DISCO: 3-D moving-mesh magnetohydrodynamics package

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Ada Coda
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DISCO: 3-D moving-mesh magnetohydrodynamics package

Post by Ada Coda » Mon May 30, 2016 11:04 pm

DISCO: 3-D moving-mesh magnetohydrodynamics package

Abstract: DISCO evolves orbital fluid motion in two and three dimensions, especially at high Mach number, for studying astrophysical disks. The software uses a moving-mesh approach with a dynamic cylindrical mesh that can shear azimuthally to follow the orbital motion of the gas, thus removing diffusive advection errors and permitting longer timesteps than a static grid. DISCO uses an HLLD Riemann solver and a constrained transport scheme compatible with the mesh motion to implement magnetohydrodynamics.

Credit: Duffell, Paul C.

Site: https://github.com/duffell/Disco
https://ui.adsabs.harvard.edu/abs/2016ApJS..226....2D

Bibcode: 2016ascl.soft05011D

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2016ApJS..226....2D

ID: ascl:1605.011
Last edited by Ada Coda on Sun Oct 04, 2020 4:17 pm, edited 1 time in total.
Reason: Updated code entry.

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