activity
20172020
most citedThe effects of numerical resolution, heating timescales and background heating on thermal non-equilibrium in coronal loops

46 citations · 106 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2020

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…

astro-ph.SR2020

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…

astro-ph.SR201946 cited

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…

astro-ph.SR201942 cited

A Fast and Accurate Method to Capture the Solar Corona/Transition Region Enthalpy Exchange

C. D. Johnston, S. J. Bradshaw

The brightness of the emission from coronal loops in the solar atmosphere is strongly dependent on the temperature and density of the confined plasma. After a release of energy, th…

astro-ph.SR201718 cited

A new approach for modelling chromospheric evaporation in response to enhanced coronal heating: II Non-uniform heating

C. D. Johnston, A. W. Hood, P. J. Cargill +1

We proposed that the use of an approximate "jump condition" at the solar transition region permits fast and accurate numerical solutions of the one dimensional hydrodynamic equatio…