{"title":"DECIGO和DPF光源的研究进展","authors":"M. Musha, K. Nakagawa, K. Ueda","doi":"10.1109/ICSOS.2011.5783700","DOIUrl":null,"url":null,"abstract":"We have developed the light source for the space gravitational wave detector, DECIGO, and its pathfinder, DPF. The frequency stability of the 1 Hz/Hz1/2 at Fourier frequency around 1Hz, and output power of 10W are required as the light source for DECIGO. We will report the breadboard model of the frequency-stabilized Yb:YAG laser for DPF whose frequency is stabilized in reference to the saturated absorption of iodine molecules around 515nm, and the fiberMOPA system for DECIGO.","PeriodicalId":107082,"journal":{"name":"2011 International Conference on Space Optical Systems and Applications (ICSOS)","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2011-05-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Developments of the light source for DECIGO and DPF\",\"authors\":\"M. Musha, K. Nakagawa, K. Ueda\",\"doi\":\"10.1109/ICSOS.2011.5783700\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We have developed the light source for the space gravitational wave detector, DECIGO, and its pathfinder, DPF. The frequency stability of the 1 Hz/Hz1/2 at Fourier frequency around 1Hz, and output power of 10W are required as the light source for DECIGO. We will report the breadboard model of the frequency-stabilized Yb:YAG laser for DPF whose frequency is stabilized in reference to the saturated absorption of iodine molecules around 515nm, and the fiberMOPA system for DECIGO.\",\"PeriodicalId\":107082,\"journal\":{\"name\":\"2011 International Conference on Space Optical Systems and Applications (ICSOS)\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2011-05-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2011 International Conference on Space Optical Systems and Applications (ICSOS)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/ICSOS.2011.5783700\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2011 International Conference on Space Optical Systems and Applications (ICSOS)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/ICSOS.2011.5783700","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Developments of the light source for DECIGO and DPF
We have developed the light source for the space gravitational wave detector, DECIGO, and its pathfinder, DPF. The frequency stability of the 1 Hz/Hz1/2 at Fourier frequency around 1Hz, and output power of 10W are required as the light source for DECIGO. We will report the breadboard model of the frequency-stabilized Yb:YAG laser for DPF whose frequency is stabilized in reference to the saturated absorption of iodine molecules around 515nm, and the fiberMOPA system for DECIGO.
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