Feedback Stabilized Fabry-Perot Interferometer
- 1 January 1973
- journal article
- Published by Optica Publishing Group in Applied Optics
- Vol. 12 (1) , 126-130
- https://doi.org/10.1364/ao.12.000126
Abstract
A method of stabilizing a Fabry-Perot interferometer with respect to a reference wavelength, while simultaneously stabilizing the parallelism of the flats, is described. The method consists of creating correcting signals proportional to the displacement of the fringe maxima of three auxiliary spectral sources with respect to a fixed reference point and feeding these signals back to the interferometer piezoelectric drive so that the correcting signals become time invariant, and the interferometer is stabilized. The stability of the finished instrument with respect to the reference wavelength and parallelism is near λ/1000, at 546 nm, for a 6-h period; however, the actual parallelism of the etalon is limited by the surface defects of the flats. The method, as described, allows simultaneous stabilization and data taking, since the instrument is continuously updating itself.Keywords
This publication has 41 references indexed in Scilit:
- Interferometric measurements of the 6300 A Doppler temperature during a magnetic stormJournal of Geophysical Research, 1969
- Twilight and nightglow spectral line shapes of oxygen λ6300 and λ5577 radiationPlanetary and Space Science, 1968
- Description d’un spectromètre de haute résolution Fabry-PérotApplied Optics, 1968
- Automatic Control of the Spacing of Fabry–Perot InterferometersApplied Optics, 1966
- Stable, Easily Fabricated, Tunable, Passive Optical CavityReview of Scientific Instruments, 1966
- Interferometry and Laser Control with Solid Fabry–Perot EtalonsApplied Optics, 1966
- Observations of the 6300 Å OI nightglow emissionJournal of Atmospheric and Terrestrial Physics, 1966
- Nightglow 5577 Å [OI] line kinetic temperaturesPlanetary and Space Science, 1965
- Doppler Widths of the Atomic Oxygen Lines in the Airglow.The Astrophysical Journal, 1960
- The temperature in the atmospheric region emitting the nightglow OI 5577 line and in regions above faint auroral arcsJournal of Atmospheric and Terrestrial Physics, 1959