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The UK MHD Consortium: Goals and Recent Achievements

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High-Performance Computing

Abstract

The UK MHD Consortium was formed in October 1996 and brings together the prominent MHD groups in the UK. The research topics are in Astrophysics with particular emphasis on the Solar Corona (St Andrews University), the Earth’s Geodynamo (Exeter, Glasgow and Newcastle Universities) and dynamo action in turbulent plasmas (Newcastle University).

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References

  1. R. Hollerbach and C. A. Jones, A geodynamo model incorporating a finitely conducting inner core, Phys. Earth Planet Inter. 75:317 (1993).

    Google Scholar 

  2. G. R. Sarson, C. A. Jones and A. W. Longbottom, Convection driven geodynamo models of varying Ekman numbers, Geophys. Astrophys. Fluid Dyn. (submitted 1998).

    Google Scholar 

  3. K. Galsgaard, and A. Nordlund, Heating and Activity of the Solar Corona: 1 Boundary Shearing of an Initially Homogeneous Magnetic Field, J. Geophys, Res. 101:13445 (1996).

    Google Scholar 

  4. K. Galsgaard and A. W. Longbottom, Formation of Prominences by Flux Convergence, Astrophys. J (submitted 1998).

    Google Scholar 

  5. C. R. Evans and J.F. Hawley, Simulation of magnetohydrodynamic flows: a constrained transport method, Astrophys. J. 322:659 (1988).

    Google Scholar 

  6. B. van Leer, Towards the ultimate conservative difference scheme V. A second-order sequel to Godunov’s method, J. Comp. Phys. 32:101 (1979).

    Google Scholar 

  7. T. D. Arber, A. W. Longbottom and R. A. M. Van der Linden, Current sheet formation and the effect of anomalous resistivity in unstable coronal loops. In preparation.

    Google Scholar 

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© 1999 Springer Science+Business Media New York

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Hood, A. et al. (1999). The UK MHD Consortium: Goals and Recent Achievements. In: Allan, R.J., Guest, M.F., Simpson, A.D., Henty, D.S., Nicole, D.A. (eds) High-Performance Computing. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-4873-7_56

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  • DOI: https://doi.org/10.1007/978-1-4615-4873-7_56

  • Publisher Name: Springer, Boston, MA

  • Print ISBN: 978-1-4613-7211-0

  • Online ISBN: 978-1-4615-4873-7

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