
- Раздел: Elementary Particles and Fields
- URL: https://journals.rcsi.science/1063-7788/article/view/195479
- DOI: https://doi.org/10.1134/S106377881966013X
- ID: 195479
Цитировать
Аннотация
This paper presents a method for identifying heliospheric anomalies using the introduced function of characteristic deviations for the muon hodoscope matrices. The estimation of the averaged hardware function is considered. Spatial filtering is proposed to eliminate fluctuations in the functions of the characteristic deviations. An example of the implementation of the developed method using the example of the storm July 13, 2017. It is shown that for this event, the identified anomaly precedes by several hours a sharp increase in the Kp index.
Об авторах
V. Chinkin
Bauman Moscow State Technical University (BMSTU); Geophysical Center of the Russian Academy of Sciences (GC RAS)
Автор, ответственный за переписку.
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
I. Astapov
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
A. Gvishiani
Geophysical Center of the Russian Academy of Sciences (GC RAS); Schmidt Institute of Physics of the Earth of the Russian Academy of Sciences (IPE RAS)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
V. Getmanov
Geophysical Center of the Russian Academy of Sciences (GC RAS); Schmidt Institute of Physics of the Earth of the Russian Academy of Sciences (IPE RAS)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
A. Dmitrieva
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
M. Dobrovolsky
Geophysical Center of the Russian Academy of Sciences (GC RAS)
Email: v.chinkin@gcras.ru
Россия, Moscow
A. Kovylyaeva
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
R. Sidorov
Geophysical Center of the Russian Academy of Sciences (GC RAS)
Email: v.chinkin@gcras.ru
Россия, Moscow
A. Soloviev
Geophysical Center of the Russian Academy of Sciences (GC RAS); Schmidt Institute of Physics of the Earth of the Russian Academy of Sciences (IPE RAS)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
I. Yashin
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Россия, Moscow; Moscow
Дополнительные файлы
