High-speed streams and sector boundaries

Details High-speed streams and sector boundaries High-speed streams and sector boundaries

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976jgr....81.2437s&link_type=abstract

Journal of Geophysical Research, vol. 81, May 1, 1976, p. 2437-2441.

Physics

7

Interplanetary Magnetic Fields, Solar Wind Velocity, Boundaries, Frequency Distribution, Sectors, Solar Rotation, Twenty-Seven Day Variation

Scientific paper

High-speed streams in the solar wind are located with respect to interplanetary magnetic sectors, and their location in the sector is analyzed. The relation to the sector taken as a whole is clearer than the relation to sector boundaries. The streams occur preferentially near the center of the sector. Although high-speed streams, as do sector boundaries, show a clear pattern of recurrence with solar rotation and although they are about equally frequent in the period studied (1965-1971), there is no one-to-one relation between them; sectors with no stream or with more than one stream are common. Longer sectors contain more streams, showing that streams occur at a certain rate per unit time rather than at a constant number per sector.

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