stardis

Perform coupled heat transfer calculations
git clone git://git.meso-star.fr/stardis.git
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commit 6971bb392f01ed75e35f4a4e0ce70e0298c0e813
parent 484ad0894489549f10f8e5dea1e26711faf2a203
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed, 24 Apr 2024 16:08:40 +0200

Small update of the DESCRIPTION section of stardis manual

Diffstat:
Mdoc/stardis.1.in | 14+++++++++++---
1 file changed, 11 insertions(+), 3 deletions(-)

diff --git a/doc/stardis.1.in b/doc/stardis.1.in @@ -103,15 +103,23 @@ the presence of high temperature gradients. Increasing the Picard order may be necessary in this case, until the required convergence is reached. .Pp -A main property of this approach is that the resulting algorithms do -not rely on a volumic mesh of the system: only the representation -of interfaces is necessary. +One of the key features of +.Nm +is that its algorithms are not based on a volumetric mesh of the system: +only the representation of its interfaces is required. +And these are used only as a description of the system, not as a basis +for calculation, whose discretization would have an impact on the +accuracy of estimates. .Pp .Nm implements mixed parallelism. On a single computer (that is, a node), it uses shared memory parallelism while it relies on Message Passing Interface (MPI) to parallelize calculations between multiple nodes. +.Nm +can therefore be launched either directly or via a process launcher such as +.Xr mpirun 1 +to distribute the calculation on several computers. .Pp The options are as follows: .Bl -tag -width Ds