solstice

Compute collected power and efficiencies of a solar plant
git clone git://git.meso-star.com/solstice.git
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commit 45f3cf745209efe18572d814027205953d7e50b5
parent 151b84044f71b7dd40ea6941e3290faba2068f51
Author: Christophe Coustet <christophe.coustet@meso-star.com>
Date:   Fri, 12 May 2017 15:39:19 +0200

Some additions to sun documentation.

Diffstat:
Mdoc/solstice-input.5.ronn | 23++++++++++++-----------
1 file changed, 12 insertions(+), 11 deletions(-)

diff --git a/doc/solstice-input.5.ronn b/doc/solstice-input.5.ronn @@ -276,13 +276,14 @@ to be a dirac distribution (point source sun). The available sun shapes are: * `pillbox`: The `pillbox` distribution defines an uniform intensity over the sun's disk. - Its unique `aperture` parameter is the sun's disk half-angle that is linked - to the apparent size of the sun. + Its single `aperture` parameter is the sun's disk half-angle in degrees, that + is linked to the apparent size of the sun. A typical aperture is 0.2664. * `buie`: - The `buie` distribution, as first discribed in [2]. Its unique `csr` + The `buie` distribution, as first discribed in [2]. Its single `csr` parameter is the ratio between the circumsolar irradiance and the sum of - the circumsolar and sun's disk irradiances. + the circumsolar and sun's disk irradiances. An analysis on typical csr + values can be found in [3]. ## MATERIAL @@ -358,7 +359,7 @@ The available material descriptors are: ### Normal map All the material descriptors, excepted the `virtual`, provide an optional -`normal-map` attribute that defines a path toward a Portable PixMap image [3] +`normal-map` attribute that defines a path toward a Portable PixMap image [4] whose pixels store a normal expressed in the tangent space of the interface. By default the unperturbed tangent space normal is {0,0,1}. The PPM image can be encoded on 8 or 16-bits per component either in ASCII or binary. The @@ -702,14 +703,14 @@ geometry: ## NOTES -* [1]: - YAML Ain't Markup Language - <http://yaml.org> +* [1]: YAML Ain't Markup Language - <http://yaml.org> * [2]: D. Buie, A.G. Monger, C.J. Dey. "Sunshape distributions for - terrestrial solar simulations". Solar Energy, 2003, 74, pp. 113-122. - + terrestrial solar simulations". Solar Energy, 2003, 74, pp. 113-122. <https://www.researchgate.net/publication/256854372_Sunshape_distributions_for_terrestrial_solar_simulations> -* [3]: - Portable PixMap - <http://netpbm.sourceforge.net/doc/ppm.html> +* [3]: D. Buie , C.J. Dey, S. Bosi. "The effective size of the solar cone for + solar concentrating systems". Solar Energy, 2003, 74, pp. 417-427. + <http://http://documents.mx/documents/effective-size-of-solar-cone.html> +* [4]: Portable PixMap - <http://netpbm.sourceforge.net/doc/ppm.html> ## SEE ALSO `solstice`(1), `solstice-receiver`(5)