stardis-solver

Solve coupled heat transfers
git clone git://git.meso-star.fr/stardis-solver.git
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commit 2bfab77721b5c4060317343582ec2d0caa6842a9
parent 9f4dcb4c11e27b959196aad0c7685cc4ae62cc89
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Sat, 31 Mar 2018 12:09:25 +0200

Merge branch 'release_0.1' into develop

Diffstat:
MREADME.md | 14+++++++++++++-
Mcmake/CMakeLists.txt | 2+-
2 files changed, 14 insertions(+), 2 deletions(-)

diff --git a/README.md b/README.md @@ -1,7 +1,7 @@ # Stardis The purpose of this library is to solve coupled convecto - conducto - radiative -thermal problems. +thermal problems in 2D and 3D environments. ## How to build @@ -23,6 +23,18 @@ variable the install directories of its dependencies. ## Release notes +### Version 0.1 + +- Add the support of radiative temperature. +- Add the `sdis_camera` API : it defines a pinhole camera into the scene. +- Add the `sdis_accum_buffer` API : it is a pool of MC accumulators, i.e. a sum + of MC weights and square weights. +- Add the `sdis_solve_camera` function : it relies on a `sdis_camera` and a + `sdis_accum_buffer` to compute the radiative temperature that reaches each + pixel of an image whose definition is defined by the caller. Note that + actually this function uses the same underlying MC algorithm behind the + `sdis_solve_probe` function. + ### Version 0.0 First version and implementation of the Stardis solver API. diff --git a/cmake/CMakeLists.txt b/cmake/CMakeLists.txt @@ -40,7 +40,7 @@ rcmake_append_runtime_dirs(_runtime_dirs RSys Star3D StarSP) # Configure and define targets ################################################################################ set(VERSION_MAJOR 0) -set(VERSION_MINOR 0) +set(VERSION_MINOR 1) set(VERSION_PATCH 0) set(VERSION ${VERSION_MAJOR}.${VERSION_MINOR}.${VERSION_PATCH})