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

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THT<br />

TOWL<br />

TOWD<br />

IREC<br />

W<br />

H<br />

RRECL<br />

IAUTOP<br />

186<br />

Namelist REC<br />

“Tower height.” The elevation, in meters, of the<br />

center of external receiver or cavity aperture<br />

above the heliostat pivot point, not ground level.<br />

Default: THT = 175.0 (m) (II.E,IV.C-S,V.A-4)<br />

The shadow cast by the tower and receiver is modeled its<br />

the shadow cast by a cylinder that is TOWL meters tall<br />

measured above the heliostat pivot points) and has a<br />

6 iameter of TOWD meters.<br />

Default: TOWL = 175.0 (m)<br />

TOWD = 10.0 (m) (III.E-2,IV.A-4)<br />

Parameter specifying type of receiver:<br />

= 0, vertical cylindrical external receiver;<br />

= 1, cavity with aperture(s) of elliptical cross<br />

section;<br />

= 2, cavity with aperture(s) of rectangular cross<br />

section.<br />

= 3, elliptical shape flat plate receiver(s)<br />

= 4, rectangular shape flat plate receiver(s)<br />

Default: IREC = 0<br />

(II.E,IV.C-3)<br />

Diameter, in meters, of an external receiver. For flat<br />

plates or cavities, W is twice the horizontal distance<br />

from the center of the aperture or flat plate to the<br />

tower centerline.<br />

Default: W = 16.0 (m) (11. E,IV.C-3)<br />

Height, in meters, of an external receiver.<br />

Height of cavity heat absorbing surface. If<br />

H = 16.0, defaults to l.lxRY (cavity).<br />

Not needed <strong>for</strong> flat plates.<br />

Default: H = 16.0 (m) (11. E ,IV .C-3)<br />

H = l.lxRY [ ~ ~ ~ ~ ~ t ’ y )<br />

Fraction of the incident power absorbed by the receiver<br />

be<strong>for</strong>e radiation and convection losses, but after<br />

receiver reflection loss:<br />

RRECL = Powcsr iucirl(*ut -Power rc.fle.c fed<br />

P,)wc*r irrridviit<br />

Default: RRECL = 0.965 (1II.G-2)<br />

Control parameter identifying aiming strategy:<br />

= 0, single aim point at center of receiver;<br />

= 1, code calculated time dependent 1-d “smart”<br />

aiming strategy; heliostat images are spread<br />

out along the “height” of the receiver or<br />

aperture to reduce the peak flux and flux<br />

gradients with no increase in spillage.

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