Email this article Method for the Identification of Heliospheric Anomalies Based on the Functions of the Characteristic Deviations for the Observation Matrices of the Muon Hodoscope
- Authors: 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
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Affiliations:
- 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)
- Issue: Vol 82, No 6 (2019)
- Pages: 924-928
- Section: Elementary Particles and Fields
- URL: https://journal-vniispk.ru/1063-7788/article/view/195479
- DOI: https://doi.org/10.1134/S106377881966013X
- ID: 195479
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Abstract
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.
About the authors
V. E. Chinkin
Bauman Moscow State Technical University (BMSTU); Geophysical Center of the Russian Academy of Sciences (GC RAS)
Author for correspondence.
Email: v.chinkin@gcras.ru
Russian Federation, Moscow; Moscow
I. I. Astapov
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow; Moscow
A. D. 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
Russian Federation, Moscow; Moscow
V. G. 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
Russian Federation, Moscow; Moscow
A. N. Dmitrieva
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow; Moscow
M. N. Dobrovolsky
Geophysical Center of the Russian Academy of Sciences (GC RAS)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow
A. A. Kovylyaeva
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow; Moscow
R. V. Sidorov
Geophysical Center of the Russian Academy of Sciences (GC RAS)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow
A. 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
Russian Federation, Moscow; Moscow
I. I. Yashin
Geophysical Center of the Russian Academy of Sciences (GC RAS); National Research Nuclear University MEPhI (NRNU MEPhI)
Email: v.chinkin@gcras.ru
Russian Federation, Moscow; Moscow
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