The finest white-light coronal features

Details The finest white-light coronal features The finest white-light coronal features

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..148..169k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 148, no. 1, p. 169-172

Physics

8

Coronal Loops, Solar Atmosphere, Solar Corona, Astronomical Photography, Charge Coupled Devices, Image Processing, Reflecting Telescopes, Solar Eclipses

Scientific paper

An attempt to detect the finest white-light coronal features observed with a large optical telescope was made at the July 11, 1991 Solar Total Eclipse. A few selected results taken from the video-CCD high speed observations obtained at the prime focus of the Canada-France-Hawaii-Telescope (CFHT) with a red coronal interference filter are presented. The smallest (sub-arsec) detected and/or resolved coronal features are shown. The methods that were used to extract them from the noisy and seeing-limited images taken from video frames are described.

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