solstice

Compute collected power and efficiencies of a solar plant
git clone git://git.meso-star.com/solstice.git
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commit c26b5612c98f16e8fd64726f746c8c44bac67bae
parent 59ce5570ecde3624f641b82098d54be4ec011119
Author: Christophe Coustet <christophe.coustet@meso-star.com>
Date:   Mon, 18 Sep 2017 12:43:40 +0200

Documentation improvement.

Diffstat:
Mdoc/solstice-output.5.txt | 98+++++++++++++++++++++++++++++++++++++++++--------------------------------------
1 file changed, 51 insertions(+), 47 deletions(-)

diff --git a/doc/solstice-output.5.txt b/doc/solstice-output.5.txt @@ -89,8 +89,8 @@ _______ <#samples> ::= INTEGER # in [0, INF) <#failed> ::= INTEGER # in [0, INF) -<global> ::= <potential-irradiance> - <absorbed-irradiance> +<global> ::= <potential-flux> + <absorbed-flux> <cos-factor> <shadow-loss> <missing-loss> @@ -112,7 +112,7 @@ _______ <front> ::= <side> <back> ::= <side> -<side> ::= "<absorbed-irradiance> <irradiance> +<side> ::= "<absorbed-flux> <incoming-flux> <materials-loss> <atmospheric-loss> <efficiency>" @@ -139,7 +139,7 @@ _______ <rcvXprim-front> ::= <rcvXprim-side> <rcvXprim-back> ::= <rcvXprim-side> -<rcvXprim-side> ::= "<absorbed-irradiance> <irradiance> +<rcvXprim-side> ::= "<absorbed-flux> <incoming-flux> <materials-loss> <atmospheric-loss>" ------------------------------------- @@ -160,11 +160,11 @@ _______ <azimuth> ::= REAL # Degrees in [0, 360[ <elevation> ::= REAL # Degrees in [0, 90] -<potential-irradiance>::= <estimate> -<absorbed-irradiance> ::= <estimate> +<potential-flux> ::= <estimate> +<absorbed-flux> ::= <estimate> <atmospheric-loss> ::= <estimate> <cos-factor> ::= <estimate> -<irradiance> ::= <estimate> +<incoming-flux> ::= <estimate> <missing-loss> ::= <estimate> <materials-loss> ::= <estimate> <shadow-loss> ::= <estimate> @@ -200,27 +200,31 @@ the exact number of lines being part of the headers. Currently this number is 7. Each global result is a pair of real numbers: the expected value and its standard error. The global results are, in this order: -- *potential-irradiance*: maximum irradiance that all the primary - geometries could intercept if properly oriented; -- *absorbed-irradiance*: absorbed part of the irradiance reaching any - receiver geometry. At most equal to potential irradiance; -- *cos-factor*: fraction of incoming irradiance not intercepted by the - primary geometries due to their orientation; -- *shadow-loss*: irradiance lost before reaching primary geometries due to the - shadow of another geometry; -- *missing-loss*: irradiance that reaches a primary geometry, but not - absorbed by a receiver; this irradiance could have been blocked along its - path, can have missed the receivers, or can have reach a receiver but - without being absorbed; -- *materials-loss*: additional irradiance that could have been absorbed - by receivers if no absorption had occurred on non-receivers material until then; -- *atmospheric-loss*: irradiance that could have been absorbed by - receivers if atmospheric extinction had not been taken into account. +- *potential-flux*: maximum flux that all the primary + geometries could intercept if properly oriented and flat-shaped; +- *absorbed-flux*: absorbed part of the flux reaching any + receiver geometry. At most equal to the potential flux; +- *cos-factor*: cos of the angle between the sun direction and the normal of + the primary surfaces (average cos over all primary geometries); +- *shadow-loss*: potential flux intercepted by another geometry before reaching + a primary geometry. +- *missing-loss*: part of the flux that reaches a primary geometry, follows a + radiative path, but is not absorbed; this flux could have bounced on geometries, + including receivers, but without being absorbed; +- *materials-loss*: total flux absorbed by non-receivers along radiative paths; + includes both surface and volume absorption; +- *atmospheric-loss*: total flux extinction by the atmosphere along radiative paths. + +This results can be used to check conservation of energy: + +potential-flux * cos-factor and (absorbed-flux + shadow-loss + +missing-loss + materials-loss + atmospheric-loss) +should be equal whithin their respective uncertainty ranges. Per receiver results ~~~~~~~~~~~~~~~~~~~~ -After the global results, the output includes various per-receiver lines, one +Following global results, the output includes various per-receiver lines, one line per receiver, the exact number of lines being part of the headers. Each line contains the following data: @@ -236,13 +240,13 @@ The estimates of the *front* and *back* sides are listed bellow. Note that each of the following estimates is actually a pair of real numbers: the expected value and its standard error. -- *absorbed-irradiance*: irradiance absorbed by the receiver side; -- *irradiance*: irradiance that reaches the receiver side; -- *materials-loss*: irradiance that could have been absorbed by the +- *absorbed-flux*: flux absorbed by the receiver side; +- *incoming-flux*: flux that reaches the receiver side; +- *materials-loss*: additional flux that could have been absorbed by the receiver side if no absorption had occurred on non-receivers material until then; -- *atmospheric-loss*: irradiance that could have been absorbed by the +- *atmospheric-loss*: additional flux that could have been absorbed by the receiver side if atmospheric extinction had not been taken into account; -- *efficiency*: fraction of incoming irradiance absorbed by the receiver side. +- *efficiency*: fraction of potential flux absorbed by the receiver side. Both *front* and *back* side estimates are output, even if the receiver has only a single receiving side. In this case, the results of the non-receiving @@ -251,7 +255,7 @@ side are meaningless (invalid -1 value). Per primary results ~~~~~~~~~~~~~~~~~~~ -After the per-receiver results, the output includes various per-primary result +Following the per-receiver results, the output includes various per-primary result lines, one line per primary geometry, the exact number of lines being part of the headers. Each line contains: @@ -262,15 +266,15 @@ the headers. Each line contains: - *area*: area of the primary geometry; - *#sample*: number of Monte-Carlo experiments sampled on the primary geometry; -- *cos-factor*: expected value and standard error of the fraction of incoming - irradiance not intercepted by the primary geometry due to its orientation; -- *shadow-loss*: expected value and standard error of the irradiance lost - before reaching the primary geometry due to the shadow of another geometry. +- *cos-factor*: cos of the angle between the sun direction and the normal of + the primary surface (average cos on the primary geometry); +- *shadow-loss*: potential flux intercepted by another geometry before reaching + the primary geometry of interest. Per receiver and per primary results ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ -After the per-primary results, the output includes various result lines, each +Following the per-primary results, the output includes various result lines, each describing the contribution of a primary geometry to a given receiver. The total number of such lines is the number of receivers times the number of primary geometries. Each line contains: @@ -284,14 +288,14 @@ The estimated values of *rcvXprim-front* and *rcvXprim-back* are listed bellow. Each of these estimates is actually a pair of real numbers: the expected value and its standard error. -- *absorbed-irradiance*: irradiance absorbed by the receiver side coming +- *absorbed-flux*: flux absorbed by the receiver side coming from the primary geometry; -- *irradiance*: irradiance reaching the receiver side coming from the primary +- *incoming-flux*: flux reaching the receiver side coming from the primary geometry; -- *materials-loss*: irradiance that could have been absorbed by the +- *materials-loss*: additional flux that could have been absorbed by the receiver side coming from the primary geometry if no absorption had occurred on non-receivers material until then; -- *atmospheric-loss*: irradiance that could have been absorbed by +- *atmospheric-loss*: additional flux that could have been absorbed by the receiver side coming from the primary geometry if atmospheric extinction had not been taken into account. @@ -303,13 +307,13 @@ Receiver map ~~~~~~~~~~~~ A receiver defined in the submitted *solstice-receiver*(5) file, can have a -per-primitive irradiance estimate if its *per_primitive* flag is active. In +per-primitive incoming-flux estimate if its *per_primitive* flag is active. In this case, *solstice*(1) generates a *receiver-map* that is actually an ASCII VTK file [2] that stores the triangular mesh of the receiver and, for each -triangle, the estimate of its associated irradiance. The "definition" of the +triangle, the estimate of its associated incoming-flux. The "definition" of the receiver map is thus controlled by the discretisation of the receiver's shape, as described in the *solstice-input*(5) file. Note that to obtain a good -estimate of the per-triangle irradiance, one have to ensure that the number +estimate of the per-triangle incoming-flux, one have to ensure that the number of per-triangle experiments is sufficient regarding the targeted accuracy. Since only a small fraction of the overall sampled radiative paths reach a given triangle, the total number of experiments required through the *-n* @@ -317,9 +321,9 @@ option of *solstice*(1) should be increased significantly, as 1 or 2 order of magnitude. If only the front or the back side of the receiver is active, then only one set -of per triangle irradiance estimate is written. If the *side* attribute of -the receiver is set to *FRONT_AND_BACK*, the irradiance estimate for the -front facing triangles are written before to the estimate of the back facing +of per triangle incoming-flux estimate is written. If the *side* attribute of +the receiver is set to *FRONT_AND_BACK*, the incoming-flux estimates for the +front facing triangles are written before the estimates of the back facing ones. The following grammar gives a brief description of the formatting of a *VTK-RECEIVER-MAP*. Please refer to the VTK format specification [2] for more informations on the VTK file format. @@ -352,8 +356,8 @@ VTK-RECEIVER-MAP ::= # vtk DataFile Version 2.0 <map-side-data> ::= SCALARS <side-name> float 2 LOOKUP_TABLE default - <irradiance> - [ <irradiance> ... ] + <incoming-flux> + [ <incoming-flux> ... ] <map-side-name> ::= Front_faces | Back_faces