Onset of a Large Ejective Solar Eruption from a Typical Coronal-jet-base Field Configuration-Reference-Cited by-同舟云学术

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Onset of a Large Ejective Solar Eruption from a Typical Coronal-jet-base Field Configuration

Published:2017-08-09 Issue:1 Volume:845 Page:26
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Joshi Navin Chandra,Sterling Alphonse C.^ORCID,Moore Ronald L.,Magara Tetsuya^ORCID,Moon Yong-Jae^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/845/i=1/a=26/pdf

Reference80 articles.

1. A Model for Solar Coronal Mass Ejections

2. The Topology and Evolution of the Bastille Day Flare

3. The standard flare model in three dimensions

4. Slip-Running Reconnection in Quasi-Separatrix Layers

5. Radio evidence for breakout reconnection in solar eruptive events

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1. An explanation for the slow-rise phase of solar eruptions;Monthly Notices of the Royal Astronomical Society;2024-09-06

2. Magnetic Eruption from a Three-ribbon Flare;The Astrophysical Journal;2024-08-28

3. Recent advances in solar data-driven MHD simulations of the formation and evolution of CME flux ropes;Reviews of Modern Plasma Physics;2024-08-10

4. Periods and Frequency Drifts of Groups of the Decimetric Spikes in Two Solar Flares;Solar Physics;2024-08

5. Circular-ribbon flares and the related activities;Reviews of Modern Plasma Physics;2024-03-10

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