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To view the Trough System Costs page, click Dish Collector on the main window's navigation menu. Note that for the trough input pages to be available, the technology option in the Technology and Market window must be Concentrating Solar Power - Dish Stirling System. |
The collector consists of parabolic mirrors, a support structure, and two-axis tracking system. The mirrors focus direct normal solar radiation on the aperture of the receiver. The receiver aperture size is typically optimized to maximize the quantity of reflected solar radiation that enters the receiver and minimize convection and radiation losses out of the aperture.
The relevant sections of the thesis Stirling Dish System Performance Prediction Model (Fraser 2008) https://www.nrel.gov/analysis/sam/pdfs/thesis_fraser08.pdf (4.1 MB) are:
| • | 2.1 Parabolic Concentrator, p 7 |
| • | 3.1 Parabolic Collector Model, p 63 |
| • | Appendix A: TRNSYS Parabolic Collector Model, p 150 |
| • | Appendix A: TRNSYS Parasitic Power Model, p 158 |
Input Variable Reference
The parameters on the Collector page are used to calculate the power output of the collector. The parameters are for a single dish collector, and are assumed to apply to each dish in the solar field.
Mirror Parameters
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Performance
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Table 25. Collector default parameter values.
Variable |
SES |
WGA |
SBP |
SAIC |
Projected Mirror Area |
87.7 |
41.2 |
56.7 |
113.5 |
Total Mirror Area |
91.0 |
42.9 |
60 |
117.2 |
Insolation Cut In |
200 |
275 |
250 |
375 |
Wind Stow Speed |
16 |
16 |
16 |
16 |
Receiver Aperture Diameter for Reference Intercept Factor |
0.184 |
0.14 |
0.15 |
0.38 |
Reference Intercept Factor |
0.995 |
0.998 |
0.93 |
0.90 |
Reference Focal Length of Mirror |
7.45 |
5.45 |
4.5 |
12.0 |