Open AccessInvestigation of local deformations of muon flux angular distribution during CME with GSE-mapping technique
Author(s) -
И. И. Астапов,
N. S. Barbashina,
А. Н. Дмитриева,
I. A. Melnikova,
N. V. Osetrova,
В. В. Шутенко,
I. I. Yashin
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1390/1/012067
Subject(s) - hodoscope , physics , muon , cosmic ray , flux (metallurgy) , heliosphere , coronal mass ejection , angular resolution (graph drawing) , matrix (chemical analysis) , astrophysics , nuclear physics , solar wind , materials science , plasma , mathematics , combinatorics , metallurgy , composite material
Coronal mass ejections (CME) have an impact on the flux of cosmic rays that penetrate the disturbed areas in the heliosphere and the near-terrestrial space. Unlike most ground-based cosmic ray detectors, the URAGAN muon hodoscope (MEPhI) allows to investigate both the integrated counting rate of registered particles and angular characteristics of the muon flux at the ground level. To select the local areas with statistically significant intensity changes, the angular distributions for the last hour and preceding it 24 hours corrected for the barometric effect are used. Angular distributions are smoothed, and the matrix of relative changes of the angular distribution in units of statistical errors is formed. The use of asymptotic directions calculated in advance, the angular cells of the matrix are mapped from the local coordinate system to the GSE coordinate system. The results of the study of GSE-mapping of local deformations of the angular distributions for different types of CMEs are discussed.