Physics
Scientific paper
Apr 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52...91m&link_type=abstract
Solar Physics, vol. 52, Apr. 1977, p. 91-100.
Physics
3
Force-Free Magnetic Fields, Magnetic Field Configurations, Solar Corona, Solar Magnetic Field, Solar X-Rays, Lines Of Force, Magnetic Flux, Solar Rotation
Scientific paper
A large long-lived soft X-ray emitting arch system was observed during the last Skylab mission. This arcade stayed in the same approximate position for several solar rotations. It is suggested that these long-lived arches owe their stability to the stable coronal magnetic-field configuration. A global constant-alpha force-free magnetic-field analysis, as developed by Nakagawa et al. (1977), is used to describe the arches, and results in a marked resemblance between the theoretical magnetic-field configuration and the observed X-ray emitting feature.
Krall K. R.
McGuire James P. Jr.
Smith Jeffrey B.
Speich David M.
Tandberg-Hanssen Einar
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