The Solar Corona - Flat Formation

Details The Solar Corona - Flat Formation The Solar Corona - Flat Formation

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..142..213g&link_type=abstract

Solar Physics, Volume 142, Issue 1, pp.213-216

Physics

12

Scientific paper

During the greater part of the 11-year sunspot cycle the solar corona represents largely a similar flat formation as in the minimum (looking like a galaxy), The observed variety of coronal forms is mainly due to variations of the corona's orientation as seen from the Earth. Two limiting cases of coronal orientation are discussed: perpendicular to the plane of the sky (‘edgewise’ towards the observer) and parallel with the plane of the sky. The first case is illustrated with the coronal observations of 11 July, 1991. The second case provides an opportunity to observe the corona from above the solar magnetic poles.

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