Codes for solar flux calculation dedicated to central receiver system applications: A comparative review

被引：185

作者：

Garcia, Pierre ^{[1
]}

Ferriere, Alain ^{[1
]}

Bezian, Jean-Jacques ^{[2
]}

机构：

[1] CNRS PROMES Lab, F-66120 Font Romeu, France

[2] CNRS LGPSD, F-81013 Albi 9, France

来源：

SOLAR ENERGY | 2008年 / 82卷 / 03期

关键词：

solar flux calculation; central receiver systems; optical modeling; ray-tracing; cone optics;

D O I：

10.1016/j.solener.2007.08.004

中图分类号：

TE [石油、天然气工业]; TK [能源与动力工程];

学科分类号：

0807 ; 0820 ;

摘要：

As we need adapted software to calculate the solar flux concentration through a tower-heliostat field system, an overview of computer codes was performed, detailing their features, strengths and weaknesses. For this a questionnaire was sent to developers or heavy users of codes that are currently used in the concentrated solar power (CSP) community. Answers to this questionnaire make it possible to determine which tool is relevant depending on the objectives of the simulation. Modeling tools for central receiver systems (CRS) can be divided into two main categories, corresponding to two kinds of problems: on one hand those dedicated to system optimization and on the other hand those designed to detailed analysis of the optical performances. A bibliographic study on first generation and developing codes complements this overview of tools that may be interesting for CSP research or industry. (C) 2007 Elsevier Ltd. All rights reserved.

引用

页码：189 / 197

页数：9

共 33 条

[1]

[Anonymous], 1986, HDB SOLAR CENTRAL RE

[2]

Biggs F., 1977, HELIOS COMPUTATIONAL

[3]

Blanco M.J., 2005, P 2005 ASME INT MECH

[4]

*FIN PUBL REP SOLG, 2005, ENK5CT200000333

[5]

GARCIA P, 2006, P SOLARPACES 13 INT

[6]

HENAULT F, 2005, COSAC VERS 2 5

[7]

HENAULT F, 1987, THESIS U PARIS SUD, P35

[8]

IZYGON M, 1987, P SEM HEL SPRING

[9]

Kiera M., 1989, GAST P FIN PRES, P95, DOI [10.1007/978-3-642-83559-9_7, DOI 10.1007/978-3-642-83559-9_7]

[10]

Kiera M., 1986, BESCHREIBUNG HANDHAB

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