SHEAR PHOTOSPHERIC FORCING AND THE ORIGIN OF TURBULENCE IN CORONAL LOOPS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/722/i=1/a=65/pdf
Reference63 articles.
1. DOES THE COMPRESSION OR THE EXPANSION OF A SIMPLE TOPOLOGY POTENTIAL MAGNETIC FIELD LEAD TO THE DEVELOPMENT OF CURRENT SHEETS?
2. The topology of force-free magnetic fields and its implications for coronal activity
3. SELF-ORGANIZED BRAIDING AND THE STRUCTURE OF CORONAL LOOPS
4. Fast reconnection in high-Lundquist-number plasmas due to the plasmoid Instability
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