CAOSP abstracts, Volume: 22, year: 1992

Abstract: The large-scale and long-term intensity variations of the green emission line corona FeXIV 530.3 nm over the 4.5 solar activity cycles are presented. Difficulties of putting the data of different observatories to the common photometric scale are discussed. Analysis of variability and periodicity of the coronal brightness in the separated belts of the heliographic latitudes seems to be very useful when studying responses of the solar activity in the heliosphere and geoactivity.

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