Analysis of the anisotropy of the muon flux, according to data obtained by the URAGAN muon hodoscope during heliospheric disturbances. Bulletin of the Russian Academy of Sciences: Physics Volume 77, Issue 5, May 2013, Pages 529-531
14 сентября 2018
209
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| Вид публикации | Статья |
| Контактные данные автора публикации | Astapov, I.I. , Barbashina, N.S., Dmitrieva, A.N., Mishutina, Yu.N., Petrukhin, A.A., Shutenko, V.V., Yakovleva, E.I., Yashin, I.I. National Research Nuclear University MEPhI |
| Ссылка на публикацию в интернете | www.scopus.com/record/display.url?origin=recordpage&eid=2-s2.0-84879112819&citeCnt=29&noHighlight=false&sort=plf-f&src=s&st1=MEPhI&nlo=&nlr=&nls=&sid=F0743CC1BB1CEC168410A18CB87C48A7.Vdktg6RVtMfaQJ4pNTCQ:20&sot=b&sdt=b&sl=31&s=AFFIL(MEPhI) AND PUB |
Аннотация
Features of studying heliospheric disturbances caused by changes in the parameters of the interplanetary magnetic field by the anisotropy of the muon flux of cosmic rays detected on the surface of the Earth by the URAGAN muon hodoscope are considered. The anisotropy of the muon flux in the period 2007-2011 is analyzed. The forecasting potential of our approaches to studying heliospheric disturbances using the penetrating component of cosmic rays is evaluated. © 2013 Allerton Press, Inc.
Indexed keywords
Interplanetary magnetic fields; Muon flux; Muon hodoscopes
Indexed keywords
Interplanetary magnetic fields; Muon flux; Muon hodoscopes
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