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Titlebook: Natural Electromagnetic Phenomena below 30 kc/s; Proceedings of a NAT David F. Bleil Conference proceedings 1964 Springer Science+Business

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51#
發(fā)表于 2025-3-30 12:11:49 | 只看該作者
52#
發(fā)表于 2025-3-30 15:29:29 | 只看該作者
J. E. Lokkens held in conjunction with the 8th FIRA International Conference on Secure and Trust Computing, Data Management, and Applications, STA 2011, in Crete, Greece, in June 2011. STA 2011 is the first conference after the merger of the successful SSDU, UbiSec, and TRUST symposium series previously held fr
53#
發(fā)表于 2025-3-30 17:36:19 | 只看該作者
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發(fā)表于 2025-3-31 00:26:21 | 只看該作者
55#
發(fā)表于 2025-3-31 00:53:45 | 只看該作者
Some Aspects of the Structure and Dynamics of the Terrestrial Magnetosphere,tion of the fact that gaseous comet tails tend to trail directly away from the sun. It had been known for many years that magnetic storms must be the result of isolated bursts of corpuscular radiation, and the fact that some aurora and geomagnetic disturbance always occur at high latitudes may be co
56#
發(fā)表于 2025-3-31 06:24:19 | 只看該作者
57#
發(fā)表于 2025-3-31 10:21:24 | 只看該作者
The Ionosphere: Propagation Theory,es. The ionization is produced (Friedman, 1962; Ratcliffe, 1960) by the short-wave electromagnetic spectrum of the sun, X-rays and ultra-violet; and to some extent by particles, cosmic rays, meteors, and ion clouds from the sun. In general, a given ionizing agent will produce a layer with maximum io
58#
發(fā)表于 2025-3-31 16:14:38 | 只看該作者
Experimental Results and Tentative Explanations for Geomagnetic Effects Caused by High Altitude Nuc effects. From the study of all these effects, we will restrict our present investigation to the discussion of the magnetic perturbations caused by such detonations. We feel that this limitation is justified, not only for the sake of coherency, but also for the two subsequent reasons:
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