Ciaravella, A. Loop modeling of stellar coronae and their spectra. Accademia Peloritana dei Pericolanti Classe FF.MM.NN., LXXII (Supplement 1). pp. 379-386.
![[thumbnail of atti_3_1994_sup1_379.pdf]](http://cab.unime.it/mus/style/images/fileicons/application_pdf.png) |
PDF
atti_3_1994_sup1_379.pdf - Published Version Restricted to users from Unime Download (2MB) | Request a copy |
Abstract
This paper considers a loop model of the corona and compares it with an ana1ogous isothermai slab modei; in particular it evaluates how the predicted spectra differ and how much such differences are significant. We study the influence ori the spectra and the intensity of loop emission of heat conduction regime already known to affect the plasma stratification inside coronal loops. The scope is to obtain a good grasp on these issues in the perspective of applying them to the detailed modeling of stellar and solar coronal emission in terms of emission from loops
| Item Type: | Article |
|---|---|
| Subjects: | M.U.S. - Miscellanea > Atti Accademia Peloritana > Classe di Scienze Fisiche, Matematiche e Naturali > 1994 > Supplemento 1 parte 2 M.U.S. - Miscellanea > Atti Accademia Peloritana > Classe di Scienze Medico-Biologiche > 1994 > Supplemento 1 parte 2 M.U.S. - Miscellanea > Atti Accademia Peloritana > Classe di Scienze Giuridiche, Economiche e Politiche > 1994 > Supplemento 1 parte 2 M.U.S. - Miscellanea > Atti Accademia Peloritana > Classe di Lettere Filosofia e belle Arti > 1994 > Supplemento 1 parte 2 |
| Depositing User: | Mr Nunzio Femminò |
| Date Deposited: | 14 Apr 2014 14:59 |
| Last Modified: | 17 Apr 2014 07:44 |
| URI: | http://cab.unime.it/mus/id/eprint/5157 |
Actions (login required)
 |
View Item |
