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- W2093337701 abstract "In this paper the propagation and dissipation characteristics of a number of individual internal gravity waves are discussed and compared by using a multilayer, time-averaged model in which the waves lose energy due to viscous, thermal conduction and ion-drag dissipation. From this both the height and horizontal distance (from an assumed 'source') at which the waves achieve a maximum density amplitude may be determined. Such calculations are performed for both a very hot and a very cold thermosphere, and the subsequent differences in the wave characteristics and their relation to the control of orbiting spacecraft for each of these is discussed." @default.
- W2093337701 created "2016-06-24" @default.
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- W2093337701 date "1987-03-24" @default.
- W2093337701 modified "2023-09-23" @default.
- W2093337701 title "A theoretical comparison of internal gravity wave propagation and dissipation in high and low temperature thermospheres Implications for orbiting spacecraft" @default.
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- W2093337701 doi "https://doi.org/10.2514/6.1987-266" @default.
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