FLASH: Adaptive Mesh Hydrodynamics Code for Modeling Astroph

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FLASH: Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes

Post by owlice » Sat Oct 30, 2010 5:18 pm

FLASH: Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes

Abstract: The FLASH code, currently in its 4th version, is a publicly available high performance application code which has evolved into a modular, extensible software system from a collection of unconnected legacy codes. FLASH consists of inter-operable modules that can be combined to generate different applications. The FLASH architecture allows arbitrarily many alternative implementations of its components to co-exist and interchange with each other. A simple and elegant mechanism exists for customization of code functionality without the need to modify the core implementation of the source. A built-in unit test framework combined with regression tests that run nightly on multiple platforms verify the code.

Credit: Fryxell, B.; Olson, K.; Ricker, P.; Timmes, F. X.; Zingale, M.; Lamb, D. Q.; MacNeice, P.; Rosner, R.; Truran, J. W.; Tufo, H.

Site: http://flash.uchicago.edu/site/flashcode/
https://ui.adsabs.harvard.edu/abs/2005Ap%26SS.298..341W

Bibcode: 2010ascl.soft10082F

Preferred citation method: Please acknowledge with this text: "The software used in this work was developed in part by the DOE NNSA ASC- and DOE Office of Science ASCR-supported Flash Center for Computational Science at the University of Chicago."

ID: ascl:1010.082
Last edited by Ada Coda on Sat Jun 13, 2020 5:34 pm, edited 1 time in total.
Reason: Updated code entry.
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