Assessment of the potential improvement due to multiple apertures in central receiver systems with secondary concentrators

被引:154
作者
Schmitz, M [1 ]
Schwarzbözl, P
Buck, R
Pitz-Paal, R
机构
[1] Deutsch Zentrum Luft & Raumfahrt EV DLR, Solar Res, D-51147 Cologne, Germany
[2] Deutsch Zentrum Luft & Raumfahrt EV DLR, Solar Res, D-70569 Stuttgart, Germany
关键词
solar thermal power; central receiver system; CRS; gas turbine; combined cycle; multiple apertures; heliostat field; HFLCAL;
D O I
10.1016/j.solener.2005.02.012
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
When striving for maximum efficiencies in solar thermal central receiver systems (CRS) the use of gas turbines with bottoming cycles is inevitable. Pressurized volumetric receivers have proven their feasibility and good performance, and their integration into gas turbine cycles has been demonstrated. One disadvantage of this system is the necessity to use secondary concentrators. The sunlight has to be concentrated into the relatively small glass windows of the receiver, which leads to a limited view cone. This means that of all the possible heliostat positions around the tower, only those within the ellipse, resulting from the section boundary of the view cone with the ground plane, are usable. For small systems, for which tower costs are small, the resulting heliostat field layout is similar. with or without secondary concentrator. For large systems, which are more cost-effective, tower costs become significant, and the losses due to atmospheric attenuation and spillage dominate over the cosine losses. Thus, the purely North-oriented fields become increasingly sub-optimal. This article shall demonstrate at what power levels this problem can be alleviated by not using a single, North-oriented aperture, but up to six apertures-each of them associated with a separate heliostat field. (c) 2005 Elsevier Ltd. All rights reserved.
引用
收藏
页码:111 / 120
页数:10
相关论文
共 15 条
[1]  
Becker M., 1989, GAST GAS COOLED SOLA
[2]  
BUCK R, 2000, IEA SOL THERM 2000 I, P95
[3]  
HILLESLAND T, 1990, SOLAR THERMAL TECHNO, P165
[4]  
JONES S, 2003, ISES SOL WORLD C 14
[5]   The DIAPR: A high-pressure, high-temperature solar receiver [J].
Karni, J ;
Kribus, A ;
Doron, P ;
Rubin, R ;
Fiterman, A ;
Sagie, D .
JOURNAL OF SOLAR ENERGY ENGINEERING-TRANSACTIONS OF THE ASME, 1997, 119 (01) :74-78
[6]  
KIERA M, 1989, GAST P FIN PRES SPRI, P95
[7]  
Leary P.L., 1979, SAND778280 SAND LAB, P14
[8]  
MANCINI T, 2000, 3100 PACES
[9]   Representative terrestrial solar brightness profiles [J].
Neumann, A ;
Witzke, A ;
Jones, SA ;
Schmitt, G .
JOURNAL OF SOLAR ENERGY ENGINEERING-TRANSACTIONS OF THE ASME, 2002, 124 (02) :198-204
[10]  
Pitman C.L., 1982, ASES PROGR SOLAR ENE, P1247