501 citations · 1.5k across the 19 of their papers we have counts for
21 papers
The Role of Non-local Thermal Transport in Flare-Driven Chromospheric Evaporation
Thomas Parmenter, Tony Arber, Sergey Belov +1
Thermal conduction plays an important role in energy transport during solar flares. Flares heat the solar atmosphere to tens of MK which, combined with mean free paths in excess of…
Inflationary stimulated Raman scattering in shock-ignition plasmas
SJ Spencer, Alexander Seaton, Tom Goffrey +1
In the shock-ignition inertial confinement fusion scheme, high-intensity lasers propagate through an inhomogeneous coronal plasma, driving a shock designed to cause fuel ignition.…
Unveiling the magnetic nature of chromospheric vortices
Mariarita Murabito, Juie Shetye, Marco Stangalini +5
Vortex structures in the Sun's chromosphere are believed to channel energy between different layers of the solar atmosphere. We investigate the nature and dynamics of two small-sca…
Signatures of quiet Sun reconnection events in Ca~{\sc ii}, H and Fe~{\sc i}
J. Shetye, S. Shelyag, A. L. Reid +3
We use observations of quiet Sun (QS) regions in the H 6563 Å, Ca~{\sc ii} 8542 Å\, and Fe~{\sc i} 6302 Å lines. We observe brightenings in the wings of the H and Ca~{\sc ii}…
Simulations of Alfven wave driving of the solar chromosphere - efficient heating and spicule launching
C. S. Brady, T. D. Arber
Two of the central problems in our understanding of the solar chromosphere are how the upper chromosphere is heated and what drives spicules. Estimates of the required chromospheri…
Alfvén Wave Heating of the Solar Chromosphere: 1.5D models
T. D. Arber, C. S. Brady, S. Shelyag
Physical processes which may lead to solar chromospheric heating are analyzed using high-resolution 1.5D non-ideal MHD modelling. We demonstrate that it is possible to heat the chr…