Cosmic ray modulatin and merged interaction regions

dc.contributor.authorBurlaga, L. F.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorMcDonald, F. B.
dc.date.accessioned2023-11-03T14:52:18Z
dc.date.available2023-11-03T14:52:18Z
dc.date.issued1985-08
dc.description19th Intern. Cosmic Ray Conf.en_US
dc.description.abstractBeyond several AU, interactions among shocks and streams give rise to merged interaction regions in which the magnetic field is turbulent. The integral intensity of . 75 MeV/Nuc cosmic rays at Voyager is generally observed to decrease when a merged interaction region moves past the spacecraft and to increase during the passage of a rarefaction region. When the separation between interaction regions is relatively large, the cosmic ray intensity tends to increase on a scale of a few months. This was the case at Voyager 1 from July 1, 1983 to May 1, 1984, when the spacecraft moved from 16.7 to 19.6 AU. Changes in cosmic ray intensity were related to the magnetic field strength in a simple way. It is estimated that the diffusion coefficient in merged interaction regions at this distance is similar to 0.6 x 10 to the 22nd power sq cm/s.en_US
dc.description.urihttps://ui.adsabs.harvard.edu/abs/1985ICRC....4..396B/abstracten_US
dc.format.extent4 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.identifierdoi:10.13016/m2vpun-fvra
dc.identifier.citationBurlaga, L. F., M. L. Goldstein, and F. B. McDonald. “Cosmic Ray Modulatin and Merged Interaction Regions” 19th Intern. Cosmic Ray Conf. 4 (August 1, 1985): 396–99. https://ui.adsabs.harvard.edu/abs/1985ICRC....4..396B/abstract.en_US
dc.identifier.urihttp://hdl.handle.net/11603/30529
dc.language.isoen_USen_US
dc.publisherNASAen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis is a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleCosmic ray modulatin and merged interaction regionsen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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