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pro vyhledávání: '"Johnston, Craig D."'
Unconditionally stable time stepping schemes are useful and often practically necessary for advancing parabolic operators in multi-scale systems. However, serious accuracy problems may emerge when taking time steps that far exceed the explicit stabil
Externí odkaz:
http://arxiv.org/abs/2403.01004
Recent observations of rapidly-rotating cool dwarfs have revealed H$\alpha$ line asymmetries indicative of clumps of cool, dense plasma in the stars' coronae. These clumps may be either long-lived (persisting for more than one stellar rotation) or dy
Externí odkaz:
http://arxiv.org/abs/2309.04264
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 build up in a field before it is explosively released. This has implicatio
Externí odkaz:
http://arxiv.org/abs/2307.13825
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 rate of heat deposition within them. Using an improved multi-stranded loo
Externí odkaz:
http://arxiv.org/abs/2105.12499
Akademický článek
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Publikováno v:
Johnston, Craig D. Hood, Alan W. De Moortel, Ineke Pagano, Paolo Howson, Thomas A. . A fast multi-dimensional magnetohydrodynamic formulation of the transition region adaptive conduction (TRAC) method. Astronomy and Astrophysics (A & A). 2021, 654
Astronomy and Astrophysics (A & A)
Astronomy and Astrophysics (A & A)
Externí odkaz:
http://hdl.handle.net/10852/90046
https://www.duo.uio.no/bitstream/handle/10852/90046/1/aa40987-21.pdf
https://www.duo.uio.no/bitstream/handle/10852/90046/1/aa40987-21.pdf
Publikováno v:
Van Damme, H. J. de Moortel, Ineke Pagano, P. Johnston, Craig D. . Chromospheric evaporation and phase mixing of Alfvén waves in coronal loops. Astronomy and Astrophysics (A & A). 2020, 635
Astronomy and Astrophysics (A & A)
Astronomy and Astrophysics (A & A)
Externí odkaz:
http://hdl.handle.net/10852/82981
https://www.duo.uio.no/bitstream/handle/10852/82981/2/aa37266-19.pdf
https://www.duo.uio.no/bitstream/handle/10852/82981/2/aa37266-19.pdf
Autor:
Johnston, Craig D., Cargill, P. J., Hood, A. W., de Moortel, Ineke, Bradshaw, S. J., Vassekar, A. C.
Publikováno v:
Johnston, Craig D. Cargill, P. J. Hood, A. W. de Moortel, Ineke Bradshaw, S. J. Vassekar, A. C. . Modelling the solar transition region using an adaptive conduction method. Astronomy and Astrophysics (A & A). 2020, 635
Astronomy and Astrophysics (A & A)
Astronomy and Astrophysics (A & A)
Externí odkaz:
http://hdl.handle.net/10852/82980
https://www.duo.uio.no/bitstream/handle/10852/82980/2/aa36979-19.pdf
https://www.duo.uio.no/bitstream/handle/10852/82980/2/aa36979-19.pdf