The Solar Corona3D coronal equilibria, instabilities & numerical MHD
The GeodynamoNumerical models of dynamos & convection in planetary
MHD Stability of a Twisted, Flux Tube Prominence Model (51Kb)
with figures (92Kb)
Effect of Magnetic Shear on the MHD Stability of a Prominence Model (52Kb)
with figures (63Kb) Nonlinear m=0 instability in a flux tube:
Nonlinear MHD evolution of Axisymmetric Line-tied Loops in the Solar Corona
with figures (671Kb) Parker's Braiding Problem:
Flux Braiding: Force-Free Equilibria and Current Sheets (52Kb)
with figures (309Kb) Multigrid Methods in Solar MHD:
Some Practical Aspects of Multigrid Methods In Obtaining Three-Dimensional
Coronal Equilibrium Solutions (53Kb)
with figures (105Kb) Review (Chapman Conference on CMEs):
Topology and Instability of Complex Magnetic Fields (35Kb)
with figures (126Kb) Prominence Equilibria:
MHD model for solar coronal plumes (130kb) Geodynamo and Convection
Magnetoconvection in a rotating spherical shell, incorporating a finitely
conducting inner core (53Kb)
with figures (394Kb)
self-consistent convection driven geodynamo model, incorporating a finitely
conducting differentially rotating inner core (48Kb)
with figures (1.068Mb)
influence of boundary region heterogeneities on the geodynamo (1.249Mb)
602 people have accessed this page since 8 August 1997.
Linear Stability of Prominence Equilibria:
Return to Personnel
of the Solar Theory Group.
Return to the Solar
Theory Group WWW Server.
Return to the School
of Mathematical Sciences www page.
Aaron Longbottom / email@example.com
Last Update 31 October 1996