117 citations · 279 across the 16 of their papers we have counts for
17 papers · 1 filter
On the dynamics, thermodynamics and fine structure of virtual erupting filaments
Dion Donné, Yuhao Zhou, Hebe Cremades +1
It is not fully understood why some solar filaments erupt while others do not. Those that do typically undergo a slow rise followed by an acceleration phase, though this transition…
The Formation of Solar Prominences: Plasma Origin and Mechanisms
Yuhao Zhou
Solar prominences, or solar filaments, are cool and dense plasma structures in the hot solar corona, whose formation mechanisms have remained a fundamental challenge in solar physi…
Modeling multiphase plasma in the corona: prominences and rain
Rony Keppens, Yuhao Zhou, Chun Xia
We review major achievements in our understanding of multiphase coronal plasma, where cool-dense and hot-tenuous matter coexists, brought about by advances in modeling and theory,…
Response of the solar atmosphere to flux emergence: With emergence-driven prominence formation
Xiaohong Li, Yuhao Zhou, Rony Keppens
Flux emergence is crucial for the formation of solar active regions and triggering of various eruptions. However, the detailed mechanisms by which flux emergence drives these erupt…
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…
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…