Sub-Alfvénic flows in the quiet and recurrent solar winds

Details Sub-Alfvénic flows in the quiet and recurrent solar winds Sub-Alfvénic flows in the quiet and recurrent solar winds

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..482z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 4, p. 482-486.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Observed instances are given in this paper to show that
sub-Alfvénic flow can be formed in the quiet and recurrent
low-speed solar wind streams. This kind of flow appears in regions with
abnormal enhancement of Alfvénic speed and is associated with a
specific type of magnetic configuration.

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