The “beam down” optics or “solar tower reflector” has been successfully used recently for testing in different projects at the Weizmann Institute of Science. There are currently sufficient data on this technology to evaluate its upscaling for commercial uses. The sizing of a tower reflector (TR) is directly linked to the layout of the heliostat field and the geometry of the ground secondary concentrator (compound parabolic concentrator (CPC)). It depends on its position relative to the aim point of the field, amount of spillage around it, and the allowable solar flux striking the TR. Its position influences the size of the image at the entrance plane of the ground CPC and the spillage around the CPC aperture. The spillage around the CPC is also directly related to the exit diameter of the CPC (equal to the entrance opening of the solar reactor, matching the CPC exit) and therefore linked to the input energy concentration, thermal losses, and working temperature in the reactor. Restrictions on the size of the exit of the CPC can influence the entire design of the optical system. This paper provides the correlations between the main design parameters and their sensitivity analysis. These correlations are based on edge-ray methodology, which provides a quick and sufficiently accurate means for preliminary evaluating large-scale beam down solar plants without the need for detailed design of the heliostat field and considering their errors. The size of the TR and the geometry of the CPC are correlated to the size of the reflective area of the heliostats field (and the power output). Thermal modeling of the TR has been performed, showing the maximum energy flux allowed on the reflector to avoid overheating, using natural cooling to the surrounding air. The current mirrors of the TR are limited to working temperatures of 120130°C to achieve reasonable lifetime. This parameter must be considered when determining the TR position. A key issue discussed in this paper is the amount of spillage around the CPC entrance. To reduce the spillage losses, one needs to increase the size of the exit aperture (although there are practical limitations to this, e.g., due to the size of the reactor’s window). This, however, reduces the concentration and increases the thermal losses from the reactor and requires optimization work.

1.
Guillot
,
E.
,
Epstein
,
M.
,
Wieckert
,
G.
,
Olalde
,
G.
,
Steinfeld
,
A.
,
Santen
,
S.
,
Frommherz
,
U.
,
Kraupl
,
S.
, and
Osinga
,
T.
, 2005, “
Solar Carbothermic Production of Zinc from Zinc Oxide-SOLZINC
,”
Proceedings of ISEC 2005
,
Orlando, FL
, Aug. 6–12; Paper No. ISEC2005-76015.
2.
Kogan
,
A.
,
Kogan
,
M.
, and
Barak
,
S.
, 2005, “
Production of Hydrogen and Carbon by Solar Thermal Methane Splitting. III. Fluidization, Entrainment and Seeding Powder Particles into a Volumetric Solar Receiver
,”
Int. J. Hydrogen Energy
0360-3199,
30
(
1
), pp.
35
43
.
3.
Segal
,
A.
, and
Epstein
,
M.
, 2003, “
Solar Ground Reformer
,”
Sol. Energy
0038-092X,
75
, pp.
479
490
.
4.
Segal
,
A.
, and
Epstein
,
M.
, 1991, “
The Reflective Solar Tower as an Option for High Temperature Central Receivers
,”
Proceedings of the Ninth International Symposium on Solar Thermal Concentrating Technologies
,
Font-Romeu, France
, June 22–26,
J. Phys. IV
1155-4339,
3
, pp.
Pr3
-53–Pr3-
58
.
5.
Segal
,
A.
, and
Epstein
,
M.
, 1999, “
Comparative Performances of Tower-Top and Tower-Reflector Central Solar Receivers
,”
Sol. Energy
0038-092X,
65
(
4
), pp.
206
226
.
6.
Rabl
,
A.
, 1985,
Active Solar Collectors and Their Applications
,
Oxford University Press
,
Oxford
.
7.
Segal
,
A.
, and
Epstein
,
M.
, 1995, “
Optimized Working Temperature of a Solar Central Receiver
,”
Sol. Energy
0038-092X,
75
, pp.
503
510
.
8.
Segal
,
A.
, and
Epstein
,
M.
, 1999, “
Comparative Performances of Tower-Top and Tower-Reflector Central Solar Receivers
,”
Sol. Energy
0038-092X,
65
, pp.
207
226
.
9.
Lipps
,
F. W.
, and
Vant-Hull
,
L. L.
, 1978, “
A Cellwise Method for the Optimization of Large Central Receiver Systems
,”
Sol. Energy
0038-092X,
20
, pp.
505
516
.
10.
Sanchez
,
M.
, and
Romero
,
M.
, 2006, “
Methodology for Generation of Heliostat Field Layout in Central Receiver Systems Based on Yearly Normalized Energy Surfaces
,”
Sol. Energy
0038-092X,
80
,
861
874
.
11.
WINDELSOL 1.0, computer package, 2002, “
Central Receiver Technologies
,” eds. Acia, Ciemat, and Solucar.
12.
Segal
,
A.
, and
Epstein
,
M.
, 1996, “
A Model for Optimization of a Heliostat Field Layout
,”
Solar Thermal Concentrating Technologies
Proceedings of the Eighth International Symposium
,
Köln, Germany
, Oct. 6–11,
C.F.Müller
,
Heidelberg
, pp.
989
998
.
13.
1991,
Solar Power Plants: Fundamentals, Technology, Systems, Economics
,
C. J.
Winter
.
R. L.
Sizmann
, and
L. L.
Vant-Hull
, eds.,
Springer-Verlag
,
Berlin
.
14.
Segal
,
A.
, 1999,
Thermodynamic Approach to the Optimization of Central Solar Energy Systems
, NATO Advanced Study Institute on Thermodynamics and Optimization of Complex Energy Systems;
Kluwer Academic
,
Dordrecht, the Netherlands
, pp.
323
334
.
15.
Segal
,
A.
, and
Epstein
,
M.
, 2000, “
The Optics of the Solar Tower Reflector
,”
Sol. Energy
0038-092X,
69
, pp.
229
241
.
You do not currently have access to this content.