The solar corona 530.3 NM in the 20th cycle

Details The solar corona 530.3 NM in the 20th cycle The solar corona 530.3 NM in the 20th cycle

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...61..301r&link_type=abstract

Solar Physics, vol. 61, Mar. 1979, p. 301-310.

Physics

6

Astronomical Spectroscopy, Infrared Spectra, Solar Corona, Solar Spectra, Sunspot Cycle, Emission Spectra, Line Spectra, Maxima, Northern Hemisphere, Southern Hemisphere

Scientific paper

Data from the Lomnicky Stit station for the 1965-1976 period was used in performing an analysis of the 530.3-nm coronal emission line. It is found that the development of intensities often differed in the northern and southern hemispheres. The third increase of intensities in the course of the cycle was observed nearly at all latitudes; the maximum of intensities of this 'burst of activity' was observed at latitudes around 60 deg in both hemispheres.

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