1 September 1996 Ramsey resonance characteristics of the optically pumped Cesium beam frequency standard at kriss
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Proceedings Volume 2778, 17th Congress of the International Commission for Optics: Optics for Science and New Technology; 277857 (1996) https://doi.org/10.1117/12.2299070
Event: 17th Congress of the International Commission for Optics: Optics for Science and New Technology, 1996, Taejon, Korea, Republic of
Abstract
We investigated Ramsey resonance characteristics of the optically pumped cesium beam frequency standard constructed at KRISS. The linewidth of the Ramsey signal from a 38-cm long microwave cavity was about 260 Hz. The linewidth and peak-to-valley values of the Ramsey signal versus the microwave power were observed and compared with theoretical results obtained by taking into account the 1/v-weighted Maxwell velocity distribution in the cesium atomic beam. Both results coincided quite well, but the asymmetry in the Ramsey signal occurred, the causes of which were discussed.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ho Seong Lee, "Ramsey resonance characteristics of the optically pumped Cesium beam frequency standard at kriss", Proc. SPIE 2778, 17th Congress of the International Commission for Optics: Optics for Science and New Technology, 277857 (1 September 1996); doi: 10.1117/12.2299070; https://doi.org/10.1117/12.2299070
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