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Change of cosmic ray anisotropy with solar activityMuon telescope data at various depths underground in Yakutsk within energy range 10 to 300 GeV for 1957 to 1984 are analyzed. The 22-year variation of the interplanetary magnetic field aligned component is found. The variation is caused by interaction of heliomagnetosphere with the local galactic field and interstellar wind.
Document ID
19850026724
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kravtsov, N. G. (Academy of Sciences (USSR) Yakutsk, Ussr)
Krivoshapkin, P. A. (Academy of Sciences (USSR) Yakutsk, Ussr)
Kuzmin, A. I. (Academy of Sciences (USSR) Yakutsk, Ussr)
Skripin, G. V. (Academy of Sciences (USSR) Yakutsk, Ussr)
Transky, I. A. (Academy of Sciences (USSR) Yakutsk, Ussr)
Shafer, G. V. (Academy of Sciences (USSR) Yakutsk, Ussr)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 5
Subject Category
Space Radiation
Report/Patent Number
SH-4.5-20
Report Number: SH-4.5-20
Accession Number
85N35037
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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