Origin and structures of solar eruptions I: magnetic flux rope
Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
eruptive phenomena in our solar system and able to release a large quantity of plasma and …
The source and engine of coronal mass ejections
Coronal mass ejections (CMEs) are large-scale expulsions of coronal plasma and magnetic
field propagating through the heliosphere. Because CMEs are observed by white-light …
field propagating through the heliosphere. Because CMEs are observed by white-light …
The standard flare model in three dimensions-III. Slip-running reconnection properties
Context. A standard model for eruptive flares aims at describing observational 3D features of
the reconnecting coronal magnetic field. Extensions to the 2D model require the physical …
the reconnecting coronal magnetic field. Extensions to the 2D model require the physical …
Magnetic flux ropes in the solar corona: structure and evolution toward eruption
R Liu - Research in Astronomy and Astrophysics, 2020 - iopscience.iop.org
Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
Direct In Situ Measurements of a Fast Coronal Mass Ejection and Associated Structures in the Corona
We report on the first direct in situ measurements of a fast coronal mass ejection (CME) and
shock in the corona, which occurred on 2022 September 5. In situ measurements from the …
shock in the corona, which occurred on 2022 September 5. In situ measurements from the …
Deciphering the slow-rise precursor of a major coronal mass ejection
X Cheng, C ** magnetic reconnection during an X-class solar flare observed by SDO/AIA
J Dudík, M Janvier, G Aulanier… - The Astrophysical …, 2014 - iopscience.iop.org
We present SDO/AIA observations of an eruptive X-class flare of 2012 July 12, and compare
its evolution with the predictions of a three-dimensional (3D) numerical simulation. We focus …
its evolution with the predictions of a three-dimensional (3D) numerical simulation. We focus …
Decoding the pre-eruptive magnetic field configurations of coronal mass ejections
A clear understanding of the nature of the pre-eruptive magnetic field configurations of
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …
Coronal Mass Ejections (CMEs) is required for understanding and eventually predicting …