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Statements

Subject Item
n2:RIV%2F67985815%3A_____%2F12%3A00388084%21RIV13-AV0-67985815
rdf:type
skos:Concept n5:Vysledek
dcterms: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 instrument reviewed 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. 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 instrument reviewed 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.
dcterms:title
The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission
skos:prefLabel
The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission The spectrometer telescope for imaging x-rays on board the Solar Orbiter mission
skos:notation
RIV/67985815:_____/12:00388084!RIV13-AV0-67985815
n5:predkladatel
n6:ico%3A67985815
n3:aktivita
n13:I
n3:aktivity
I
n3:dodaniDat
n10:2013
n3:domaciTvurceVysledku
n15:9507337 n15:9031006
n3:druhVysledku
n18:D
n3:duvernostUdaju
n9:S
n3:entitaPredkladatele
n20:predkladatel
n3:idSjednocenehoVysledku
170365
n3:idVysledku
RIV/67985815:_____/12:00388084
n3:jazykVysledku
n19:eng
n3:klicovaSlova
telescopes; imaging spectroscopy; pectrometers
n3:klicoveSlovo
n4:pectrometers n4:imaging%20spectroscopy n4:telescopes
n3:kontrolniKodProRIV
[C6BE0CF64700]
n3:mistoKonaniAkce
Amsterdam
n3:mistoVydani
Bellingham
n3:nazevZdroje
Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
n3:obor
n8:BN
n3:pocetDomacichTvurcuVysledku
2
n3:pocetTvurcuVysledku
60
n3:rokUplatneniVysledku
n10:2012
n3:tvurceVysledku
Iseli, L. Arnold, N. G. Orleanski, P. Benz, A. O. Fárník, František Klober, S. Krucker, S. Hurford, G. J. Gröbelbauer, H.-P. Kašparová, Jana Wiehl, H. J. Csillaghy, A.
n3:typAkce
n16:WRD
n3:zahajeniAkce
2012-07-01+02:00
s:numberOfPages
15
n14:hasPublisher
International Society for Optical Engineering
n7:isbn
9780819491442