The plasma properties of the solar upper atmosphere determined from high resolution observations and the nature of the physical processes sustaining it*-Reference-Cited by-同舟云学术

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The plasma properties of the solar upper atmosphere determined from high resolution observations and the nature of the physical processes sustaining it*

Published:1994-05 Issue:5 Volume:1 Page:1390-1402
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Feldman Uri

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.870689

Reference43 articles.

1. Nanoflares and the solar X-ray corona

2. Energy release in solar flares

3. Heating solar coronal holes

4. Mass and Energy Flow in the Solar Chromosphere and Corona

Cited by 5 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Electric Currents as the Main Cause of Coronal and Flare Activity in the Sun and in Many Late-Type Stars;Physica Scripta;2002-01-01

2. On the Correlation between Coronal and Lower Transition Region Structures at Arcsecond Scales;The Astrophysical Journal;2001-12-10

3. Conventional solar flare theory re-examined;Physics of Plasmas;1997-05

4. Electromagnetic properties of hot collisionless plasma in magnetic reconnection regions;Radiophysics and Quantum Electronics;1996-02

5. Nonlinear dynamics of twisted magnetic flux tubes;Physics of Plasmas;1995-12

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