High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae

Details High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae High-order methods for the simulation of hydromagnetic instabilities in core-collapse supernovae

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..479r&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 479-481

Astronomy and Astrophysics

Astrophysics

Reconstruction Schemes, Riemann Solvers, Hydromagnetic Instabilities

Scientific paper

We present an assessment of the accuracy of a recently developed MHD code used to study hydromagnetic flows in supernovae and related events. The code, based on the constrained transport formulation, incorporates unprecedented ultra-high-order methods (up to 9th order) for the reconstruction and the most accurate approximate Riemann solvers. We estimate the numerical resistivity of these schemes in tearing instability simulations.

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