@prefix skos: . @prefix ns0: . skos:changeNote """2020-03-16 18:49:36.0 [sritz] update Definition ([For archive only. The Earth-Observing One (EO-1) satellite was decommissioned March 2017.] The Hyperion instrument provides a new class of Earth observation data for improved Earth surface characterization. The Hyperion provides a science grade instrument with quality calibration based on heritage from the LEWIS Hyperspectral Imaging Instrument (HSI). The Hyperion capabilities provide resolution of surface properties into hundreds of spectral bands versus the ten multispectral bands flown on traditional Landsat imaging missions. Through these large number of spectral bands, complex land eco-systems shall be imaged and accurately classified. The Hyperion provides a high resolution hyperspectral imager capable of resolving 220 spectral bands (from 0.4 to 2.5 µm) with a 30 meter spatial resolution. The instrument images a 7.5 km by 100 km land area per image and provides detailed spectral mapping across all 220 channels with high radiometric accuracy. The major components of the instrument include the following: 1. System fore-optics design based on the KOMPSAT EOC mission. The telescope provides for two separate grating image spectrometers to improve signal-to-noise ratio (SNR). 2. A focal plane array which provides separate short wave infrared (SWIR) and visible/near infrared (VNIR) detectors based on spare hardware from the LEWIS HSI program. 3. A cryocooler identical to that fabricated for the LEWIS HSI mission for cooling of the SWIR focal plane. [Summary provided by NASA] Group: Instrument_Details Entry_ID: HYPERION Group: Instrument_Identification Instrument_Category: Earth Remote Sensing Instruments Instrument_Class: Passive Remote Sensing Instrument_Type: Spectrometers/Radiometers Instrument_Subtype: Hyperspectral Spectrometers/Radiometers Short_Name: HYPERION Long_Name: HYPERSPECTRAL IMAGER End_Group Group: Associated_Platforms Short_Name: EO-1 End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Visible Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Near Infrared Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Infrared > Reflected Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Online_Resource: https://www.usgs.gov/centers/eros/science/usgs-eros-archive-earth-observing-one-eo-1-hyperion?qt-science_center_objects=0#qt-science_center_objects Creation_Date: 2007-07-06 Group: Instrument_Logistics Instrument_Owner: USA/NASA End_Group End_Group); update Definition (https://www.usgs.gov/centers/eros/science/usgs-eros-archive-earth-observing-one-eo-1-hyperion?qt-science_center_objects=0#qt-science_center_objects); delete Resource (null); """ ; ns0:altLabel [ ] ; skos:definition """[For archive only. The Earth-Observing One (EO-1) satellite was decommissioned March 2017.] The Hyperion instrument provides a new class of Earth observation data for improved Earth surface characterization. The Hyperion provides a science grade instrument with quality calibration based on heritage from the LEWIS Hyperspectral Imaging Instrument (HSI). The Hyperion capabilities provide resolution of surface properties into hundreds of spectral bands versus the ten multispectral bands flown on traditional Landsat imaging missions. Through these large number of spectral bands, complex land eco-systems shall be imaged and accurately classified. The Hyperion provides a high resolution hyperspectral imager capable of resolving 220 spectral bands (from 0.4 to 2.5 µm) with a 30 meter spatial resolution. The instrument images a 7.5 km by 100 km land area per image and provides detailed spectral mapping across all 220 channels with high radiometric accuracy. The major components of the instrument include the following: 1. System fore-optics design based on the KOMPSAT EOC mission. The telescope provides for two separate grating image spectrometers to improve signal-to-noise ratio (SNR). 2. A focal plane array which provides separate short wave infrared (SWIR) and visible/near infrared (VNIR) detectors based on spare hardware from the LEWIS HSI program. 3. A cryocooler identical to that fabricated for the LEWIS HSI mission for cooling of the SWIR focal plane. [Summary provided by NASA] Group: Instrument_Details Entry_ID: HYPERION Group: Instrument_Identification Instrument_Category: Earth Remote Sensing Instruments Instrument_Class: Passive Remote Sensing Instrument_Type: Spectrometers/Radiometers Instrument_Subtype: Hyperspectral Spectrometers/Radiometers Short_Name: HYPERION Long_Name: HYPERSPECTRAL IMAGER End_Group Group: Associated_Platforms Short_Name: EO-1 End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Visible Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Near Infrared Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Group: Spectral_Frequency_Information Wavelength_Keyword: Infrared > Reflected Spectral_Frequency_Coverage_Range: 0.4 μm - 2.5 μm End_Group Online_Resource: https://www.usgs.gov/centers/eros/science/usgs-eros-archive-earth-observing-one-eo-1-hyperion?qt-science_center_objects=0#qt-science_center_objects Creation_Date: 2007-07-06 Group: Instrument_Logistics Instrument_Owner: USA/NASA End_Group End_Group"""@en ; skos:prefLabel "HYPERION"@en ; skos:inScheme ; skos:broader ; a skos:Concept . skos:prefLabel "Hyperspectral Spectrometers/Radiometers"@en ; a skos:Concept ; skos:narrower .