Solar corona irradiance variability during the 1943-1999 period (Articolo in rivista)

Type
Label
  • Solar corona irradiance variability during the 1943-1999 period (Articolo in rivista) (literal)
Anno
  • 2002-01-01T00:00:00+01:00 (literal)
Alternative label
  • Kora J., Badalayan O.G., Storini M. (2002)
    Solar corona irradiance variability during the 1943-1999 period
    in Advances in space research
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Kora J., Badalayan O.G., Storini M. (literal)
Pagina inizio
  • 1975 (literal)
Pagina fine
  • 1978 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 29 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Titolo
  • Solar corona irradiance variability during the 1943-1999 period (literal)
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. (literal)

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