Observational Features of Large-Scale Structures as Revealed by the Catastrophe Model of Solar Eruptions
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/1009-9271/7/4/01/pdf
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1. SOHOObservations of a Coronal Mass Ejection
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3. How much energy can be stored in a three-dimensional force-free magnetic field?
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1. CONTRIBUTION OF VELOCITY VORTICES AND FAST SHOCK REFLECTION AND REFRACTION TO THE FORMATION OF EUV WAVES IN SOLAR ERUPTIONS;The Astrophysical Journal;2015-05-28
2. Numerical experiments on the evolution in coronal magnetic configurations including a filament in response to the change in the photosphere;Research in Astronomy and Astrophysics;2015-02-26
3. An EUV Jet and Hα Filament Eruption Associated with Flux Cancelation in a Decaying Active Region;Solar Physics;2009-01-15
4. References;Astronomy and Astrophysics Library
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