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Solar Magnetic Loops Observed with TRACE and EIT

Published online by Cambridge University Press:  26 May 2016

Markus J. Aschwanden  and
Alan M. Title
Markus J. Aschwanden
Affiliation:
Lockheed Martin, Solar & Astrophysics Laboratory, Palo Alto, CA 94304, USA
Alan M. Title
Affiliation:
Lockheed Martin, Solar & Astrophysics Laboratory, Palo Alto, CA 94304, USA

Abstract

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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 foot-points, (5) the magnetic energy budget for heating, and (6) oscillations and waves in coronal loops.

Type
Part 10: Structural Elements: Magnetic Loops
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 503 - 516
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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