The structure of the white-light corona on June 11, 1983

Details The structure of the white-light corona on June 11, 1983 The structure of the white-light corona on June 11, 1983

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..281r&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 36, Sept. 1985, p. 281-283. Research supported by the

Astronomy and Astrophysics

Astronomy

1

Solar Corona, Solar Eclipses, Brightness, Coronal Loops

Scientific paper

The structure of the white-light corona during the total solar eclipse of June 11, 1983 was of the temporary type and displayed four different features: coronal holes (polar), polar rays, mid- and equatorial latitude streamers as well as neutral sheet type rays. The dominating feature is the helmet streamer in the southeast quadrant, a system of loops and the coronal condensation above the W limb. For the given ellipticity the total brightness of the white-light corona should be JK = 0.83×10-6±20% of the brightness of the solar disk.

Affiliated with

Also associated with

No associations

Rating

The structure of the white-light corona on June 11, 1983 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The structure of the white-light corona on June 11, 1983, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The structure of the white-light corona on June 11, 1983 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-800549