FARGO: Fast Advection in Rotating Gaseous Objects

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FARGO: Fast Advection in Rotating Gaseous Objects

Post by owlice » Tue Feb 15, 2011 9:49 am

FARGO: Fast Advection in Rotating Gaseous Objects

Abstract: FARGO is an efficient and simple modification of the standard transport algorithm used in explicit eulerian fixed polar grid codes, aimed at getting rid of the average azimuthal velocity when applying the Courant condition. This results in a much larger timestep than the usual procedure, and it is particularly well-suited to the description of a Keplerian disk where one is traditionally limited by the very demanding Courant condition on the fast orbital motion at the inner boundary. In this modified algorithm, the timestep is limited by the perturbed velocity and by the shear arising from the differential rotation. The speed-up resulting from the use of the FARGO algorithm is problem dependent. In the example presented in the code paper below, which shows the evolution of a Jupiter sized protoplanet embedded in a minimum mass protoplanetary nebula, the FARGO algorithm is about an order of magnitude faster than a traditional transport scheme, with a much smaller numerical diffusivity.

Credit: Masset, Frederic

Site: http://fargo.in2p3.fr/-Legacy-archive-
https://ui.adsabs.harvard.edu/abs/2000A%26AS..141..165M

Bibcode: 2011ascl.soft02017M

ID: ascl:1102.017
Last edited by Ada Coda on Sun Jul 19, 2020 6:45 pm, edited 1 time in total.
Reason: Updated code entry.
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