Accurate measurements of thermal radiation from a tungsten photonic lattice
Creators
- 1. Sandia National Laboratories, P.O. Box 5800, Albuquerque, New Mexico 87185 (United States)
Description
Recently, photonic lattice structures have become available that are fabricated from refractory materials such as tungsten and thus stable in vacuo at high temperatures. Such structures can be tailored to exhibit optical properties that are not achievable with ordinary optical materials. In particular, photonic lattices can be designed to suppress thermal emission in undesired spectral regions, and can thereby enhance the overall energy efficiency of emission at useful wavelengths. We report measurements of the thermal emission spectra of tungsten photonic lattices in the wavelength range 3 to 24 μm. Suppression of thermal emission at wavelengths longer than the photonic bandedge (∼6 μm) is observed, along with significant emission at shorter wavelengths. We show that from 404 to 546 K the spectral emissivity E(λ) is temperature independent and approaches [1-R(λ)], where R(λ) is the measured specular reflectance spectrum. These results are in accord with Kirchhoff's law
Additional details
Identifiers
- DOI
- 10.1063/1.1941460;
Publishing Information
- Journal Title
- Applied Physics Letters
- Journal Volume
- 86
- Journal Issue
- 24
- Journal Page Range
- p. 244105-244105.3
- ISSN
- 0003-6951
- CODEN
- APPLAB
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37017589
- Subject category
- S36: MATERIALS SCIENCE;
- Descriptors DEI
- CRYSTALS; EMISSION SPECTRA; EMISSIVITY; ENERGY CONSERVATION; ENERGY EFFICIENCY; REFLECTIVITY; REFRACTORIES; TEMPERATURE DEPENDENCE; TEMPERATURE RANGE 0400-1000 K; THERMAL RADIATION; TUNGSTEN
- Descriptors DEC
- EFFICIENCY; ELECTROMAGNETIC RADIATION; ELEMENTS; METALS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; REFRACTORY METALS; SPECTRA; SURFACE PROPERTIES; TEMPERATURE RANGE; TRANSITION ELEMENTS
Optional Information
- Notes
- (c) 2005 American Institute of Physics