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A User's Manual for DELSOL3 - prod.sandia.gov - Sandia National ...

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a final per<strong>for</strong>mance calculation on the optimized system. This difference will be<br />

most noticeable in flux profiles.<br />

The speed of the Hermite method results from the fact that a severely trun-<br />

cated polynomial (6th order) expansion is an accurate approximation to the flux<br />

density. As discussed in Reference 5, the accuracy of the Hermite method in-<br />

creases as the error sources of heliostat per<strong>for</strong>mance and/or their effect on the<br />

flux profile become larger. Specifically, DELSOL becomes more accurate in pre-<br />

dicting the flux and spillage when: (1) the errors increase; (2) the slant range in-<br />

creases; or (3) the size of the heliostat is reduced (either physically or effectively<br />

by focusing or canting).<br />

To calculate the fraction of the flux intercepted by the receiver, Equation<br />

(1II.F-1) must be integrated over the projection of the receiver on the image<br />

plane. The resulting two dimensional integral can be evaluated analytically in one<br />

dimension and numerically, using a 16 point Gaussian quadrature, in the other.<br />

I1I.F-I. More Accurate Images from Canted Heliostats-The normal method<br />

used in DELSOL is to use a single Hermite series to represent the heliostat’s im-<br />

age. When the heliostat to receiver distance is small this can result in a blurring<br />

of the sharp edges of the image. A slower running option which calculates a more<br />

accurate image is available <strong>for</strong> canted heliostats (INDC=l in Namelist HSTAT).<br />

The location of the center of the image from each cant panel is calculated. Then<br />

a separate Hermite series is used to represent the image from each cant panel.<br />

This option can only be used in per<strong>for</strong>mance calculations with a single<br />

aimpoint at the center of the receiver (IAUTOP=l, Namelist REC). Its<br />

effect on an optimized system can be determined by rerunning a per<strong>for</strong>mance cal-<br />

culation on the optimized system with INDC=l.<br />

II1.F-2. When to do Fluz Calculations-Flux calculations should be done ei-<br />

ther to design flux limited systems or to define a detailed flux map of a previously<br />

optimized system. There<strong>for</strong>e, flux calculations should not be done (IFLX=O) dur-<br />

ing an initial per<strong>for</strong>mance calculation. It is recommended that, during system op-<br />

timization, a grid of flux points be defined covering either the entire heat absorb-<br />

ing surface or a known area of concern, and that up to four points from that grid<br />

be checked during optimization to verify that flux limits are not exceeded. During<br />

the final per<strong>for</strong>mance calculation, fluxes should be calculated <strong>for</strong> points over the<br />

entire heat absorbing surface to verify that flux limits have not been exceeded at<br />

any other points than those checked during optimization.<br />

1II.G. Time Independent Losses<br />

The hourly and seasonal variation of: a) atmospheric attenuation from the he-<br />

liostat to the receiver, b) receiver radiation and convection losses, and c) piping<br />

insulation losses are assumed negligible. In addition, mirror and receiver reflec-<br />

tivity, the thermal to electric conversion efficiency, and parasitic loads are repre-<br />

sented by constant time averaged values.<br />

77

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