Thank you Markus for the preprint.
Looking at your most important Fig. 3, you give the impression that MORE free energy is available in the corona AFTER the peak of the flare (GOES HXR, SXR emissions, etc) than before. 
Is not exactly the opposite of what we would wait following your Introductory presentation of the topic and even the title of the paper?
Or did I miss something fundamental?
Best,
S.

Le 13/04/2015 21:06, Markus J. Aschwanden a écrit :
 Aschwanden,M.J. . 2015, ApJL ... (revised, 2015 Apr 2)
URL1="http://www.lmsal.com/~aschwand/eprints/2015_iris.pdf" 
Magnetic energy dissipation during the 2014 Mar 29 flare: 
Consistent measurements in the transition region and corona with IRIS and AIA/SDO


____________________________________
Dr. Markus J. Aschwanden
Solar & Astrophysics Laboratory
Lockheed Martin Advanced Techology Center
A021S, Bldg. 252
3251 Hanover St., Palo Alto, CA 94304, USA
Phone: 650-424-4001, FAX: 650-424-3994
URL: http://www.lmsal.com/~aschwand/
e-mail: aschwanden@lmsal.com
____________________________________




_______________________________________________
Loops mailing list
Loops@solar.physics.montana.edu
https://mithra.physics.montana.edu/mailman/listinfo/loops