M. Pelizzo, M. Padovani, A. Corso, G. Santi, M. Uslenghi, D. Faccini, M. Fiorini, S. Incorvaia, G. Toso, E. Fabbrica, M. Carminati, C. Fiorini, G. Favaro, M. Bazzan, G. Maggioni, G. Naletto, V. Andretta, A. Milillo
{"title":"Spectroscopic observation of planetary and Moon exospheres in the ultraviolet","authors":"M. Pelizzo, M. Padovani, A. Corso, G. Santi, M. Uslenghi, D. Faccini, M. Fiorini, S. Incorvaia, G. Toso, E. Fabbrica, M. Carminati, C. Fiorini, G. Favaro, M. Bazzan, G. Maggioni, G. Naletto, V. Andretta, A. Milillo","doi":"10.1117/12.2633821","DOIUrl":null,"url":null,"abstract":"The planetary extreme ultraviolet spectrometer (PLUS) is a project funded by the Italian Space Agency focused on the development of an extreme (EUV) and far-ultraviolet (FUV) high-performance spectrograph, which adopts a dual channel optical scheme. Thanks to an optimized layout based on the use of variable line space (VLS) gratings in an off-Rowland configuration, high spectral and spatial resolution are achieved. The efficiency improvement is obtained by the optimization of the coatings on the optical components. Improved detection limit, shorter observations integration time and unprecedented performance in terms of dynamic range will be achieved by the use of high resolution/dynamic range solar blind photon counting detectors. The photon counting detectors will be based on a micro-channel plate (MCP) coupled with an application specific integrated circuit (ASIC) read out system.","PeriodicalId":137463,"journal":{"name":"Astronomical Telescopes + Instrumentation","volume":"70 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2022-08-31","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomical Telescopes + Instrumentation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2633821","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
The planetary extreme ultraviolet spectrometer (PLUS) is a project funded by the Italian Space Agency focused on the development of an extreme (EUV) and far-ultraviolet (FUV) high-performance spectrograph, which adopts a dual channel optical scheme. Thanks to an optimized layout based on the use of variable line space (VLS) gratings in an off-Rowland configuration, high spectral and spatial resolution are achieved. The efficiency improvement is obtained by the optimization of the coatings on the optical components. Improved detection limit, shorter observations integration time and unprecedented performance in terms of dynamic range will be achieved by the use of high resolution/dynamic range solar blind photon counting detectors. The photon counting detectors will be based on a micro-channel plate (MCP) coupled with an application specific integrated circuit (ASIC) read out system.