The Long‐Term Evolution of AR 7978: Testing Coronal Heating Models-Reference-Cited by-同舟云学术

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The Long‐Term Evolution of AR 7978: Testing Coronal Heating Models

Published:2003-03-20 Issue:1 Volume:586 Page:592-605
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Demoulin P.,van Driel‐Gesztelyi L.,Mandrini C. H.,Klimchuk J. A.,Harra L.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/586/i=1/a=592/pdf

Reference68 articles.

1. Modeling of Coronal EUV Loops Observed withTRACE. I. Hydrostatic Solutions with Nonuniform Heating

2. Three‐dimensional Stereoscopic Analysis of Solar Active Region Loops. II.SOHO/EIT Observations at Temperatures of 1.5–2.5 MK

3. Energy-crossing number relations for braided magnetic fields

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1. Construction of coronal hole and active region magnetohydrostatic solutions in two dimensions: Force and energy balance;Astronomy & Astrophysics;2022-04

2. Global Energetics of Solar Flares. XII. Energy Scaling Laws;The Astrophysical Journal;2020-10-29

3. The Role of Magnetic Field Disturbances in the Heating of Active Region Loops;Journal of Physics: Conference Series;2020-09-01

4. Global conditions in the solar corona from 2010 to 2017;Science Advances;2017-07-07

5. A THREE-DIMENSIONAL MODEL OF ACTIVE REGION 7986: COMPARISON OF SIMULATIONS WITH OBSERVATIONS;The Astrophysical Journal;2016-01-19

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