The properties of closed coronal loops are reviewed. First we discuss the main features of the static, hot loop models. In these models thermal conduction plays the dominant role in determining the temperature and density structure. Next the cool loop models and their implications for solar observations are discussed. Finally, some new theoretical results on coronal abundances are presented. It is argued that chromospheric evaporation, which is a basic feature of the hot models, can account for the observed anomalies in the coronal element abundances.
The physics of coronal closed-field structures
Advances in Space Research ; 14 , 4
1994-04-01
Miscellaneous
No indication
English
The Physics of Coronal Closed-Field Structures
Online Contents | 1994
|The Physics of Coronal Closed-Field Structures
British Library Conference Proceedings | 1994
|The physics of coronal closed-filed structures
Elsevier | 1993
|NTRS | 1965
|Coronal physics from eclipse observations
Elsevier | 1993
|