Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016

Coronal mass ejections (CMEs) are the brightest manifestations of solar activity. During periods of higher solar activity, dozens of ejections are observed daily and affect cosmic ray fluxes in interplanetary space. Observation of CMEs is usually carried out by means of various satellite apparatuses...

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Veröffentlicht in:	Physics of atomic nuclei 2018-12, Vol.81 (9), p.1370-1373
Hauptverfasser:	Astapov, I. I., Barbashina, N. S., Bogoutdinov, Sh. R., Borog, V. V., Veselovsky, I. S., Getmanov, V. G., Gvishiani, A. D., Dmitrieva, A. N., Mishutina, Yu. N., Osetrova, N. V., Petrukhin, A. A., Sidorov, R. V., Solov’ev, A. A., Shutenko, V. V., Yashin, I. I.
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy Coronal mass ejection Cosmic rays Detection equipment Fluxes Interaction of Plasma Interplanetary space Muons Particle and Nuclear Physics Particle Beams Physics Physics and Astronomy Radiation with Matter Satellites Solar activity Solar corona
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