361 citations · 2.4k across the 37 of their papers we have counts for
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Twist Accumulation and Topology Structure of a Solar Magnetic Flux Rope
Y. Guo, M. D. Ding, X. Cheng +2
To study the build up of a magnetic flux rope before a major flare and coronal mass ejection (CME), we compute the magnetic helicity injection, twist accumulation, and the topology…
First observational application of a connectivity--based helicity flux density
K. Dalmasse, E. Pariat, G. Valori +2
Measuring the magnetic helicity distribution in the solar corona can help in understanding the trigger of solar eruptive events because magnetic helicity is believed to play a key…
Photospheric Injection of Magnetic Helicity: Connectivity--based Flux Density Method
K. Dalmasse, E. Pariat, P. Démoulin +1
Magnetic helicity quantifies how globally sheared and/or twisted is the magnetic field in a volume. This quantity is believed to play a key role in solar activity due to its conser…
The standard flare model in three dimensions III. Slip-running reconnection properties
Miho Janvier, Guillaume Aulanier, Etienne Pariat +1
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 unders…
Accuracy of magnetic energy computations
G. Valori, P. Demoulin, E. Pariat +1
For magnetically driven events, the magnetic energy of the system is the prime energy reservoir that fuels the dynamical evolution. In the solar context, the free energy is one of…