202 citations · 677 across the 17 of their papers we have counts for
6 papers · 1 filter
Understanding the plasma and magnetic field evolution of a filament using observations and Nonlinear force-free field modelling
Stephanie L. Yardley, Antonia Savcheva, Lucie M. Green +4
We present observations and magnetic field models of an intermediate filament present on the Sun in August 2012, associated with a polarity inversion line that extends from AR 1154…
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…
Stealth Coronal Mass Ejections from Active Regions
Jennifer O'kane, Lucie Green, David M. Long +1
Stealth coronal mass ejections (CMEs) are eruptions from the Sun that have no obvious low coronal signature. These CMEs are characteristically slower events, but can still be geoef…
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…
Transient Inverse-FIP Plasma Composition Evolution within a Confined Solar Flare
Deborah Baker, Lidia van Driel-Gesztelyi, David H. Brooks +9
Understanding elemental abundance variations in the solar corona provides an insight into how matter and energy flow from the chromosphere into the heliosphere. Observed variations…
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…