Coronal Heating, Spicules, and SolarB

Details Coronal Heating, Spicules, and SolarB Coronal Heating, Spicules, and SolarB

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..283m&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

2

Scientific paper

We summarize certain observations of coronal luminosity, network magnetic flux, spicules, and macrospicules. These observations together imply that in quiet regions that are not influenced by active regions the coronal heating comes from magnetic activity in the edges of the network flux, possibly from explosions of sheared core fields around granule-sized inclusions of opposite-polarity flux. This scenario can be tested by SolarB.

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