activity
20052025
most citedHighly Efficient Modeling of Dynamic Coronal Loops

318 citations · 1k across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2025★ 2 cited

Heating and cooling at a coronal magnetic null

P. J. Cargill, A. W. Hood, D. Johnson

Conductive cooling of the solar corona at a magnetic null is examined. An initial equilibrium is set up, balancing thermal conduction and a constant, spatially uniform coronal heat…

astro-ph.SR2021★ 18 cited

Static and dynamic solar coronal loops with cross-sectional area variations

P. J. Cargill, S. J. Bradshaw, J. A. Klimchuk +1

The Enthalpy Based Thermal Evolution of Loops (EBTEL) approximate model for static and dynamic coronal loops is developed to include the effect of a loop cross-sectional area which…

astro-ph.SR2021

High resolution soft X-ray spectroscopy and the quest for the hot (5-10 MK) plasma in solar active regions

G. Del Zanna, V. Andretta, P. J. Cargill +5

We discuss the diagnostics available to study the 5-10 MK plasma in the solar corona, which is key to understanding the heating in the cores of solar active regions. We present sev…

astro-ph.SR2020★ 29 cited

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.SR2019★ 46 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.SR2017★ 5 cited

Comparison of Methods for modelling Coronal Magnetic Fields

E. E. Goldstraw, A. W. Hood, P. K. Browning +1

Four different approximate approaches used to model the stressing of coronal magnetic fields due to an imposed photospheric motion are compared with each other and the results from…