Shock tube measurements of Van der Waals broadened silicon lines.
Van der Waals broadened Si lines measurements using shock tube and scanning Fabry-Perot interferometer
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Van der Waals broadened Si lines measurements using shock tube and scanning Fabry-Perot interferometer
High resolution spectral scans of alpha Herculis with pressure swept Fabry-Perot interferometer for carbon dioxide
Spectral line profiles on neon and argon determined by high resolution, photoelectric recording, pressure tuned Fabry-Perot interferometer
Fabry-Perot interferometer retrodirective reflector modulator for optical communication
Widths measurements of van der Waals broadened Si I spectral lines by shock tube and scanning Fabry-Perot interferometer, using argon as perturbing gas
Interferometrically measured wavelengths tabulated for Th lines in 2747-4572 A range, using liquid nitrogen cooled hollow cathode lamp and Fabry- Perot interferometer
Fabry-Perot interferometer measurements of emission line profiles in solar corona
Internal radial velocities of diffuse emission nebulae in H II region, using photographic Fabry-Perot interferometer
Diagram extracting Lorentzian line widths from Fabry-Perot interferometer profiles
Fabry-Perot interferometer series as tunable optical narrow passband filter with high spectral and angular resolution, discussing performance in solar magnetograph
IR gas pulsed lasers continuous self mode locking, observing optical spectra with scanning Fabry-Perot interferometer
Measurement of velocity of light - use of interferometer
Magnetostrictively scanned interferometer for airborne recording of coronal temperatures during solar eclipse
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