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C. D. Johnston

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • cs.CE1
ORCID 0000-0003-4023-9887

identity via Semantic Scholar / OpenAlex

most citedAdvancing parabolic operators in thermodynamic MHD models II: Evaluating a Practical Time Step Limit for Unconditionally Stable Methods

1 citations · 1 across the 3 of their papers we have counts for

collaborators

3 papers

cs.CE2024★ 1 cited

Advancing parabolic operators in thermodynamic MHD models II: Evaluating a Practical Time Step Limit for Unconditionally Stable Methods

Ronald M. Caplan, Craig D. Johnston, Lars K. S. Daldoff +1

Unconditionally stable time stepping schemes are useful and often practically necessary for advancing parabolic operators in multi-scale systems. However, serious accuracy problems…

astro-ph.SR2023

Heating and cooling in stellar coronae: coronal rain on a young Sun

Simon Daley-Yates, Moira M. Jardine, Craig D. Johnston

Recent observations of rapidly-rotating cool dwarfs have revealed Hα line asymmetries indicative of clumps of cool, dense plasma in the stars' coronae. These clumps may be either…

astro-ph.SR2023

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…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.