The evolution and the secondary maximum of the green line intensity |
| |
| Authors: | J Xanthakis B Petropoulos H Mavromichalaki |
| |
| Institution: | (1) Research Center for Astronomy and Applied Mathematics, Academy of Athens, Anagnóstopoulou 14, Athens, Greece;(2) Cosmic Ray Group, University of Athens, Nuclear Physics Lab., Solonos 104, 144 Athens, Greece |
| |
| Abstract: | A new relation has been given in order to calculate the intensity of the green line of the solar corona at 5303 Å as a function of the number of proton events N
P
and the R
 (R) index of solar activity. This relation is available for the 19th and 20th solar cycles. Moreover there is given a theoretical justification of this relationship taking into account as a new parameter the evolution of the coronal magnetic field during the solar cycle. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
