THE MAGNETIC FIELD OF ACTIVE REGION 11158 DURING THE 2011 FEBRUARY 12-17 FLARES: DIFFERENCES BETWEEN PHOTOSPHERIC EXTRAPOLATION AND CORONAL FORWARD-FITTING METHODS-Reference-Cited by-同舟云学术

THE MAGNETIC FIELD OF ACTIVE REGION 11158 DURING THE 2011 FEBRUARY 12-17 FLARES: DIFFERENCES BETWEEN PHOTOSPHERIC EXTRAPOLATION AND CORONAL FORWARD-FITTING METHODS

Published:2014-03-21 Issue:1 Volume:785 Page:34
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Aschwanden Markus J.,Sun Xudong,Liu Yang

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/785/i=1/a=34/pdf

Reference91 articles.

1. Magneto-Acoustic Energetics Study of the Seismically Active Flare of 15 February 2011

2. A Code for Automated Tracing of Coronal Loops Approaching Visual Perception

3. A Nonlinear Force-Free Magnetic Field Approximation Suitable for Fast Forward-Fitting to Coronal Loops. I. Theory

4. A Nonlinear Force-Free Magnetic Field Approximation Suitable for Fast Forward-Fitting to Coronal Loops. III. The Free Energy

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