|Instrument: HIRS/3 : High Resolution Infrared Radiation Sounder/3|
Earth Remote Sensing Instruments
Instrument Class: Passive Remote Sensing
Instrument Type: Profilers/Sounders
Wavelength Keyword: Near Infrared
Number Channels: 19
Spectral/Frequency Coverage/Range: 6.5 to 15 micrometers & 3.7 to 4.6 micrometers
Wavelength Keyword: Visible
Number Channels: 1
Spectral/Frequency Coverage/Range: 0.69 micrometers
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The High Resolution Infrared Radiation Sounder (HIRS/3) is a discrete stepping, line-scan instrument designed to measure scene radiance in 20 spectral bands to permit the calculation of the vertical temperature profile from Earth's surface to about 40 km.
Multispectral data from one visible channel (0.69 micrometers), seven shortwave channels (3.7 to 4.6 micrometers) and twelve longwave channels (6.5 to 15 micrometers) are obtained from a single telescope and a rotating filter wheel containing twenty individual filters. An elliptical scan mirror provides cross-track scanning of 56 increments of 1.8 degrees. The mirror steps rapidly (<35 msec), then holds at each position while the 20 filter segments are sampled. This action takes place each 100 msec. The instantaneous FOV for each channel is approximately 1.4 degrees in the visible and shortwave IR and 1.3 degrees in the longwave IR band which, from an altitude of 833 kilometers, encompasses an area of 20.3 kilometers and 18.9 kilometers in diameter, respectively, at nadir on the Earth.
Three detectors are used to sense the radiation. A silicon photodiode at the instrument temperature (nominally 15 degrees C) detects the visible energy. An Indium Antimonide detector and a Mercury Cadmium Telluride detector (mounted on a passive radiator and operating at 100K) sense the shortwave and longwave IR energy. The shortwave and visible optical paths have a common field stop, while the longwave path has an identical but separate field stop. Registration of the fields of view in all channels is largely determined by these stops with secondary effects from detector position.
IR Calibration of the HIRS/3 is provided by programmed views of two radiometric targets: a warm target mounted to the instrument base and a view of space. Data from these views provides sensitivity calibrations for each channel every 40 lines (256 seconds), if commanded. Internally generated electronic signals provide calibration and stability monitoring of the amplifier and readout electronics.
Data from the instrument is multiplexed into a single data stream controlled by the TIP system of the spacecraft. Information from the radiometric channels and voltage telemetry are converted to 13-bit binary data. Radiometric information is processed to produce the maximum dynamic range such that instrument and digitizing noises are a small portion of the signal output. Each channel is characterized by a noise equivalent radiance (NE?N) and a set of calibration data that may be used to derive atmospheric temperatures and probable errors.
The HIRS/3 instrument is a single package mounted on the Instrument Mounting Platform (IMP) of the NOAA KLM spacecraft.
Information obtained from http://www2.ncdc.noaa.gov/docs/klm/html/c3/sec32-1.htm
Instrument Owner: NOAA/NASA