The Conical Scanning Millimeter-wave Imaging Radiometer (CoSMIR) is an airborne imaging radiometer that was developed to validate the Special Sensor Microwave Imager/Sounder (SSMIS) instrument. CoSMIR operates across 9 spectral channels in the 50-183 GHz range to measure microwave brightness temperature. CoSMIR has a surface footprint resolution of 1.4 km x 1.4 km at an altitude of 20 km at nadir. It can perform both conical and cross-tracking scanning.


Instrument Details
- Spectrometer/Radiometer
- Earth Science > Spectral/engineering > Microwave > Brightness TemperatureEarth Science > Spectral/engineering > Microwave > Microwave Radiance
- Land Surface
- 2-3 s
- 1.4 km x 1.4 km
- 50-183 GHz
- https://doi.org/10.1109/IGARSS.2001.976672
Rachael Kroodsma
Rachael Kroodsma
Currently unavailable
NASA's Defense Meteorological Satellite Program (DMSP)
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