170 citations · 1.3k across the 27 of their papers we have counts for
5 papers · 1 filter
Surface flux evolution constraints for flux transport dynamos
R. H. Cameron, D. Schmitt, J. Jiang +1
The surface flux transport (SFT) model of solar magnetic fields involves empirically well-constrained velocity and magnetic fields. The basic evolution of the Sun's large-scale sur…
Waves as the source of apparent twisting motions in sunspot penumbrae
L. Bharti, R. H. Cameron, M. Rempel +2
The motion of dark striations across bright filaments in a sunspot penumbra has become an important new diagnostic of convective gas flows in penumbral filaments. The nature of the…
Break up of returning plasma after the 7 June 2011 filament eruption by Rayleigh-Taylor instabilities
D. E. Innes, R. H. Cameron, L. Fletcher +2
A prominence eruption on 7 June 2011 produced spectacular curtains of plasma falling through the lower corona. At the solar surface they created an incredible display of extreme ul…
Simulations of the solar near-surface layers with the CO5BOLD, MURaM, and Stagger codes
B. Beeck, R. Collet, M. Steffen +6
Radiative hydrodynamic simulations of solar and stellar surface convection have become an important tool for exploring the structure and gas dynamics in the envelopes and atmospher…
Vortices, shocks, and heating in the solar photosphere: effect of a magnetic field
R. Moll, R. H. Cameron, M. Schüssler
Aims: We study the differences between non-magnetic and magnetic regions in the flow and thermal structure of the upper solar photosphere. Methods: Radiative MHD simulations repres…