arXiv · astro-ph/0108043
Initial magnetic field configurations for 3-dimensional simulations of astrophysical jets
Abstract
We solve, and provide analytical expressions, for current-free magnetic configurations in the context of initial setups of 3-dimensional simulations of astrophysical jets involving an accretion disk corona in hydrostatic balance around a central object. These configurations which thread through the accretion disk and its corona preserve the initial hydrostatic state. This work sets stage for future 3-dimensional jet simulations (including disk rotation and mass-load) where launching, acceleration and collimation mechanisms can be investigated.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
M. Jorgensen, R. Ouyed, M. Christensen. 2001-10-03. Initial magnetic field configurations for 3-dimensional simulations of astrophysical jets. https://doi.org/10.1051/0004-6361%3A20011367
Cite the original work for its findings. Save a collection to share your selection of sources.