Inferring the magnetic field from the Rayleigh–Taylor instability
BJ Gréa, A Briard - The Astrophysical Journal, 2023 - iopscience.iop.org
By extending the potential approach of Layzer and Goncharov to the
magnetohydrodynamics equations, we find the nonlinear solutions to the single-mode …
magnetohydrodynamics equations, we find the nonlinear solutions to the single-mode …
Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC. II. Optimization and Application in 3D Models
Y Zhou, X Li, JM Jenkins, J Hong… - The Astrophysical …, 2024 - iopscience.iop.org
The frozen-field hydrodynamic (ffHD) model is a simplification of the full
magnetohydrodynamical equations under the assumption of a rigid magnetic field, which …
magnetohydrodynamical equations under the assumption of a rigid magnetic field, which …
Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC II: Optimization and application in three-dimensional models
Y Zhou, X Li, JM Jenkins, J Hong… - arXiv preprint arXiv …, 2024 - arxiv.org
The frozen-field hydrodynamic (ffHD) model is a simplification of the full
magnetohydrodynamical (MHD) equations under the assumption of a rigid magnetic field …
magnetohydrodynamical (MHD) equations under the assumption of a rigid magnetic field …
Prominence and coronal rain formation by steady versus stochastic heating and how we can relate it to observations
V Jerčić, JM Jenkins, R Keppens - arXiv preprint arXiv:2406.02955, 2024 - aanda.org
Context. Prominences and coronal rain are two forms of coronal condensations for which we
still lack satisfactory details on the formation pathways and conditions under which the two …
still lack satisfactory details on the formation pathways and conditions under which the two …