WHERE IS THE CHROMOSPHERIC RESPONSE TO CONDUCTIVE ENERGY INPUT FROM A HOT PRE-FLARE CORONAL LOOP? (2014)
Attributed to:
Rolling Programme in Solar and Plasma Astrophysics
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1088/0004-637x/789/1/47
Publication URI: http://dx.doi.org/10.1088/0004-637x/789/1/47
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 1