The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00388084" target="_blank" >RIV/67985815:_____/12:00388084 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission
Original language description
The Spectrometer Telescope for Imaging X-rays (STIX) is one of 10 instruments on board Solar Orbiter, a confirmed Mclass mission of the European Space Agency (ESA) within the Cosmic Vision program scheduled to be launched in 2017. STIX applies a Fourier-imaging technique using a set of tungsten grids (at pitches from 0.038 to 1 mm) in front of 32 pixelized CdTe detectors to provide imaging spectroscopy of solar thermal and non-thermal hard X-ray emissions from 4 to 150 keV. The status of the instrumentreviewed in this paper is based on the design that passed the Preliminary Design Review (PDR) in early 2012. Particular emphasis is given to the first light of the detector system called Caliste-SO.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
ISBN
9780819491442
ISSN
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e-ISSN
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Number of pages
15
Pages from-to
"84433L"-"1-84433L-15"
Publisher name
International Society for Optical Engineering
Place of publication
Bellingham
Event location
Amsterdam
Event date
Jul 1, 2012
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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