{"title":"用于球载Pronaos亚毫米外差实验的宽带、宽温度工作范围声光光谱仪。","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":"{\"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}","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
摘要
为了实现Pronaos气球载SubMill米外差实验的科学目标,我们开发了一种宽带A.O.S.(带宽> 700 MHz),在大工作温度范围内(10到40”)具有非常好的稳定性。在与Thomson-Sin tra合作设计和制造了一种以2 GHz为中心的L - m - o - 3 (Y+123”取向)新型Bragg电池,获得了光谱仪(B*T > 1000)的最佳频率分辨率。我们描述了我们为最小化设备的尺寸、重量和功率以及提高其可靠性而实施的新解决方案。所有这些改进导致了一种非常简单和可靠的设备,既适用于空间实验,也适用于低成本的地面应用。
Wide Band, Wide Temperature Operating Range Acousto-optical Spectrometer (A.O.S) For The Balloon Borne Pronaos Submillimetre Heterodyne Experiment.
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.