Multiple heliospheric current sheets and coronal streamer belt dynamics

Details Multiple heliospheric current sheets and coronal streamer belt dynamics Multiple heliospheric current sheets and coronal streamer belt dynamics

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.9371c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A6, p. 9371-9381.

Physics

100

Current Sheets, Heliosphere, Solar Corona, Solar Magnetic Field, Plasma Sheaths, Solar Cycles

Scientific paper

The occurrence of multiple directional discontinuities in the coronal streamer belt at sector boundary crossings in the heliosphere, often ascribed to waves or kinks in the heliospheric current sheet, may alternatively be attributed to a network of extended current sheets from multiple helmet streamers with a hierarchy of sizes at the base of the corona. Frequent transient outflows from these helmets can account for a variety of signatures observed at sector boundaries, including ordered field rotations, planar magnetic structures and sandwichlike plasma structure.

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