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Dynamic signatures of quiet sun magnetic fields

Author
Martin, S. F.
Published
JAN 1, 1983.
Physical Description
1 electronic document
Online Version

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Summary
The collision and disappearance of opposite polarity fields is observed most frequently at the borders of network cells. Due to observational limitations, the frequency, magnitude, and spatial distribution of magnetic flux loss have not yet been quantitatively determined at the borders or within the interiors of the cells. However, in agreement with published hypotheses of other authors, the disapperance of magnetic flux is speculated to be a consequence of either gradual or rapid magnetic reconnection which could be the means of converting magnetic energy into the kinetic, thermal, and nonthermal sources of energy for microflares, spicules, the solar wind, and the heating of the solar corona.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 19840012396.
Accession ID: 84N20464.
NASA-CR-173361.
BBSO-0228.
NAS 1.26:173361.
Sacramento Peak Workshop on Small-Scale Dyn. Processes; 25-29 Jul. 1983.
Terms of Use and Reproduction
No Copyright.
View MARC record | catkey: 15708453