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The Spectrometer Telescope for Imaging X-rays (STIX) is one of the 10 instruments that are part of the scientific payload for the ESA Solar Orbiter mission, to be launched in 2020. The STIX instrument is an X-ray imaging spectrometer, whose purpose is to study the extremely hot solar plasma and the high-energy electrons accelerated during a solar flare. It can detect X-rays from 4 to 150 keV and exploits an indirect imaging technique based on the moiré effect, to produce images with few arcsec angular resolution in any given energy range.

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  • Espectrómetro / Telescopio para Rayos X de Imagenología (STIX) (es)
  • Spectrometer Telescope for Imaging X-rays (en)
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  • El Espectrómetro / Telescopio para Rayos X de Imagenología (STIX) es uno de los 10 instrumentos que forman parte de la carga científica de la misión de la ESA Solar Orbiter, que se lanzará en octubre de 2018. El instrumento STIX es un espectrómetro de imágenes de rayos X, cuyo propósito es estudiar el plasma solar extremadamente caliente y los electrones de alta energía acelerados durante una llamarada solar. Puede detectar rayos X de 4 a 150 keV y explora una técnica de imagen indirecta basada en el Patrón de Moiré, para producir imágenes con poca resolución angular de arco en cualquier rango de energía dado. El instrumento ha sido desarrollado por una colaboración internacional liderada por la . (es)
  • The Spectrometer Telescope for Imaging X-rays (STIX) is one of the 10 instruments that are part of the scientific payload for the ESA Solar Orbiter mission, to be launched in 2020. The STIX instrument is an X-ray imaging spectrometer, whose purpose is to study the extremely hot solar plasma and the high-energy electrons accelerated during a solar flare. It can detect X-rays from 4 to 150 keV and exploits an indirect imaging technique based on the moiré effect, to produce images with few arcsec angular resolution in any given energy range. (en)
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  • El Espectrómetro / Telescopio para Rayos X de Imagenología (STIX) es uno de los 10 instrumentos que forman parte de la carga científica de la misión de la ESA Solar Orbiter, que se lanzará en octubre de 2018. El instrumento STIX es un espectrómetro de imágenes de rayos X, cuyo propósito es estudiar el plasma solar extremadamente caliente y los electrones de alta energía acelerados durante una llamarada solar. Puede detectar rayos X de 4 a 150 keV y explora una técnica de imagen indirecta basada en el Patrón de Moiré, para producir imágenes con poca resolución angular de arco en cualquier rango de energía dado. El instrumento ha sido desarrollado por una colaboración internacional liderada por la . (es)
  • The Spectrometer Telescope for Imaging X-rays (STIX) is one of the 10 instruments that are part of the scientific payload for the ESA Solar Orbiter mission, to be launched in 2020. The STIX instrument is an X-ray imaging spectrometer, whose purpose is to study the extremely hot solar plasma and the high-energy electrons accelerated during a solar flare. It can detect X-rays from 4 to 150 keV and exploits an indirect imaging technique based on the moiré effect, to produce images with few arcsec angular resolution in any given energy range. The instrument has been developed by an international collaboration led by the . (en)
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