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Our principal experimental research instruments are atmospheric radars, and we operate two wind-profilers, four meteor radars and jointly collaborate with Prof. J. MacDougall in sharing an MF radar. These instruments all measure atmospheric wind motions, although in different ways. The wind-profiler radars utilize radio-wave scatter from inhomogeneities in the clear air which are generated by turbulence and other small-scale phemomena, whilst the meteor radars use scatter from meteor trails at 80 to 100 km altitude. The MF radar uses inhomogeneities in electron density concentrations in the region between 60 and 100 km altitude. In all cases, we employ the Doppler shift of the back-scattered radio waves to calculate the velocities of the scattering entities and hence the velocity of the atmospheric winds at the height of scatter.
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Wayne K. Hocking, Victoria L. Pinnegar
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Jorge L. Chau, Raffaele Marino,Fabio Feraco, Juan Miguel Urco Cordero,Gerd Baumgarten,Franz-Josef Luebken,Wayne K. Hocking,Carsten Schult,Toralf Renkwitz,Ralph Latteck
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