@prefix ns0: <http://gcmd.gsfc.nasa.gov/kms#> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

<https://gcmd.earthdata.nasa.gov/kms/concept/5207aaad-b875-40ed-b2cc-69c1b112fe37>
  ns0:resource [ ] ;
  skos:changeNote """2018-02-22 17:49:21.0 [sritz]  
update Definition (The Tropospheric Emission Spectrometer (TES) was flown on the Earth Observing System (EOS) Aura spacecraft launched in July 2004. The primary goal of the TES is the global mapping of tropospheric ozone and its photochemical precursors. The TES is a high spectral resolution infrared imaging Fourier transform spectrometer with spectral coverage from 2.3 to 16.7 micrometers with four single-line arrays optimized for different spectral regions. TES has the
capability to make both limb and down-looking observations. In the limb mode, tropospheric profiles of chemical species are made with a height resolution of 2.3 km from 0 to 30 km. In the down-looking mode, TES provides tropospheric profiles with a spatial resolution of 50 x 5 km (global) and 5 x 0.5 km (local), and a swath of 50 x 180 km (global) and 5 x 18 km (local). Both modes sensing thermal emission from the atmosphere and surface will be used to generate 3-dimensional profiles on a global scale for retrievals of O3, CO, CH4, H2O, and NOy from the surface to the lower stratosphere. See Beer, R. and
T.A.Glavich,"Remote sensing of the troposphere by infrared emission
spectroscopy", in Advanced Optical Instrumentation for Remote Sensing of Earth's Surface from Space, vol. 1129, pp 42-51,SPIE,1989.

The TES Principal Investigator is Reinhard Beer.

Additional information available at
https://tes.jpl.nasa.gov/

For more information on EOS, see:
https://eospso.gsfc.nasa.gov/eos_homepage/mission_profiles/index.php 


Group: Instrument_Details
   Entry_ID: TES
   Group: Instrument_Identification
      Instrument_Category: Earth Remote Sensing Instruments
      Instrument_Class: Passive Remote Sensing
      Instrument_Type: Spectrometers/Radiometers
      Instrument_Subtype: Spectrometers
      Short_Name: TES
      Long_Name: Tropospheric Emission Spectrometer
   End_Group
   Group: Associated_Platforms
      Short_Name: AURA
   End_Group
   Group: Spectral_Frequency_Information
      Wavelength_Keyword: Infrared > Reflected
      Spectral_Frequency_Coverage_Range: 650 to 2250 cm-1
      Spectral_Frequency_Resolution: 0.1 cm-1
   End_Group
   Online_Resource: https://tes.jpl.nasa.gov/
   Sample_Image: https://remus.jpl.nasa.gov/jpeg/tes.jpg
   Creation_Date: 2007-05-21
   Group: Instrument_Logistics
      Data_Rate: 4.5 MBPS
      Instrument_Owner: USA/NASA
   End_Group
End_Group); 
update Resource (image); 
update Resource (https://remus.jpl.nasa.gov/jpeg/tes.jpg); 
""", """2018-02-22 17:52:10.0 [sritz]  
update Definition (The Tropospheric Emission Spectrometer (TES) was flown on the Earth Observing System (EOS) Aura spacecraft launched in July 2004. The primary goal of the TES is the global mapping of tropospheric ozone and its photochemical precursors. The TES is a high spectral resolution infrared imaging Fourier transform spectrometer with spectral coverage from 2.3 to 16.7 micrometers with four single-line arrays optimized for different spectral regions. TES has the
capability to make both limb and down-looking observations. In the limb mode, tropospheric profiles of chemical species are made with a height resolution of 2.3 km from 0 to 30 km. In the down-looking mode, TES provides tropospheric profiles with a spatial resolution of 50 x 5 km (global) and 5 x 0.5 km (local), and a swath of 50 x 180 km (global) and 5 x 18 km (local). Both modes sensing thermal emission from the atmosphere and surface will be used to generate 3-dimensional profiles on a global scale for retrievals of O3, CO, CH4, H2O, and NOy from the surface to the lower stratosphere. See Beer, R. and
T.A.Glavich,"Remote sensing of the troposphere by infrared emission
spectroscopy", in Advanced Optical Instrumentation for Remote Sensing of Earth's Surface from Space, vol. 1129, pp 42-51,SPIE,1989.

The TES Principal Investigator is Reinhard Beer.

Additional information available at
https://tes.jpl.nasa.gov/

Group: Instrument_Details
   Entry_ID: TES
   Group: Instrument_Identification
      Instrument_Category: Earth Remote Sensing Instruments
      Instrument_Class: Passive Remote Sensing
      Instrument_Type: Spectrometers/Radiometers
      Instrument_Subtype: Spectrometers
      Short_Name: TES
      Long_Name: Tropospheric Emission Spectrometer
   End_Group
   Group: Associated_Platforms
      Short_Name: AURA
   End_Group
   Group: Spectral_Frequency_Information
      Wavelength_Keyword: Infrared > Reflected
      Spectral_Frequency_Coverage_Range: 650 to 2250 cm-1
      Spectral_Frequency_Resolution: 0.1 cm-1
   End_Group
   Online_Resource: https://tes.jpl.nasa.gov/
   Sample_Image: https://remus.jpl.nasa.gov/jpeg/tes.jpg
   Creation_Date: 2007-05-21
   Group: Instrument_Logistics
      Data_Rate: 4.5 MBPS
      Instrument_Owner: USA/NASA
   End_Group
End_Group); 
""" ;
  ns0:altLabel [ ] ;
  skos:definition """The Tropospheric Emission Spectrometer (TES) was flown on the Earth Observing System (EOS) Aura spacecraft launched in July 2004. The primary goal of the TES is the global mapping of tropospheric ozone and its photochemical precursors. The TES is a high spectral resolution infrared imaging Fourier transform spectrometer with spectral coverage from 2.3 to 16.7 micrometers with four single-line arrays optimized for different spectral regions. TES has the
capability to make both limb and down-looking observations. In the limb mode, tropospheric profiles of chemical species are made with a height resolution of 2.3 km from 0 to 30 km. In the down-looking mode, TES provides tropospheric profiles with a spatial resolution of 50 x 5 km (global) and 5 x 0.5 km (local), and a swath of 50 x 180 km (global) and 5 x 18 km (local). Both modes sensing thermal emission from the atmosphere and surface will be used to generate 3-dimensional profiles on a global scale for retrievals of O3, CO, CH4, H2O, and NOy from the surface to the lower stratosphere. See Beer, R. and
T.A.Glavich,"Remote sensing of the troposphere by infrared emission
spectroscopy", in Advanced Optical Instrumentation for Remote Sensing of Earth's Surface from Space, vol. 1129, pp 42-51,SPIE,1989.

The TES Principal Investigator is Reinhard Beer.

Additional information available at
https://tes.jpl.nasa.gov/

Group: Instrument_Details
   Entry_ID: TES
   Group: Instrument_Identification
      Instrument_Category: Earth Remote Sensing Instruments
      Instrument_Class: Passive Remote Sensing
      Instrument_Type: Spectrometers/Radiometers
      Instrument_Subtype: Spectrometers
      Short_Name: TES
      Long_Name: Tropospheric Emission Spectrometer
   End_Group
   Group: Associated_Platforms
      Short_Name: AURA
   End_Group
   Group: Spectral_Frequency_Information
      Wavelength_Keyword: Infrared > Reflected
      Spectral_Frequency_Coverage_Range: 650 to 2250 cm-1
      Spectral_Frequency_Resolution: 0.1 cm-1
   End_Group
   Online_Resource: https://tes.jpl.nasa.gov/
   Sample_Image: https://remus.jpl.nasa.gov/jpeg/tes.jpg
   Creation_Date: 2007-05-21
   Group: Instrument_Logistics
      Data_Rate: 4.5 MBPS
      Instrument_Owner: USA/NASA
   End_Group
End_Group"""@en ;
  skos:prefLabel "TES"@en ;
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  skos:broader <https://gcmd.earthdata.nasa.gov/kms/concept/055a79c7-61db-4250-abad-f1e09909f14c> ;
  a skos:Concept .

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  skos:prefLabel "Spectrometers"@en ;
  a skos:Concept ;
  skos:narrower <https://gcmd.earthdata.nasa.gov/kms/concept/5207aaad-b875-40ed-b2cc-69c1b112fe37> .

