Stability of the photometric observations of the solar corona and variations of its intensity in the solar cycle 21

Details Stability of the photometric observations of the solar corona and variations of its intensity in the solar cycle 21 Stability of the photometric observations of the solar corona and variations of its intensity in the solar cycle 21

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...90..177g&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 90, Jan. 1984, p. 177-184.

Physics

6

Coronagraphs, Solar Corona, Solar Cycles, Correlation Coefficients, Error Analysis, Instrument Errors, Radiant Flux Density, Solar Spectra, Stellar Spectrophotometry

Scientific paper

A comparison of intensity measurements of the coronal line 5303 Å from observations at Norikura, Kislovodsk and Lomnický Štít is used to determine the stability of photometric systems and cancel the effect of its variations. The intensity variations of the solar corona during the 21st solar cycle are plotted. It is confirmed that the 11-year solar cycle consists of two maxima of activity; the first one is characterized by a simultaneous enhancement of activity at all latitudes and the second one shows up only in the equatorial zone.

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