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spase://NASA/NumericalData/Hinode/XRT/Level0/FITS
Description
Hinode XRT Level0 FITS data are uncalibrated observational data acquired by the X-Ray Telescope (XRT) onboard the Hinode spacecraft. The Level0 FITS files contain telemetry-derived CCD images of the solar corona obtained through X-ray analysis filters and visible-light optics, together with instrument configuration parameters and observational metadata. Each file typically corresponds to a single exposure.
XRT is a grazing-incidence soft X-ray telescope designed to observe high-temperature coronal plasma with high spatial and temporal resolution. The instrument includes Wolter-I type X-ray optics, focal-plane filter wheels, a shutter mechanism, visible-light optics, and a 2048 × 2048 CCD detector.
The Level0 FITS data preserve the original observation content before calibration and scientific processing. These files provide the basis for higher-level calibrated products and support studies of active regions, flares, coronal heating, plasma dynamics, and eruptive phenomena such as coronal mass ejections. The XRT instrument was developed through a Japan–US collaboration involving the Harvard-Smithsonian Center for Astrophysics, NASA Marshall Space Flight Center, JAXA, and NAOJ.
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Add 'Z' to RevisionEvent:ReleaseDate(s), PublicationDate. ZCB
Description
Hinode XRT Level0 FITS data are uncalibrated observational data acquired by the X-Ray Telescope (XRT) onboard the Hinode spacecraft. The Level0 FITS files contain telemetry-derived CCD images of the solar corona obtained through X-ray analysis filters and visible-light optics, together with instrument configuration parameters and observational metadata. Each file typically corresponds to a single exposure.
XRT is a grazing-incidence soft X-ray telescope designed to observe high-temperature coronal plasma with high spatial and temporal resolution. The instrument includes Wolter-I type X-ray optics, focal-plane filter wheels, a shutter mechanism, visible-light optics, and a 2048 × 2048 CCD detector.
The Level0 FITS data preserve the original observation content before calibration and scientific processing. These files provide the basis for higher-level calibrated products and support studies of active regions, flares, coronal heating, plasma dynamics, and eruptive phenomena such as coronal mass ejections. The XRT instrument was developed through a Japan–US collaboration involving the Harvard-Smithsonian Center for Astrophysics, NASA Marshall Space Flight Center, JAXA, and NAOJ.
PublicationInfo
Authors
The Hinode XRT Consortium: Harvard-Smithsonian Center for Astrophysics (USA); Japan Aerospace Exploration Agency (Japan); National Astronomical Observatory of Japan (Japan); NASA Marshall Space Flight Center (USA); NASA Goddard Space Flight Center (USA)