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The Magnetic Structure of Plages

Zirin, H. (1974) The Magnetic Structure of Plages. In: Chromospheric Fine Structure. International Astronomical Union Symposium (IAUS). No.56. Springer Netherlands , Dordrecht, pp. 161-175. ISBN 9789027702883. https://resolver.caltech.edu/CaltechAUTHORS:20201013-155619814

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Abstract

Every sunspot group is surrounded by regions of weaker magnetic field; traditionally those parts which appear in emission in resonance lines are called plages. There is a more extensive region of enhanced magnetic field which is not bright because the magnetic field is horizontal; this region is easily discernible by dark horizontal fibrils in Hα and is included in our discussion. The plage includes most of the magnetic field in an active center and is the locus of most of the flares.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-010-2103-6_20DOIArticle
Additional Information:© International Astronomical Union 1974. This research was supported by NASA under NGR 05-002-034 and by NSF Atmospheric Sciences program under GA-24015.
Funders:
Funding AgencyGrant Number
NASANGR 05-002-034
NSFGA-24015
Subject Keywords:Active Region; Magnetic Structure; Solar Physics; Sunspot Group; Neutral Line
Series Name:International Astronomical Union Symposium (IAUS)
Issue or Number:56
Record Number:CaltechAUTHORS:20201013-155619814
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201013-155619814
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106050
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:14 Oct 2020 20:05
Last Modified:14 Oct 2020 20:05

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