Special Sensor Microwave/Imager

The Special Sensor Microwave/Imager (SSM/I) is a seven-channel, four-frequency, linearly polarized passive microwave radiometric system. The instrument measures surface/atmospheric microwave brightness temperatures (TBs) at 19.35, 22.235, 37.0 and 85.5 GHz. The four frequencies are sampled in both horizontal and vertical polarizations, except the 22 GHz which is sampled in the vertical only.

The SSM/I has been a very successful instrument, superseding the across-track and Dicke radiometer designs of previous systems. Its combination of constant-angle rotary-scanning and total power radiometer design has become standard for passive microwave imagers, e.g. TRMM Microwave Imager, AMSR.

Its predecessor, the Scanning Multichannel Microwave Radiometer (SMMR), provides similar information.

Additional recommended knowledge

Guide to balance cleaning: 8 simple steps

How to ensure accurate weighing results every day?

Don't let static charges disrupt your weighing accuracy

Products

With the predecessor SMMR, SSM/I products are available from late 1978 to present.

Information within the SSM/I TBs measurements allow the retrieval of four important geophysical parameters over the ocean: near-surface wind speed (note scalar not vector), total columnar water vapor, total columnar cloud liquid water and precipitation. However, accurate and quantitative measurement of these parameters from the SSM/I TBs is a non-trivial task. Variations within the meteorological parameters significantly modify the TBs. As well as open ocean retrievals, it is also possible to retrieve quantitatively reliable information on sea ice [1], land snow cover and over-land precipitation.

Instrument characteristics

The instrument is flown onboard the United States Air Force Defense Meteorological Satellite Program (DMSP) Block 5D-2 spacecraft. These are in circular or near-circular Sun-synchronous and near-polar orbits at altitudes of 833 km with inclinations of 98.8° and orbital periods of 102.0 minutes, each making 14.1 full orbits per day. The scan direction is from the left to the right with the active scene measurements lying ±51.2 degrees about when looking in the forward (F10-F15) or aft (F8) direction of the spacecraft. This results in a nominal swath width of 1394 km allowing frequent ground coverage, especially in the polar regions. All parts of the globe at latitudes higher than 58° are covered at least twice daily except for small unmeasured circular sectors of 2.4° about the poles. Extreme polar regions (> 72° N or S) receive coverage from two or more overpasses from both the ascending and descending orbits each day.

The spin rate of the SSM/I provides a period of 1.9 sec during which the DMSP spacecraft sub-satellite point travels 12.5 km. Each scan 128 discrete, uniformly spaced radiometric samples are taken at the two 85 GHz channels and, on alternate scans, 64 discrete samples are taken at the remaining 5 lower frequency channels. The resolution is determined by the Nyquist limit and the Earth surface's contribution of 3dB bandwidth of the signal at a given frequency (see Table). The radiometer direction intersects the Earth’s surface at a nominal incidence angle of 53.1 degrees, as measured from the local Earth normal.

Table 1 Radiometric characteristics of the SSM/I (Hollinger 1989).

Instrument history

The SMMR was flown on Seasat and NASA Nimbus 7 in 1978. The latter operated until 1985.

The SSM/I has been operating almost continuously on Block 5D-2 flights F8-F15 (not F9) since June 1987. Concerns about the radiometer's performance over the full range of space environmental conditions led to the F8 instrument being switched off in early December 1987 to avoid overheating. The 85 GHz vertical polarization channel failed to switch on in January 1988. Analysis showed inadequate thermal shielding of the sensor's radiometers due to excessive heating at perihelion. The 85 GHz horizontal polarization subsequently had a large increase in radiometric errors and was switched off in summer 1988.

The launch of the next SSM/I, on board the F10 satellite, took place on 1 December 1990, but was not fully successful. The explosion of the booster rocket left the F10 in an elliptical orbit. The incidence angle of the F10 SSM/I boresight would vary in relation to the Earth throughout each orbit and this also altered the surface area of the Earth viewed by the radiometer. The deviations in the incidence angle of up to 1.4° were quite large and would alter the responses of several geophysical algorithms if not taken into consideration. Further, related changes in the swath width from a minimum of 1226 km at perigee to 1427 km at apogee altered the amounts of radiation viewed by the F10 SSM/I radiometers. The non-circular orbit also caused slight precession of the equatorial crossing time of the F10 by 50 seconds per week.

The F12 imager had a delayed launch date (the spacecraft was out of the DMSP build sequence) due to a faulty SSM/I. The extra time and costs taken to rectify the problem did not, however, help. The SSM/I failed to ‘spin-up’ after launch, and consequently data were not available from this instrument. The SSM/Is on F11, F13, F14 and F15 have all produced excellent data.

Before the F8 was decommissioned, it aided investigations into measuring passive microwaves at higher Earth incidence angles (i.e. > 51 degrees). An increase in angle would allow a greater swath width to be utilised, giving a greater amount of coverage at the Earth's surface. The F8 Tilt Experiment (see links) was carried out between 25th June and 13th July 1993.

Table 2 SSM/I Satellites characteristics (source: DSMP website & www.ssmi.com).

F17 and F19 will follow at 3 year intervals, or as needed.

References

Hollinger, J.P. 1989: DMSP Special Sensor Microwave/Imager Calibration/Validation. Final Report, Vol. I., Space Sensing Branch, Naval Research Laboratory, Washington D.C.