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Titlebook: Exploration of the Polar Upper Atmosphere; Proceedings of the N Charles S. Deehr,Jan A. Holtet Conference proceedings 1981 D. Reidel Publis

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Nato Science Series C:http://image.papertrans.cn/e/image/319396.jpg
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https://doi.org/10.1007/978-94-009-8417-2Absorption; Ionosphere; Precipitation; Scale; Weather; Wind; magnetosphere; satellite
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978-94-009-8419-6D. Reidel Publishing Company, Dordrecht, Holland 1981
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Hayek: A Collaborative Biographyet which limit the quantity of useful data. Nevertheless, there have been a sufficient number of satisfactory observations to allow the characteristic features of high latitude emissions to be identified. In the sections that follow, a summary of results of observations of dayside aurora and polar cap arcs is given.
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Hayek: A Collaborative Biographyfect on the preceding region, the magnetosphere; this in turn influences the form and rate of solar energy delivery to the upper atmosphere. The magnetosphere thus plays an important role as a non-linear transducer of solar energy. For a general review of the solar-terrestrial system see Parker et al. (1979).
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