D. S. Acton, P. Stomski, P. Wizinowich, J. Maute, T. Gregory, M. Ealey, T. Price
{"title":"Keck Adaptive Optics: Test of a Deformable Mirror in a Freezing Environment","authors":"D. S. Acton, P. Stomski, P. Wizinowich, J. Maute, T. Gregory, M. Ealey, T. Price","doi":"10.1364/adop.1996.afa.2","DOIUrl":null,"url":null,"abstract":"The W. M. Keck Observatory and Lawrence Livermore National Labs are currently developing an adaptive optics system for use on Keck II--a 10.8-meter segmented telescope. This AO system will make use of a 349-actuator deformable mirror (DM). The Keck II telescope sits atop Hawaii’s Mauna Kea, where the ambient nighttime temperature varies between -5 and 5 degrees C. In order to reduce dome seeing, and to minimize the thermal emissivity, the AO system (and hence the DM) will be cooled to the ambient temperature of the outside air. Therefore, we are motivated to use actuators in the DM that are optimized for operation at 0 degrees C.","PeriodicalId":256393,"journal":{"name":"Adaptive Optics","volume":"62 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Adaptive Optics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1364/adop.1996.afa.2","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
The W. M. Keck Observatory and Lawrence Livermore National Labs are currently developing an adaptive optics system for use on Keck II--a 10.8-meter segmented telescope. This AO system will make use of a 349-actuator deformable mirror (DM). The Keck II telescope sits atop Hawaii’s Mauna Kea, where the ambient nighttime temperature varies between -5 and 5 degrees C. In order to reduce dome seeing, and to minimize the thermal emissivity, the AO system (and hence the DM) will be cooled to the ambient temperature of the outside air. Therefore, we are motivated to use actuators in the DM that are optimized for operation at 0 degrees C.
W. M.凯克天文台和劳伦斯利弗莫尔国家实验室目前正在开发一种用于凯克二号的自适应光学系统——一个10.8米的分段望远镜。该AO系统将使用349致动器变形镜(DM)。凯克II号望远镜位于夏威夷的莫纳克亚山上,那里的夜间环境温度在-5到5摄氏度之间变化。为了减少圆顶的可见度,并最大限度地减少热辐射率,AO系统(因此DM)将被冷却到外部空气的环境温度。因此,我们有动力在DM中使用针对0℃操作进行优化的执行器。