stardis-solver

Solve coupled heat transfers
git clone git://git.meso-star.fr/stardis-solver.git
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commit dd2e030c17b514f61e83ce83dd4dc5c4299a9497
parent 507e409671de06a36a5b2f2322cef51790012bcf
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Thu,  3 Mar 2022 16:39:21 +0100

Fix a typo in the README.md file

Diffstat:
MREADME.md | 2+-
1 file changed, 1 insertion(+), 1 deletion(-)

diff --git a/README.md b/README.md @@ -20,7 +20,7 @@ The hypothesis these algorithms are based upon are the following: - *convection*: fluid media are supposed to be isothermal, even if their temperature may vary with time. This hypothesis relies on the assumption of perfectly agitated fluids. -- *radiation*: local radiative transfer is solved by a iterative numerical +- *radiation*: local radiative transfer is solved by an iterative numerical method (Picard algorithm) that requires the knowledge of a reference temperature field. At the basic level (one level of recursion), and using a uniform reference temperature field, this algorithm translates into the