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https://hdl.handle.net/2440/99159
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DC Field | Value | Language |
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dc.contributor.author | McFerran, J.J. | - |
dc.contributor.author | Dawkins, S.T. | - |
dc.contributor.author | Stanwix, P.L. | - |
dc.contributor.author | Tobar, M.E. | - |
dc.contributor.author | Luiten, A.N. | - |
dc.date.issued | 2006 | - |
dc.identifier.citation | Optics Express, 2006; 14(10):4316-4327 | - |
dc.identifier.issn | 1094-4087 | - |
dc.identifier.issn | 1094-4087 | - |
dc.identifier.uri | http://hdl.handle.net/2440/99159 | - |
dc.description.abstract | We demonstrate an optical frequency comb with fractional frequency instability of </=2x10(-14) at measurement times near 1 s, when the 10th harmonic of the comb spacing is controlled by a liquid helium cooled microwave sapphire oscillator. The frequency instability of the comb is estimated by comparing it to a cavity-stabilized optical oscillator. The less conventional approach of synthesizing low-noise optical signals from a microwave source is relevant when a laboratory has microwave sources with frequency stability superior to their optical counterparts. We describe the influence of high frequency environmental noise and how it impacts the phase-stabilized frequency comb performance at integration times less than 1 s. | - |
dc.description.statementofresponsibility | J. J. McFerran, S. T. Dawkins, P. L. Stanwix, M. E. Tobar and A. N. Luiten | - |
dc.language.iso | en | - |
dc.publisher | Optical Society of America | - |
dc.rights | © 2006 Optical Society of America | - |
dc.source.uri | http://dx.doi.org/10.1364/oe.14.004316 | - |
dc.title | Optical frequency synthesis from a cryogenic microwave sapphire oscillator | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1364/OE.14.004316 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Luiten, A.N. [0000-0001-5284-7244] | - |
Appears in Collections: | Aurora harvest 7 IPAS publications |
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