The transition region and corona associated with sunspots

Details The transition region and corona associated with sunspots The transition region and corona associated with sunspots

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...28..423o&link_type=abstract

(International Astronomical Union, Joint Meeting on MHD of Sunspots, Montreal, Canada, Aug. 20, 1979.) Space Science Reviews, vo

Astronomy and Astrophysics

Astronomy

7

Chromosphere, Coronal Loops, Magnetic Flux, Solar Corona, Stellar Evolution, Sunspots, Dynamic Models, Extreme Ultraviolet Radiation, Magnetohydrodynamic Stability, Mass Transfer, Plasma Diagnostics, Solar X-Rays

Scientific paper

It is noted that thus far no structure has been identified immediately above the chromosphere in sunspots that is invariably present and that thus might be called the transition region and corona over the spot. However, the magnetic flux tubes emerging from spots give rise to many of the plasma filled loops that characterize the active region corona. These emit strongly from ions typical of the transition region, or the corona, but seldom both simultaneously. An overview is given of the morphology, evolution, and theory of these structures.

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