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...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
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
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	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. In this work, features of the investigation of coronal mass ejections that are detected in the muon flux by the ground-based URAGAN muon hodoscope operating as a part of the Experimental complex NEVOD at the Moscow Engineering Physics Institute are discussed. Results of studying the anisotropy of the cosmic ray muon flux during the CMEs of 2016 are presented.
ISSN:	1063-7788 1562-692X
DOI:	10.1134/S106377881809003X