A tunable birefringent Fabry-Perot interferometer.
Tunable birefringent Fabry-Perot interferometer used in study of solar magnetic fields, using Zeeman effect
SEARCH · Search NASA
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Tunable birefringent Fabry-Perot interferometer used in study of solar magnetic fields, using Zeeman effect
Automatic control of spacing of Fabry-Perot interferometers to transmit at given wavelength
Photographic investigation of arc spectrum of tin by plane and concave grating spectrographs and Fabry-Perot interferometers
High altitude measurement to determine ratio of deuterium to hydrogen in solar atmosphere - Fabry-Perot interferometer
H-alpha line emission in night airglow and helium emission of night airglow with fabry-perot interferometer and electronic image converter
Fabry-Perot interferometer investigations for techniques of millimeter wave measurements and accurate attenuation
Fabry-Perot interferometers used to determine ratio of deuterium to hydrogen in solar atmosphere
Reflection coefficient of cavity tubing as explanation for power level of helium-neon IR FABRY-PEROT interferometer
Fiber-optic bolometers (FOBs) designed for plasma radiation measurement in magnetically confined fusion environments have been previously developed and tested at the DIII-D tokamak. These FOBs utilize a silicon Fabry–Perot interferometer at the fiber tip for temperature measurement and a gold disk as a radiation absorber. This paper presents recent advancements in the development of FOBs with reduced cooling time constants and enhanced temperature tolerance. We also demonstrate high-temperature operation and report findings from irradiation tests. By incorporating a copper sensor holder as a thermal sink and integrating two closely packed sensor heads into a compact design, the cooling time constants were reduced to ∼100 ms in vacuum, while minimizing uncertainties caused by temperature gradients. The FOBs were subjected to heating at 400 °C for five hours, with no observed degradation in noise performance post-heating. High-temperature operation tests were conducted at ∼220 °C using a 404 nm square-wave modulated laser to simulate the plasma radiation. In addition, four FOBs constructed from copper-coated pure-silica fibers were fabricated and underwent irradiation testing, enduring a total γ-radiation dose of 15.2 MGy and a neutron fluence of 1.6 × 10 18 n/cm 2 . As a result, the FOBs maintained their physical integrity and the optical signal shows high visibility throughout the test.
Brillouin scattering in liquids excited by He-Ne maser and observed by Fabry-Perot interferometer, noting acoustic wave velocity and line broadening
Arc spectrum of silicon at low pressure measured with plane and concave grating spectrographs and Fabry-Perot interferometers, identifying new solar lines and energy levels
Measurement of velocity of light - use of interferometer
Fiber-optic bolometers (FOBs) based on a fiber-tipped silicon Fabry–Perot (FP) interferometric temperature sensor and a gold disk absorber have been shown to be an attractive alternative to conventional resistive bolometers for plasma radiation measurement in fusion devices. Either a high-finesse FP or a low-finesse FP can be used, each with trade-offs between noise performance and fabrication complexity. In this paper, we present an FOB design that overcomes these limitations by combining a low-finesse long silicon FP cavity with a large gold disk absorber to achieve enhanced sensitivity and noise performance without increasing the fabrication complexity and the time constant. We also demonstrated a fabrication method for the sensor head facilitated by thermal release tape and precise laser heating. Our FOB demonstrates a temperature resolution of 0.08 mK, a cooling time constant of 230 ms, and a noise equivalent power density of 0.015 W m −2 . This represents an eightfold improvement over previous high-finesse FOBs and 26-fold improvement over previous low-finesse FOBs with similar demodulation bandwidths and similar cooling time constants.
Modified Al-dielectric-Al Fabry-Perot interference filter for isolating Hg 1849 angstrom emission line from Hg 2536 angstrom line
Optical determination of temperature variations throughout solar corona during eclipse of May 30, 1965
Isotope shift measurement for 6328 angstroms helium-neon laser transition
Explore the source record for details and available documents.