star-line

Structure for accelerating line importance sampling
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commit c126c34e04bbcd6541ec7e392d5529c17b6247b5
parent f2e7291c8a22cf46d1585f4a027f1d27158f67d0
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Mon, 23 Mar 2026 17:38:44 +0100

Use "transmissivity" in the sln-slab man page

It was previously named "transmittance"

Diffstat:
Mdoc/sln-slab.1 | 8++++----
1 file changed, 4 insertions(+), 4 deletions(-)

diff --git a/doc/sln-slab.1 b/doc/sln-slab.1 @@ -36,7 +36,7 @@ .\"""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""" .Sh DESCRIPTION .Nm -calculates the transmittance and the emissivity in a one-dimensional +calculates the transmissivity and the emissivity in a one-dimensional homogeneous slab of arbitrary thickness using a Monte Carlo algorithm that samples the spectral lines that make up the gas mixture. These computations are accelerated by sampling the lines based on the @@ -62,7 +62,7 @@ of the same quantity performed by another radiative transfer code. .Pp The output of .Nm -displays the estimated transmittance and emissivity, their standard +displays the estimated transmissivity and emissivity, their standard deviation, and the number of Monte Carlo realisations rejected due to issues encountered during the computation, such as numerical uncertainty. @@ -133,8 +133,8 @@ The maximum is 3. .Ex -std .\"""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""""" .Sh EXAMPLES -Estimate the transmittance and emissivity between 100 and 2500 cm^-1 for -a slab 2 meters thick. +Estimate the transmissivity and emissivity between 100 and 2500 cm^-1 +for a slab 2 meters thick. The slab consists of a homogeneous gas mixture of H2O, CO2 and CO molecules. The thermodynamic properties of the mixture, such as its pressure,