{"title":"Wide Band, Wide Temperature Operating Range Acousto-optical Spectrometer (A.O.S) For The Balloon Borne Pronaos Submillimetre Heterodyne Experiment.","authors":"C. Rosolen, D. Michet, C. Gac, A. Lecacheux","doi":"10.1109/SBMO.1993.589551","DOIUrl":null,"url":null,"abstract":"In order to fulfill the scientific objectives of the Pronaos balloon borne SubMill imetre heterodyne experiment, we developed a wide band A.O.S. (bandwidth > 700 MHz) having very good stability over a large operating temperature range (loo to 40\"). The optimization of the frequency resolution of the spectrometer (B*T > 1000) was obtained in designing and building, in collaboration with Thomson-Sin tra, a new kind of Bragg cell in L i m o 3 (Y+123\" orientation) centered at 2 GHz. We described the new solutions that we have implemented for minimizing the size, weight and power of the device and for improving its reliability. All these improvements lead to a very simple and reliable device as well adapted for space experiments as for low cost, ground based applications.","PeriodicalId":219944,"journal":{"name":"SBMO International Microwave Conference/Brazil,","volume":"487 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1993-08-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"SBMO International Microwave Conference/Brazil,","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/SBMO.1993.589551","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
In order to fulfill the scientific objectives of the Pronaos balloon borne SubMill imetre heterodyne experiment, we developed a wide band A.O.S. (bandwidth > 700 MHz) having very good stability over a large operating temperature range (loo to 40"). The optimization of the frequency resolution of the spectrometer (B*T > 1000) was obtained in designing and building, in collaboration with Thomson-Sin tra, a new kind of Bragg cell in L i m o 3 (Y+123" orientation) centered at 2 GHz. We described the new solutions that we have implemented for minimizing the size, weight and power of the device and for improving its reliability. All these improvements lead to a very simple and reliable device as well adapted for space experiments as for low cost, ground based applications.