star-schiff

Library for estimating radiative properties
git clone git://git.meso-star.com/star-schiff.git
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commit 3a834566538d274ca1a7ea67f2524ad24a769487
parent 99ef5ec9c665b0e259deb46f727e38722fb82186
Author: Vincent Forest <vincent.forest@meso-star.com>
Date:   Wed, 30 Mar 2016 14:50:55 +0200

Fix some misspellings and update the README file

Diffstat:
MREADME.md | 42+++++++++++++++++++-----------------------
1 file changed, 19 insertions(+), 23 deletions(-)

diff --git a/README.md b/README.md @@ -1,25 +1,21 @@ # Star Schiff -The purpose of this library is to numericaly solve the radiative properties of +The purpose of this library is to numerically solve the radiative properties of soft particles with respect to an "Approximation Method for Short Wavelength or -High-Energy Scattering" (L. Schiff, 1956). - -It will estimate total cross-sections (absorption, scattering and -extinction cross-sections) in addition to the phase -function, its cumulative and its inverse cumulative, for a mixture of -different particule types. - -A given type of particule is defined by its optical properties -(refractive index, provided at various wavelengths) -and any user-defined geometry distribution. - -The Monte-Carlo Method is used in order to solve Maxwell's equations -within Schiff's approximation, as presented in -[Charon et al. 2015](http://www.sciencedirect.com/science/article/pii/S0022407315003283). The -main advantages of using this method are: the possibility to address -any shape of particule, and the fact results are provided with a -numerical accuracy. The user has therefore the ability to increase the -computation time in order to obtain more accurate results if needed. +High-Energy Scattering" (L. Schiff, 1956). The Monte-Carlo Method is used in +order to solve Maxwell's equations within Schiff's approximation, as presented +in +[Charon et al.2015](http://www.sciencedirect.com/science/article/pii/S0022407315003283). +The main advantages of using this method are: the possibility to address any shape +of particle, and the results are provided with a numerical accuracy. The user +has therefore the ability to increase the computation time in order to obtain +more accurate results if needed. + +Monte-Carlo is used to estimates total cross-sections (absorption, scattering +and extinction cross-sections) in addition to the phase function, its +cumulative and its inverse cumulative, for a mixture of several particles. +These set of particles is defined by its optical properties (refractive index, +provided at various wavelengths) and a geometry distribution that controls the ## How to build @@ -38,10 +34,10 @@ the one of the RCMake package. ## License -Star-Schiff is developped by [|Meso|Star>](http://www.meso-star.com) for the -the [National Center for Scientific Research](http://www.cnrs.fr/index.php) -(CNRS). It is a free software copyright (C) CNRS 2015-2016 released under the -[OSI](http://opensource.org)-approved GPL v3.0 license. You are welcome to +Star-Schiff is developed by [|Meso|Star>](http://www.meso-star.com) for the +[National Center for Scientific Research](http://www.cnrs.fr/index.php) (CNRS). +It is a free software copyright (C) CNRS 2015-2016 released under the +[OSI](http://opensource.org)-approved GPL v3+ license. You are welcome to redistribute it under certain conditions; refer to the COPYING file for details.