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Evaluation of the evacuated solar annular receivers used at the midtemperature solar systems test facility (MSSTF)

Technical Report ·
OSTI ID:6082886

Experimental studies at the Sandia/DOE Midtemperature Solar Systems Test Facility (MSSTF) using the parabolic-cylindrical collector field subsystem are described. Tests evaluated vacuum integrity characteristics of ten glass-to-metal sealed concentric-cylinder receivers installed at the MSSTF in May 1977. Additional testing measured heat-loss reductions and related collector performance gains possible by annulus gas evacuation. Structural defects in four receivers and gas desorption from the receiver tubes at temperatures > 470/sup 0/K necessitated continuous annulus gas evacuation. Pressure rises of 1.8 x 10/sup -4/ Pa/s and 2.2 x 10/sup -2/ Pa/s, measured with receiver tube surfaces at 443/sup 0/K and 578/sup 0/K, respectively, are indicative of the outgassing. One-sun heat-loss and collector efficiency tests were performed with air-filled annular spaces maintained at 8.379 x 10/sup 4/ Pa (atmospheric pressure) and at pressures < 10 Pa. Overall collector efficiency improved by 3.5 to 9% and one-sun heat losses were reduced by 20 to 50%, depending upon operating temperature, annulus pressures, and insolation. Failure of the receiver assemblies to maintain annulus pressures below 1 Pa precluded expected overall efficiency improvements of 11 to 12%. Further, onsite vacuum maintenance was proved unfeasible because of the extensive pumpout manifolding and the additional manpower, parasitic energy, and capital equipment costs required.

Research Organization:
Sandia Labs., Albuquerque, NM (USA)
DOE Contract Number:
EY-76-C-04-0789
OSTI ID:
6082886
Report Number(s):
SAND-78-0983
Country of Publication:
United States
Language:
English