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Solar Magnetic Loops Observed with TRACE and EIT View all abstracts by submitter

Markus J. Aschwanden   Submitted: 2003-11-03 15:39

We select some highlights and new results that have been obtained from detailed ``microscopic'' observations of coronal loop structures with the Transition Region and Coronal Explorer (TRACE) and Extreme Ultraviolet Imager (EIT) instruments, including: (1) the inhomogeneous substructure of EUV loops, (2) the dynamic and non-hydrostatic nature, (3) the non-uniform heating, (4) the magnetic topology at the loop footpoints, (5) the magnetic energy budget for heating, and (6) oscillations and waves in coronal loops.

Authors: Markus J. Aschwanden and Alan M. Title
Projects: Soho-EIT,TRACE

Publication Status: in Stars as Suns: Activity, Evolution and Planets, Symposium S219, IAU 25th Coll. and General Assembly, held in Sydney, Australi
Last Modified: 2003-11-03 15:49
Go to main E-Print page  The evolution of twisting coronal magnetic flux tubes  Global Sausage Modes of Coronal Loops  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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