Arrow leftBack to Explore

Instrument

CoSMIR-H
Conical Scanning Millimeter-wave Imaging Radiometer - Hyperspectral

The Conical Scanning Millimeter-wave Imaging Radiometer Hyperspectral (CoSMIR-H) is a passive airborne hyperspectral radiometer. It is a modified version of CoSMIR that replaces the 50 and 183 GHz receivers with hyperspectral receivers in 50-58 GHz and 175-191 GHz frequencies. CoSMIR-H still retains the dual-polarized channels at 89 and 165 GHz. It measures brightness temperature to retrieve vertical profiles of temperature, water vapor, and cloud properties. CoSMIR-H has a nadir footprint of 1.6 km and 1.4 km at the 50-58 GHz and 89-183 GHz frequencies, respectively, for a flight altitude of 20 km. It has an integration time of 10 ms.

NASA's DC-8 flying laboratory passes Antarctica's tallest peak, Mount Vinson, on Oct. 22, 2012, during a flight over the continent to measure changes in the massive ice sheet and sea ice. Credit: NASA/Michael Studinger (Photography courtesy NASA Images)

Instrument Details

Spectrometer/Radiometer
Earth Science > Atmosphere > Clouds > Cloud Properties
Earth Science > Atmosphere > Atmospheric Water Vapor > Water Vapor Profiles
Earth Science > Atmosphere > Atmospheric Temperature > Upper Air Temperature > Vertical Profiles
Earth Science > Spectral/engineering > Microwave > Brightness Temperature
Land Surface
10 ms, 70 ms
1.6 km x 1.6 km, 1.4 km x 1.4 km
50-58 GHz, 89 GHz, 165 GHz, 175-191 GHz
Currently unavailble
  • Rachael Kroodsma

  • Rachael Kroodsma

  • Currently unavailable

  • Currently unavailable

  • Currently unavailable