We present different aspects of the large-scale distribution of the coronal Fe XIV 530.3 nm emission line brightness (the abbreviation CGL- coronal green line-is used below). Evolution of this line intensity over the solar cycles is demonstrated and the relevance of the solar middle- latitude zones in displaying the coronal activity and variability is underlined.
Solar corona irradiance variability during the 1943-1999 period
2002
Abstract
We present different aspects of the large-scale distribution of the coronal Fe XIV 530.3 nm emission line brightness (the abbreviation CGL- coronal green line-is used below). Evolution of this line intensity over the solar cycles is demonstrated and the relevance of the solar middle- latitude zones in displaying the coronal activity and variability is underlined.File in questo prodotto:
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