46 citations · 198 across the 9 of their papers we have counts for
9 papers
The Thickness of Electric Current Sheets and Implications for Coronal Heating
James A. Klimchuk, James E. Leake, Lars K. S. Daldorff +1
The thickness of current sheets is extremely important, especially as it relates to the onset of fast magnetic reconnection. Onset determines how much magnetic free energy can buil…
A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method
C. D. Johnston, A. W. Hood, I. De Moortel +2
We have demonstrated that the Transition Region Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations, success…
Multi-Stranded Coronal Loops: Quantifying Strand Number and Heating Frequency from Simulated Solar Dynamics Observatory (SDO) Atmospheric Imaging Assembly (AIA) Observations
Thomas Williams, Robert W. Walsh, Stephane Regnier +1
Coronal loops form the basic building blocks of the magnetically closed solar corona yet much is still to be determined concerning their possible fine-scale structuring and the rat…
Modelling the solar transition region using an adaptive conduction method
C. D. Johnston, P. J. Cargill, A. W. Hood +3
Modelling the solar Transition Region with the use of an Adaptive Conduction (TRAC) method permits fast and accurate numerical solutions of the field-aligned hydrodynamic equations…
Chromospheric evaporation and phase mixing of Alfvén waves in coronal loops
H. J. Van Damme, I. De Moortel, P. Pagano +1
Phase mixing of Alfvén waves has been studied extensively as a possible coronal heating mechanism but without the full thermodynamic consequences considered self-consistently. It h…
The effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops
C. D. Johnston, P. J. Cargill, P. Antolin +3
Thermal non-equilibrium (TNE) is believed to be a potentially important process in understanding some properties of the magnetically closed solar corona. Through one-dimensional hy…