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Coronal holes, solar diurnal anisotropy of cosmic rays and off-ecliptic interplanetary magnetic fieldsThe information regarding the electromagnetic states of the interplanetary medium, derived from the analyses of the cosmic ray intensity variations observed with a global network of cosmic ray detectors such as neutron monitors and muon telescopes, is reviewed. The relation of the temporal characteristics of the cosmic ray solar diurnal anisotropy to the large scale characteristics of the interplanetary magnetic field, far away from the ecliptic plane, is addressed. A model for the phenomenon is described.
Document ID
19800009705
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ahluwalia, H. S.
(New Mexico Univ. Albuquerque, NM, United States)
Date Acquired
August 10, 2013
Publication Date
February 1, 1980
Publication Information
Publication: NASA. Goddard Space Flight Center Study of the Solar Cycle from Space
Subject Category
Solar Physics
Accession Number
80N17967
Funding Number(s)
CONTRACT_GRANT: NSF ATM-78-10727
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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