The Fast Collisionless Reconnection Condition and the Self‐Organization of Solar Coronal Heating-Reference-Cited by-同舟云学术

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The Fast Collisionless Reconnection Condition and the Self‐Organization of Solar Coronal Heating

Published:2007-12-20 Issue:2 Volume:671 Page:2139-2153
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Uzdensky Dmitri A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference116 articles.

1. Evidence for Nonuniform Heating of Coronal Loops Inferred from Multithread Modeling ofTRACEData

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

3. The New Solar Corona

4. The Coronal Heating Paradox

5. Time Variability of the “Quiet” Sun Observed withTRACE. II. Physical Parameters, Temperature Evolution, and Energetics of Extreme‐Ultraviolet Nanoflares

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