Solar Wind: Corotating Interaction Regions

Details Solar Wind: Corotating Interaction Regions Solar Wind: Corotating Interaction Regions

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2311k&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2311. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Heliosphere And Cosmic Rays

Scientific paper

For several years around each solar activity minimum corotating interaction regions are the dominant and most extensive feature in the heliosphere except for the termination shock. At this time the solar atmosphere shows a well developed and long-lasting stable structure of polar CORONAL HOLES, often extending far down to low latitudes, and a well-developed narrow streamer belt region encircling ...

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