Evidence for magnetic energy storage in coronal active regions

Details Evidence for magnetic energy storage in coronal active regions Evidence for magnetic energy storage in coronal active regions

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...47..117k&link_type=abstract

(NASA, IAU, IUGG, and International Council of Scientific Unions, Workshop on Flare Build-up Study, Falmouth, Mass., Sept. 8-11,

Astronomy and Astrophysics

Astronomy

15

Photosphere, Skylab Program, Solar Corona, Solar Magnetic Field, Solar X-Rays, Spaceborne Astronomy, Extrapolation, Solar Atmosphere, X Ray Spectroscopy, X Ray Telescopes

Scientific paper

Examination of X-ray images obtained by the S-054 X-ray spectrographic telescope on Skylab shows the presence of some atypical X-ray-emitting coronal structures in active regions which are not consistent with potential extrapolations of photospheric magnetic fields. Analysis of the observed temporal changes in the X-ray-emitting active-region structures demonstrates that the majority of these consist of brightness changes representing temperature (and perhaps density) variations of the material in the loops.

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