G. Valsecchi, G. Bianucci, F. Marioni, D. Vernani, F. Zocchi, T. Korhonen, G. Pareschi, I. Ferreira, M. Bavdaz
{"title":"Alignment and integration of the SPO mirror modules onto the ATHENA Telescope","authors":"G. Valsecchi, G. Bianucci, F. Marioni, D. Vernani, F. Zocchi, T. Korhonen, G. Pareschi, I. Ferreira, M. Bavdaz","doi":"10.1117/12.2629304","DOIUrl":null,"url":null,"abstract":"Several hundreds of Silicon Pore Optics (SPO) mirror modules will be integrated and co-aligned onto the ATHENA (Advanced Telescope for High-ENergy Astrophysics) Mirror Assembly Module (MAM). The integration process has been developed by Media Lario and exploits a full-size optical bench to capture the focal plane image of each mirror module when illuminated by an UV plane wavefront at 218 nm. Each mirror module, handled by a manipulator, focuses the collimated beam onto a CCD camera placed at the 12 m focal position of the ATHENA telescope. The image is processed in real time to calculate the centroid position and overlap it to the centroid of the already integrated Mirror modules. Media Lario with ESA support has designed the Assembly Integration and Test (AIT) facility, able to host the complete ATHENA telescope. The AIT facility is in construction and the 2.6 m Zerodur® parabolic mirror has been accepted for coating and ready to be delivered to Calar Alto Observatory (CAHA, Sierra de Los Filabres, Spain) for the reflective coating application. The building housing the AIT facility is under construction at the Media Lario premises near Milan, Italy, and extends 6.5 m below ground and 17 m above ground. The building also is dimensioned to accommodate the vertical X-ray (Vert-X) test facility. The co-location of these two facilities is strategic for the project and will permit regular checks of the mirror module alignment while the MAM is populated. The MAM will be moved on a rail system connecting the two facilities.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"12181 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"4","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2629304","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 4
Abstract
Several hundreds of Silicon Pore Optics (SPO) mirror modules will be integrated and co-aligned onto the ATHENA (Advanced Telescope for High-ENergy Astrophysics) Mirror Assembly Module (MAM). The integration process has been developed by Media Lario and exploits a full-size optical bench to capture the focal plane image of each mirror module when illuminated by an UV plane wavefront at 218 nm. Each mirror module, handled by a manipulator, focuses the collimated beam onto a CCD camera placed at the 12 m focal position of the ATHENA telescope. The image is processed in real time to calculate the centroid position and overlap it to the centroid of the already integrated Mirror modules. Media Lario with ESA support has designed the Assembly Integration and Test (AIT) facility, able to host the complete ATHENA telescope. The AIT facility is in construction and the 2.6 m Zerodur® parabolic mirror has been accepted for coating and ready to be delivered to Calar Alto Observatory (CAHA, Sierra de Los Filabres, Spain) for the reflective coating application. The building housing the AIT facility is under construction at the Media Lario premises near Milan, Italy, and extends 6.5 m below ground and 17 m above ground. The building also is dimensioned to accommodate the vertical X-ray (Vert-X) test facility. The co-location of these two facilities is strategic for the project and will permit regular checks of the mirror module alignment while the MAM is populated. The MAM will be moved on a rail system connecting the two facilities.
数百个硅孔光学(SPO)镜面模块将被集成到雅典娜(高能天体物理先进望远镜)镜面组装模块(MAM)上。该集成工艺由Media Lario开发,利用全尺寸光学平台,在218 nm的UV平面波前照射下捕获每个镜面模块的焦平面图像。每个镜面模块由一个机械手操纵,将准直光束聚焦到放置在雅典娜望远镜12米焦距位置的CCD相机上。实时处理图像以计算质心位置,并将其与已经集成的Mirror模块的质心重叠。在欧空局的支持下,媒体拉里奥公司设计了装配集成和测试(AIT)设施,能够承载完整的雅典娜望远镜。AIT设施正在建设中,2.6米的Zerodur®抛物面镜已被接受涂层,并准备交付给Calar Alto天文台(CAHA, Sierra de Los Filabres, Spain)进行反射涂层应用。AIT设施所在的建筑位于意大利米兰附近的Media Lario场地,地下6.5米,地上17米。该建筑的尺寸也适合垂直x射线(Vert-X)测试设施。这两个设施的共存对该项目具有战略意义,并将允许在MAM填充时定期检查镜像模块对齐。MAM将通过连接两个设施的铁路系统移动。