45 citations · 281 across the 15 of their papers we have counts for
15 papers
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code
Valeriia Liakh, Jack Jenkins
This review surveys recent advances in the numerical modeling of solar prominences and coronal rain achieved with the fully open-source adaptive-grid, parallelized Adaptive Mesh Re…
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…
The Bright Rim Prominences according to 2.5D Radiative Transfer
Jack M. Jenkins, Christopher M. J. Osborne, Ye Qiu +2
Solar prominences observed close to the limb commonly include a bright feature that, from the perspective of the observer, runs along the interface between itself and the underlyin…
3D coupled tearing-thermal evolution in solar current sheets
Samrat Sen, Jack Jenkins, Rony Keppens
Combined tearing-thermal evolution plays an important role in the disruption of current sheets, and formation of cool condensations within the solar atmosphere. However, this has r…
Simulating Rayleigh-Taylor induced magnetohydrodynamic turbulence in prominences
Madhurjya Changmai, Jack M. Jenkins, J. -B. Durrive +1
Solar prominences represent large-scale condensations suspended against gravity within the solar atmosphere. The Rayleigh-Taylor (RT) instability is proposed to be one of the impor…
1.5D NLTE spectral synthesis of a 3D filament/prominence simulation
J. M. Jenkins, C. M. J. Osborne, R. Keppens
Aims. We here demonstrate how the recently developed Lightweaver framework makes non-LTE (NLTE) spectral synthesis feasible on a new 3D ab-initio magnetohydrodynamic (MHD) filament…
The influence of flux rope heating models on solar prominence formation
N. Brughmans, J. M. Jenkins, R. Keppens
Aims. We begin by exploring the influence of two classes of commonly adopted heating models on the formation behaviour of solar prominences. These models consider either an exponen…
Velocities of an Erupting Filament
Shuo Wang, Jack M. Jenkins, Karin Muglach +5
Solar filaments exist as stable structures for extended periods of time before many of them form the core of a CME. We examine the properties of an erupting filament on 2017 May 29…
Prominence formation by levitation-condensation at extreme resolutions
Jack Jenkins, Rony Keppens
Prominences in the solar atmosphere represent an intriguing and delicate balance of forces and thermodynamics in an evolving magnetic topology. How this relatively cool material co…
Magnetic Structure of an Erupting Filament
Shuo Wang, Jack M. Jenkins, Valentin Martinez Pillet +5
The full 3-D vector magnetic field of a solar filament prior to eruption is presented. The filament was observed with the Facility Infrared Spectropolarimeter at the Dunn Solar Tel…
2D non-LTE modelling of a filament observed in the H_alpha line with the DST/IBIS spectropolarimeter
P. Schwartz, S. Gunar, J. M. Jenkins +3
We study a fragment of a large quiescent filament observed on May 29, 2017 by the Interferometric BIdimensional Spectropolarimeter (IBIS) mounted at the Dunn Solar Telescope. We fo…
Quantifying the relationship between Moreton-Ramsey waves and "EIT waves" using observations of 4 homologous wave events
David M. Long, Jack Jenkins, Gherardo Valori
Freely-propagating global waves in the solar atmosphere are commonly observed using Extreme UltraViolet passbands (EUV or "EIT waves"), and less regularly in H-alpha (Moreton-Ramse…
Modelling the Effect of Mass-Draining on Prominence Eruptions
Jack M. Jenkins, Matthew Hopwood, Pascal Démoulin +4
Quiescent solar prominences are observed to exist within the solar atmosphere for up to several solar rotations. Their eruption is commonly preceded by a slow increase in height th…
Plasma evolution within an erupting coronal cavity
David M. Long, Louise K. Harra, Sarah A. Matthews +5
Coronal cavities have previously been observed associated with long-lived quiescent filaments and are thought to correspond to the associated magnetic flux rope. Although the stand…
Understanding the Role of Mass-Unloading in Filament Eruptions
Jack Jenkins, David M Long, Lidia van Driel-Gesztelyi +1
We describe a partial filament eruption on 11 December 2011 which demonstrates that the inclusion of mass is an important next step for understanding solar eruptions. Observations…