Frequency selection of the radiation of a fiber laser with a reflection interferometer |
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| Authors: | V S Terent’ev V A Simonov |
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| Affiliation: | (1) SRON Netherlands Institute for Space Research, Landleven 12, 9747 AD Groningen, The Netherlands;(2) Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands;(3) Institute for Astronomy, University of Edinburgh, Edinburgh, EH9 3HJ, UK;(4) UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK |
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| Abstract: | This paper considers the results of using a two-mirror multiple-beam reflection interferometer (RI) which has a response function
in reflection similar to the response function of a Fabry-Perot interferometer in transmission. The two-mirror cavity of the
RI included two flat mirrors, one of which was highly reflective, and the other had an asymmetric coefficient of reflection
from different sides. The light reflected from the RI was brought to an optical fiber through a collimator lens. The optical
fiber, collimator, and RI constituted an integrated fiber RI, which was first used for continuous tuning of the wavelength
of an erbium ring fiber laser with a continuous generation in the spectral range 1520–1566 nm. |
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