English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/215898
logo share SHARE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL | DATACITE
Exportar a otros formatos:


Towards a European Stratospheric Balloon Observatory: The ESBO design study

AuthorsMaier, Philipp; Wolf, Jürgen; Keilig, Thomas; Krabbe, Alfred; Duffard, René D. ; Ortiz, José Luis ; Klinkner, Sabine; Lengowski, Michael; Müller, Thomas; Lockowandt, Christian; Krockstedt, Christian; Kappelmann, Norbert; Stelzer, Beate; Werner, Klaus; Geier, Stephan; Kalkuhl, Christoph; Rauch, Thomas; Schanz, Thomas; Barnstedt, Jürgen; Conti, Lauro; Hanke, Lars
Balloon telescopes
far infrared
Issue Date2018
PublisherThe International Society for Optics and Photonics
CitationProceedings of SPIE - The International Society for Optical Engineering 10700: 107004M (2018)
AbstractThis paper presents the concept of a community-accessible stratospheric balloon-based observatory that is currently under preparation by a consortium of European research institutes and industry. The planned European Stratospheric Balloon Observatory (ESBO) aims at complementing the current landscape of scientific ballooning activities by providing a service-centered infrastructure tailored towards broad astronomical use. In particular, the concept focuses on reusable platforms with exchangeable instruments and telescopes performing regular flights and an operations concept that provides researchers with options to test and operate own instruments, but later on also a proposal-based access to observations. It thereby aims at providing a complement to ground-, space-based, and airborne observatories in terms of access to wavelength regimes - particularly the ultraviolet (UV) and far infrared (FIR) regimes -, spatial resolution capability, and photometric stability. Within the currently ongoing ESBO Design Study (ESBO DS), financed within the European Union's Horizon 2020 Programme, a prototype platform carrying a 0.5-m telescope for UV and visible light observations is being built and concepts for larger following platforms, leading up to a next-generation FIR telescope are being studied. A flight of the UV/visible prototype platform is currently foreseen for 2021. We present the technical motivation, science case, instrumentation, and a two-stage image stabilization approach of the 0.5-m UV/visible platform. In addition, we briefly describe the novel mid-sized stabilized balloon gondola under design to carry telescopes in the 0.5 to 0.6 m range as well as the currently considered flight option for this platform. Secondly, we outline the scientific and technical motivation for a large balloon-based FIR telescope and the ESBO DS approach towards such an infrastructure. © 2018 SPIE.
Publisher version (URL)http://dx.doi.org/10.1117/12.2319248
Identifiersdoi: 10.1117/12.2319248
issn: 0277-786X
isbn: 978-1-5106-1954-8
Appears in Collections:(IAA) Artículos
Files in This Item:
File Description SizeFormat 
IAA_2018SPIE10700E..4MM.pdf823,13 kBAdobe PDFThumbnail
Show full item record
Review this work

WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.