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Titlebook: Dynamical and Chemical Coupling Between the Neutral and Ionized Atmosphere; Proceedings of the N B. Grandal,J. A. Holtet Conference proceed

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Kobaltrates of dissipation in the altitude region 81 to 97 km. Chemical releases (Blamont and de Jager 1961; Zimmerman and Champion 1963; Justus 1969; Zimmerman and Trowbridge 1973) allowed us to determine turbulent diffusion rates and turbulent dissipation by both diffusion growth rates and turbulent spectra observed in the tracer chemicals.
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Urann (1977). At relativistic energies (≳ 500 kev) the precipitating electrons deposit their energy near the base of the mesosphere; and the concomitant Bremsstrahlung X-rays provide additional energy deposition deep into the stratosphere.
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Morphology of Upper Atmosphere Temperatureshanges on longer time scales such as the quasibiennial oscillation and interannual variability, and on smaller scales such as planetary waves (both forced and free), gravity waves and tides. Until recently the only way of studying the variation of temperature of the upper stratosphere and mesosphere
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Stratospheric and Mesospheric Turbulenceaircraft have partially investigated the lower stratosphere to 20 km (Kellogg 1956; Gifford 1957; Zimmerman 1965; Lilly et al, 1975; Zimmerman and Loving 1975). Radio meteor (Roper and Elford 1963; Roper 1966; Zimmerman 1973, 1974) have been utilized to determine some bulk turbulent viscosities and
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