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Peculiarities of propagation of charged particles in solar coronaThe influence of boundaries of the large scale unipolar magnetic regions (UMR) on the Sun upon the charged particle propagation in the solar corona and interplanetary space is investigated. Increases of the charged particle fluxes from solar flares on November 4 and 20, 1978 detected by Venera-11 and Prognoz-1 and on December 7, 1982 by Venera-13 and "GMS-2" were analyzed.
Document ID
19850026497
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Morozova, E. I. (Academy of Sciences (USSR) Moscow, Ussr)
Pisarenko, N. F. (Academy of Sciences (USSR) Moscow, Ussr)
Mikryukova, N. A. (Academy of Sciences (USSR) Moscow, Ussr)
Klimenko, V. V. (Inst. of Cosmophysical Research and Astronomy)
Timofeev, V. E. (Inst. of Cosmophysical Research and Astronomy)
Shafer, Y. G. (Inst. of Cosmophysical Research and Astronomy)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-3.1-6
Report Number: SH-3.1-6
Accession Number
85N34810
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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