Physical conditions in the corona for a bipolar magnetic region

Details Physical conditions in the corona for a bipolar magnetic region Physical conditions in the corona for a bipolar magnetic region

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57..297v&link_type=abstract

Solar Physics, vol. 57, Apr. 1978, p. 297-308.

Astronomy and Astrophysics

Astronomy

4

Magnetic Field Configurations, Magnetic Flux, Solar Corona, Solar Magnetic Field, Solar Temperature, X Ray Astronomy, Lines Of Force, Photosphere, Skylab Program, Solar Activity, Solar X-Rays, X Ray Imagery

Scientific paper

The S-056 X-ray data from Skylab are used to determine quantitative values for the coronal conditions characterizing a new bipolar magnetic region (BMR). In particular, the analysis includes: (1) the time variation of the total soft X-ray flux from the BMR as a function of time; (2) the temporal and spatial variation of the temperature and emission measure; (3) the variation with time of thermal energy density; (4) the (calculated) magnetic-field configuration and magnetic flux density in the corona; and (5) the temporal variation of the magnetic-field energy in the corona. Detailed comparisons are made between the configuration of X-ray features and the magnetic-field topology.

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