243 citations · 1.1k across the 22 of their papers we have counts for
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Coronal heating by MHD waves
Tom Van Doorsselaere, Abhishek K. Srivastava, Patrick Antolin +9
The heating of the solar chromosphere and corona to the observed high temperatures, imply the presence of ongoing heating that balances the strong radiative and thermal conduction…
Magnetohydrodynamic Fast Sausage Waves in the Solar Corona
B. Li, P. Antolin, M. -Z. Guo +4
Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for solar coronal sei…
Ubiquitous hundred-Gauss magnetic fields in solar spicules
M. Kriginsky, R. Oliver, N. Freij +3
Aims. We use high-resolution spectropolarimetric observations in the Ca ii 8542 A line obtained with the SST to study the magnetic field in solar spicules. Methods. The equations t…
Temporal and Spatial Scales in Coronal Rain Revealed by UV Imaging and Spectroscopic Observations
Ryohtaroh T. Ishikawa, Yukio Katsukawa, Patrick Antolin +1
Coronal rain corresponds to cool and dense clumps in the corona accreting towards the solar surface, and is often observed above solar active regions. They are generally thought to…
Electron Beams Cannot Directly Produce Coronal Rain
Jeffrey W. Reep, Patrick Antolin, Stephen J. Bradshaw
Coronal rain is ubiquitous in flare loops, forming shortly after the onset of the solar flare. Rain is thought to be caused by a thermal instability, a localized runaway cooling of…