On the three-dimensional nature of the modulation of galactic cosmic rays

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DOIResolve DOI: http://doi.org/10.1029/JA085iA12p06893
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TypeArticle
Journal titleJournal of Geophysical Research: Space Physics
ISSN0148-0227
Volume85
IssueA12
Pages68936894; # of pages: 2
AbstractRecent results, on two different time scales, of the influence of solar polar coronal holes on the galactic cosmic ray intensity appear on the surface to be inconsistent. We show, in the context of present knowledge of the effects of high-speed solar wind streams on energetic particles, that the results are indeed mutually consistent and they support the view that coronal holes are influential in determining the three-dimensional modulation of galactic cosmic rays in the solar system.
Publication date
LanguageEnglish
AffiliationNational Research Council Canada
Peer reviewedYes
NRC number20173
NPARC number21274950
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Record identifier981e9212-d3b3-4dd5-bd78-a37c7c3e916f
Record created2015-05-04
Record modified2016-05-09
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