Electronic Resource
Springer
Space science reviews
70 (1994), S. 171-174
ISSN:
1572-9672
Keywords:
Sun: corona
;
Sun: activity
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract Parameters of expanding magnetic loops and arches and of mass flows generated by them in the corona have been computed in a 1D two-fluid approximation. Two possible trigger mechanisms of the coronal transients have been considered: (i) sudden increase of the background magnetic field strength, and (ii) heating and compression plasma inside these magnetic structures. We discuss the formation of shock waves and their dependence on dynamics and geometry of the magnetic structures.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00777862
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