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Radial evolution of interaction regionsNear and outside 1 AU, corotating interaction regions bounded by shocks form at the leading edges of high-speed streams. This paper describes the radial evolution of interaction regions, the merging of interaction regions belonging to neighboring streams, and the coalescence of interaction regions belonging to successive solar rotations.
Document ID
19910070461
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Whang, Y. C. (Catholic University of America, Washington, DC, United States)
Burlaga, L. F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Astrophysics
Accession Number
91A55084
Funding Number(s)
CONTRACT_GRANT: NSF ATM-86-14990
CONTRACT_GRANT: NAGW-1595
Distribution Limits
Public
Copyright
Other

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