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Relatively stable, large-amplitude Alfvenic waves seen at 2.5 and 5.0 AUPioneer 11 and 10 observations of the wave structure seen in a corotating interaction region at 2.5 AU on day 284 of 1973 and 8 days later at 5 AU reveal large-amplitude Alfvenic structures with many detailed correlations seen between their features at the two radial distances. Hodogram analysis suggests the dominance of near plane polarized, transverse Alfvenic mode fluctuations with periods between 2 min and one hour or more. Some wave evolution close to the Corotating Interaction Region (CIR) shock is noticed, but waves towards the center of the compression seem to propagate with little damping between the spacecraft observation positions.
Document ID
19890031684
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mavromichalaki, H.
(Athens Univ. Greece)
Moussas, X.
(Athens, National University Greece)
Quenby, J. J.
(Imperial College of Science and Technology London, United Kingdom)
Valdes-Galicia, J. F.
(Universidad Nacional Autonoma de Mexico Coyoacan, Mexico)
Smith, E. J.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Publication Information
Publication: Solar Physics
Volume: 116
Issue: 2, 19
ISSN: 0038-0938
Subject Category
Astrophysics
Accession Number
89A19055
Distribution Limits
Public
Copyright
Other

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