150 citations · 505 across the 7 of their papers we have counts for
7 papers
Observing the formation of flare-driven coronal rain
E. Scullion, L. Rouppe Van Der Voort, P. Antolin +4
Flare-driven coronal rain can manifest from rapidly cooled plasma condensations near coronal loop-tops in thermally unstable post-flare arcades. We detect 5 phases that characteris…
Modelling observed decay-less oscillations as resonantly enhanced Kelvin-Helmholtz vortices from transverse MHD waves and their seismological application
Patrick Antolin, Ineke De Moortel, Tom Van Doorsselaere +1
In the highly structured solar corona, resonant absorption is an unavoidable mechanism of energy transfer from global transverse MHD waves to local azimuthal Alfvén waves. Due to i…
Unresolved fine-scale structure in solar coronal loop-tops
Eamon Scullion, Luc Rouppe van der Voort, Sven Wedemeyer +1
New and advanced space-based observing facilities continue to lower the resolution limit and detect solar coronal loops in greater detail. We continue to discover even finer sub-st…
Simulating the in situ condensation process of solar prominences
Chun Xia, Rony Keppens, Patrick Antolin +1
Prominences in the solar corona are hundredfold cooler and denser than their surroundings, with a total mass of 1.e13 up to 1.e15 g. Here we report on the first comprehensive simul…
Detection of supersonic downflows and associated heating events in the transition region above sunspots
L. Kleint, P. Antolin, H. Tian +18
IRIS data allow us to study the solar transition region (TR) with an unprecedented spatial resolution of 0.33 arcsec. On 2013 August 30, we observed bursts of high Doppler shifts s…
Fine strand-like structure in the solar corona from MHD transverse oscillations
P. Antolin, T. Yokoyama, T. Van Doorsselaere
Current analytical and numerical modelling suggest the existence of ubiquitous thin current sheets in the corona that could explain the observed heating requirements. On the other…