The properties of plasma flows in fine ray structures of the streamer belt

Details The properties of plasma flows in fine ray structures of the streamer belt The properties of plasma flows in fine ray structures of the streamer belt

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..197..101e&link_type=abstract

Solar Physics, v. 197, Issue 1, p. 101-113 (2000).

Physics

6

Scientific paper

We show that within distances from the Sun's surface less than the height of a streamer helmet, each of two neighboring rays of the streamer belt, as they approach the solar surface, bends around the helmet on either side of it. Also, a minimum angular diameter of the rays of d~2°-3° remains virtually constant within R=1.2-6.0 R_solar. A density inhomogeneity (`blob') can be produced above the helmet top visible to at least R~6 R_solar. In this case the initial velocity of the `blob' increases with solar distance from where it is generated to something like the velocity of the bulk solar wind with which the `blob' is carried away.

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