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Radiative performance of rare earth garnet thin film selective emitters

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.47031· OSTI ID:165962
 [1]; ;  [2]
  1. Kent State University, Kent, Ohio 44242 (United States)
  2. NASA Lewis Research Center, Cleveland, Ohio 44135 (United States)
In this paper we present the first emitter efficiency results for the thin film 40% Er-1.5% Ho YAG (Yttrium Aluminum Garnet, Y{sub 3}Al{sub 5}O{sub 12}) and 25% Ho YAG selective emitter at 1500 K with a platinum substrate. Spectral emittance and emissive power measurements were made (1.2{lt}{lambda}{lt}3.2 {mu}m). Emitter efficiency and power density are significantly improved with the addition of multiple rare earth dopants. Predicted efficiency results are presented for an optimized (equal power density in the Er, {sup 4}I{sub 15/2}{minus}{sup 4}I{sub 13/2} {at}1.5 {mu}m, and Ho, {sup 5}I{sub 7}{minus}{sup 5}I{sub 8} {at}2.0 {mu}m emission bands) Er-Ho YAG thin film selective emitter. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.
Sponsoring Organization:
USDOE
OSTI ID:
165962
Report Number(s):
CONF-940101--
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 321; ISSN 0094-243X; ISSN APCPCS
Country of Publication:
United States
Language:
English