|
|||||
|
|
Solar corona irradiance variability during the 1943–1999 period |
|
| Authors: | J Sýkora O G Badalyan M Storini |
| Institution: | a Astronomical Institute, 05960, Tatranská Lomnica, Slovak Republic b Institute of the Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, 142190, Troitsk, Russia c IFSI/CNR, Via del Fosso del Cavaliere 100, 00133 Roma, Italy and Raggi Cosmici, Dip. Fisica/UNIRomaTre, Via del Vasca Navale 84, 00146, Roma, Italy |
| 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. |
| Keywords: | |
| 本文献已被 ScienceDirect 等数据库收录！ | |