XUV observations of coronal magnetic fields

Details XUV observations of coronal magnetic fields XUV observations of coronal magnetic fields

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...40..103s&link_type=abstract

Solar Physics, vol. 40, Jan. 1975, p. 103-121. NASA-supported research.

Physics

70

Far Ultraviolet Radiation, Skylab Program, Solar Corona, Solar Magnetic Field, Spectroheliographs, Coronagraphs, Emission Spectra, Iron, Photosphere, Solar Atmosphere, Solar Radiation, Ultraviolet Spectroscopy

Scientific paper

Spectroheliograms obtained with the Naval Research Laboratory's Extreme Ultraviolet Spectrograph (S082A) on Skylab are compared with Kitt Peak National Observatory magnetograms. A principal result is the characteristic reconnection of flux from an emerging bipolar magnetic region to previously existing flux in its vicinity. Examples of the disappearance of magnetic flux from the solar atmosphere are also shown. The results of a particularly simple, potential field calculation are shown for comparison with the Skylab observations.

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