Abstract
At an IUGG-IUTAM Symposium in 1966 at Kyoto, Japan, a brief paper by me made some general comments on our inadequate understanding and knowledge of the planetary boundary layer over the oceans.* The possibility that earth orbiting spacecraft could measure waves over the ocean and provide data from which very high quality synoptic surface weather maps and wind fields could be determined was described.
In 1978, an experimental spacecraft at an altitude of 800 km in a 108° retrograde orbit with a period of 100 minutes will test these concepts and provide global coverage of the vector wind field over the oceans, of water vapor and rainfall, and of wave conditions. Partial coverage of sea ice conditions in the arctic and antarctic will also be obtained. Three different kinds of radar, a passive microwave system at five frequencies, with two polarizations for each frequency, and a visible band and infrared band imaging system make up the remote sensors on this spacecraft.
Two of the radars, the altimeter and the scatterometer, were tested on SKYLAB, and an altimeter is currently on GEOS-3. Extensive tests of the scatterometer and the third radar (a synthetic aperture imaging radar) have been made from aircraft.
The present status of our research on the scatterometer is that the speed and direction of winds from about 4 M/S to 24 M/S (and probably even higher) can be determined and that above about 7 M/S the speed can be found to about ±0.5 M/S and the direction to about ±15°. Several hundred thousand vector winds will be determined each day.
SEASAT-A, and the spacecraft that will follow it, will initiate a new era in improved meteorological forecasts because of the improved initial value specification of the planetary boundary layer over the ocean. Fluxes of momentum, heat and H2O across the air-sea interface can be determined without gaps due to missing ship reports to great accuracy by means of the bulk aerodynamic equations and other methods. The winds over the ocean will be known more accurately than ever before. Also information on radiation fluxes is potentially available.
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Pierson, W.J. (1978). The Potential Impact of Seasat-A on the Study of the Planetary Boundary Layer Over the Ocean. In: Favre, A., Hasselmann, K. (eds) Turbulent Fluxes Through the Sea Surface, Wave Dynamics, and Prediction. Springer, Boston, MA. https://doi.org/10.1007/978-1-4612-9806-9_34
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