Orlando, S. and Peres , G. and Serio, S. (1994) Models of stationary siphon flows in stratified thermally conducting coronal loop. Accademia Peloritana dei Pericolanti, Classe di Scienze FF. MM. NN., LXXII (Supplement 1). pp. 647-653.
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Abstract
We present a hydrodynamic model of stationary siphon flows in a semicircular solar coronai loop. The model takes into account the effects of gravity, thermal conduction, radiative losses and a phenomenological heating term.
The model has been designed to provide a tool for insight into coronai loop physics and to help interpretation of the observations of new UV and X-ray instruments.
We derive scaling laws for subsonic flows in coronai loops which extend those of Rosner Tucker and Vaiana (1978) and of Serio et al. (1981) to the siphon flows. We explore thoroughly the space of solutions and identify four classes of solutions.
Finally, we explore the conditions for the presence of stationary shocks in critical and supersonic siphon flows in coronal loops.
Item Type: | Article |
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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: | 18 Apr 2014 10:20 |
Last Modified: | 18 Apr 2014 10:20 |
URI: | http://cab.unime.it/mus/id/eprint/5190 |
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