Grazing-incidence imaging spectrograph for solar observations in the extreme-ultraviolet domain (Contributo in atti di convegno)

Type
Label
  • Grazing-incidence imaging spectrograph for solar observations in the extreme-ultraviolet domain (Contributo in atti di convegno) (literal)
Anno
  • 2012-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1117/12.924810 (literal)
Alternative label
  • Frassetto, Fabio; Coraggia, Stefano; Miotti, Paolo; Poletto, Luca (2012)
    Grazing-incidence imaging spectrograph for solar observations in the extreme-ultraviolet domain
    in SPIE Astronomical Telescopes + Instrumentation, Amsterdam (Netherlands), 1 luglio 2012
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Frassetto, Fabio; Coraggia, Stefano; Miotti, Paolo; Poletto, Luca (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#titoloVolume
  • Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 8443 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#volumeInCollana
  • 8443 (literal)
Rivista
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#pagineTotali
  • 10 (literal)
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • Natl Council Res Italy (literal)
Titolo
  • Grazing-incidence imaging spectrograph for solar observations in the extreme-ultraviolet domain (literal)
Abstract
  • The design of an imaging spectrograph operating at grazing incidence and stigmatic in a large field-of-view is presented. (literal)
  • It is realized coupling a double telescope and a spectrometer. The instrument may be used for XUV space observations of extended sources, and is particularized to the Sun observation from the Earth. The performances of a laboratory prototype are presented. This instrument covers the 4-20 nm (310-62 eV) spectral region, with a spectral resolution of 0.1% at 10 nm and a spatial resolution of 3.5 arcsec over a field-of-view of 0.5 deg, within a total envelope of 1.2 m. The design and the characterization of the instrument in the whole spectral region of operation are presented. (literal)
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