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Titlebook: ELF-VLF Radio Wave Propagation; Proceedings of the N Jan A. Holtet Conference proceedings 1974 Springer Science+Business Media Dordrecht 19

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书目名称ELF-VLF Radio Wave Propagation
副标题Proceedings of the N
编辑Jan A. Holtet
视频video
丛书名称Nato Science Series C:
图书封面Titlebook: ELF-VLF Radio Wave Propagation; Proceedings of the N Jan A. Holtet Conference proceedings 1974 Springer Science+Business Media Dordrecht 19
描述This volume is based on lectures and discussions presented at a NATO Advanced Study Institute on ELF and VLF Radio Wave Propagation, which was held in Norway April 1974. The study of propagation of electromagnetic waves with frequen­ cies below 100 kHz has long traditions in ionospheric physics. To-day, this frequency range is still of great importance, both to the physicist, who uses the waves as diagnostic tools to study the earth‘s environment and to the engineer who exploits the characteris­ tics of these waves to improve communications, navigation and timing systems. In recent years the active interest in the field has led to very rapid progress in the development of propagation theory as well as in the application of this theory to the solution of practical problems. The intention of the Organizing Committee for this Conference was to bring together theoreticians and experi­ mentalists working on the various aspects of wave propagation, in order to stimulate a fruitful discussion and exchange of ideas.
出版日期Conference proceedings 1974
关键词X-ray; density; electromagnetic wave; electron; energy; experiment; noise; numerical method; physics; radiati
版次1
doihttps://doi.org/10.1007/978-94-010-2265-1
isbn_softcover978-94-010-2267-5
isbn_ebook978-94-010-2265-1Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1974
The information of publication is updating

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Nazi Massacres and Divided Memory,y processes that takes place in the lower thermosphere since some species, which are produced in the lower thermosphere, are brought into the mesosphere by eddy diffusion. It is therefore convenient to include heights up to 110–100 km when photochemical processes in the mesosphere are considered. In
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Random Sequence Model for Nonlinear Systemsd magnetospheric sources. Variations in the energy input to the earth’s atmosphere from these sources have been observed for nearly a half-century by means of a variety of ground based measurements including VLF (3–30 kHz) radio transmissions (e.g. Espenshied 1926; Lauter 1950, 1961; Bracewell et al
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F. J. van Spronsen,A. Bélanger-Quintanaticles within the Earth1s atmosphere. This plasma component of the air is essential for the conversion of kinetic energy of the gas into electromagnetic energy. Electromagnetic energy can be transported within the various height regions and ultimately will be dissipated through Ohm losses. Thus, the
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https://doi.org/10.1007/978-3-642-24936-5adio propagation in the ionosphere. The method differed from other approaches (see, for example, Budden, 1955a, b; Barron and Budden, 1959; Barron 1961; Johler and Harper, 1962; Keller and Keller, 1962; Price, 1964; Inoue and Horowitz, 1966) in its choice of the two solutions which correspond to wav
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