THE DEPENDENCE OF CORONAL LOOP HEATING ON THE CHARACTERISTICS OF SLOW PHOTOSPHERIC MOTIONS (2016)
Attributed to:
Dynamics of Complex Magnetic Fields: From the corona to the solar wind
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/0004-637x/824/1/19
Publication URI: http://dx.doi.org/10.3847/0004-637x/824/1/19
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1