Method for the Identification of Heliospheric Anomalies Based on the Functions of the Characteristic Deviations for the Observation Matrices of the Muon Hodoscope

被引：5

作者：

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
]}

机构：

[1] BMSTU, Moscow, Russia

[2] Russian Acad Sci, Geophys Ctr, Moscow, Russia

[3] NRNU MEPhI, Moscow, Russia

[4] Russian Acad Sci IPE RAS, Schmidt Inst Phys Earth, Moscow, Russia

来源：

PHYSICS OF ATOMIC NUCLEI | 2019年 / 82卷 / 06期

基金：

俄罗斯科学基金会;

关键词：

D O I：

10.1134/S106377881966013X

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

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.

引用

页码：924 / 928

页数：5

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