stardis-solver

Solve coupled heat transfers
git clone git://git.meso-star.fr/stardis-solver.git
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commit a7f6b5a129924c0e6e598402cbb8a1d83ebd04e4
parent 85842462e270c298f42c829a9277fecaea4ddc8a
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Thu, 31 Mar 2022 09:18:31 +0200

Fix a spelling mistake in the README file

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

diff --git a/README.md b/README.md @@ -29,7 +29,7 @@ The hypothesis these algorithms are based upon are the following: converge the result closer to the solution of a rigorous spectrally-integrated radiative transfer (a difference of temperatures to the power 4 when integrated over the whole spectrum). The higher the recursion - order, to better will be the convergence of the algorithm. + order, the better will be the convergence of the algorithm. In Stardis-Solver the system to simulate is represented by a *scene* whose geometry defines the contour of the object only: in contrast to legacy thermal