activity
19992026
most citedMPI-AMRVAC for Solar and Astrophysics

254 citations · 1k across the 52 of their papers we have counts for

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Showing 2024Show all

13 papers · 1 filter

astro-ph.SR2024

Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC II: Optimization and application in three-dimensional models

Yuhao Zhou, Xiaohong Li, Jack M. Jenkins +2

The frozen-field hydrodynamic (ffHD) model is a simplification of the full magnetohydrodynamical (MHD) equations under the assumption of a rigid magnetic field, which significantly…

astro-ph.SR2024

Mass Cycle and Dynamics of a Virtual Quiescent Prominence

Dion Donné, Rony Keppens

The mass cycle of solar prominences or filaments is still not completely understood. Researchers agree that these dense structures form by coronal in-situ condensations and plasma…

physics.plasm-ph2024

Collisional damping of wave modes in ion-electron plasmas

Joeri De Vadder, Jordi De Jonghe, Rony Keppens

To expand on recent work, we introduce collisional terms in the analysis of the warm ion-electron, two-fluid equations for a homogeneous plasma at rest. Consequently, the plasma is…

astro-ph.SR2024★ 5 cited

From eruption to post-flare rain: a 2.5D MHD model

Samrat Sen, Avijeet Prasad, Valeriia Liakh +1

The formation of the MFRs in the pre-flare stage, and how this leads to coronal rain in a post-eruption magnetic loop is not fully understood. We explore the formation, and eruptio…

physics.plasm-ph2024★ 7 cited

BxC Toolkit: Generating Tailored Turbulent 3D Magnetic Fields

Daniela Maci, Rony Keppens, Fabio Bacchini

Turbulent states are ubiquitous in plasmas and the understanding of turbulence is fundamental in modern astrophysics. Numerical simulations, which are the state-of-the-art approach…

astro-ph.SR2024

Frozen-field Modeling of Coronal Condensations with MPI-AMRVAC I: Demonstration in two-dimensional models

Yuhao Zhou, Xiaohong Li, Rony Keppens

Large-scale coronal plasma evolutions can be adequately described by magnetohydrodynamics (MHD) equations. However, full multi-dimensional MHD simulations require substantial compu…