An observation of prominence condensation out of a coronal void

Details An observation of prominence condensation out of a coronal void An observation of prominence condensation out of a coronal void

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...83..115w&link_type=abstract

Solar Physics, vol. 83, Feb. 1983, p. 115-119. Research supported by the U.S. National Research Council.

Physics

5

Coronal Holes, Solar Eclipses, Solar Limb, Solar Prominences, Astronomical Photography, High Resolution, Signal To Noise Ratios, Solar Observatories

Scientific paper

Photographic averaging of cine-camera data-frames from the 7 March 1970 eclipse provided a record of the inner white light corona with unusually high resolution for low-contrast features. The authors report that a coronal void, similar to high corona structures associated with prominence formation (MacQueen et al., 1983), extended low into the corona. During eclipse totality, a coronal rain prominence condensed from the base of the void.

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