NASA Technical Reports Server (NTRS) 19860015167: On the formation ... | |
by NASA Technical Reports Server (NTRS) | |
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A theoretical study of the formation of a coronal cavity | |
and its relation to a quiescent prominence is presented. | |
It is argued that the formation of a cavity is initiated | |
by the condensation of plasma which is trapped by the | |
coronal magnetic field in a closed streamer and which | |
then flows down to the chromosphere along the field lines | |
due to lack of stable magnetic support against gravity. | |
The existence of a coronal cavity depends on the coronal | |
magnetic field strength; with low strength, the plasma | |
density is not high enough for condensation to occur. | |
Furthermore, we suggest that prominence and cavity | |
material is supplied from the chromospheric level. | |
Whether a coronal cavity and a prominence coexist depends | |
on the magnetic field configuration; a prominence | |
requires stable magnetic support. | |
Date Published: 2016-09-17 09:09:03 | |
Identifier: NASA_NTRS_Archive_19860015167 | |
Item Size: 6510808 | |
Language: english | |
Media Type: texts | |
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