Large-scale structure of the solar plasma corona: an analysis of YOHKOH SXT images

Details Large-scale structure of the solar plasma corona: an analysis of YOHKOH SXT images Large-scale structure of the solar plasma corona: an analysis of YOHKOH SXT images

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ppcn.conf..215s&link_type=abstract

In ESA, Fourth International Toki Conference on Plasma Physics and Controlled Nuclear Fusion p 215-218 (SEE N94-22624 05-75)

Physics

Plasma Physics

Heliosphere, Photosphere, Solar Corona, Solar Flares, Sunspots, X Ray Telescopes, Japanese Space Program, Plasma Dynamics, Solar Atmosphere, Solar Observatories

Scientific paper

The Yohkoh Soft X-ray Telescope (SXT) images are analyzed. The large scale structure of the solar plasma corona is investigated. The clarified characteristics are as follows: preferred position of active regions and its possible mechanism, rules governing the coronal hole channel, a relation between the inner and outer corona, formation of the 4 sector structure, and the outer corona in pseudoaligned phase. These characteristics are in agreement with both the rotational reversing model and the triple dipole model on the structure and dynamics of the heliomagnetosphere.

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