WHERE IS THE CHROMOSPHERIC RESPONSE TO CONDUCTIVE ENERGY INPUT FROM A HOT PRE-FLARE CORONAL LOOP?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/789/i=1/a=47/pdf
Reference30 articles.
1. THERMAL TO NONTHERMAL ENERGY PARTITION AT THE EARLY RISE PHASE OF SOLAR FLARES
2. THERMAL FRONTS IN FLARING MAGNETIC LOOPS
3. Observations of conduction driven evaporation in the early rise phase of solar flares
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