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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.
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); https://doi.org/10.1117/12.2299070
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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); https://doi.org/10.1117/12.2299070