45 citations · 162 across the 5 of their papers we have counts for
7 papers
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…