Physical conditions for fast reconnection evolution in space plasmas-Reference-Cited by-同舟云学术

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Physical conditions for fast reconnection evolution in space plasmas

Published:2012-07 Issue:7 Volume:19 Page:072315
ISSN:1070-664X
Container-title:Physics of Plasmas
language:en
Short-container-title:Physics of Plasmas

Author:

Ugai M.

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Link

http://aip.scitation.org/doi/pdf/10.1063/1.4739286

Reference41 articles.

1. Magnetic Reconnection

2. Petschek‐like Reconnection with Current‐driven Anomalous Resistivity and Its Application to Solar Flares

3. Filamentary structure on the Sun from the magnetic Rayleigh–Taylor instability

4. H. E. Petschek,NASA Special Publication 50(National Aeronautics and Space Administration, Washington, DC, 1964), p. 425.

5. Theoretical models of magnetic field line merging

Cited by 6 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. Effects of Magnetic Perturbation on Reconnection and Heating in the Solar Corona;The Astrophysical Journal;2020-11-06

2. Substorm onset: Current sheet avalanche and stop layer;Journal of Geophysical Research: Space Physics;2015-03

3. Reconnection properties in collisionless plasma with open boundary conditions;Physics of Plasmas;2014-07

4. Relating reconnection rate, exhaust structure and effective resistivity;Physics of Plasmas;2014-03

5. Flux Emergence (Theory);Living Reviews in Solar Physics;2014

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