stardis-solver

Solve coupled heat transfers
git clone git://git.meso-star.fr/stardis-solver.git
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commit fc8a6fb357cdd864bca7a007bb71eb0365cdecaf
parent 870978c14925cc5b66dd4589503ff4d39e2cfb5a
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Sat, 31 Mar 2018 12:04:53 +0200

Write the 0.1 release note

Diffstat:
MREADME.md | 14+++++++++++++-
1 file changed, 13 insertions(+), 1 deletion(-)

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.