Coronal photometry and analysis of the eclipse corona of July 22, 1990

Details Coronal photometry and analysis of the eclipse corona of July 22, 1990 Coronal photometry and analysis of the eclipse corona of July 22, 1990

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26as...96..169k&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 96, no. 1, p. 169-182.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Photometry, Solar Corona, Solar Eclipses, Astronomical Observatories, Isophotes, Solar Magnetic Field, Solar Prominences

Scientific paper

Results are presented of aircraft-based observations and ground observations from multiple stations, made during the July 1990 eclipse. The main results of the analysis of the large-scale features of the inner corona concern the measurement of the flattening index of the near-maximum-activity corona; the occurrence of a large coronal hole; and the importance of the line emissions recorded on the broadband white-light pictures, due to the presence of numerous large or faint prominences all around the limb.

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