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Titlebook: Wave Propagation in the Ionosphere; Karl Rawer Book 1993 Springer Science+Business Media Dordrecht 1993 eigenvalue.electromagnetic wave.gr

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41#
發(fā)表于 2025-3-28 17:23:38 | 只看該作者
Properties of a magnetized plasmaere. It was soon found that the terrestrial magnetic field must be the source of this phenomenon. In fact, the oscillation of each individual electron excited by the electric field of the wave is disturbed by the magnetic field which exercises a force perpendicular to the motion of the charge. There
42#
發(fā)表于 2025-3-28 20:22:51 | 只看該作者
43#
發(fā)表于 2025-3-28 23:24:40 | 只看該作者
44#
發(fā)表于 2025-3-29 06:46:41 | 只看該作者
45#
發(fā)表于 2025-3-29 09:50:56 | 只看該作者
46#
發(fā)表于 2025-3-29 15:01:41 | 只看該作者
47#
發(fā)表于 2025-3-29 16:45:28 | 只看該作者
Propagation in the space between Earth and ionosphere (deka- and hektometer-waves)ortance, on the other hand, is mainly still due to the fact that it allows waves with frequencies in the HF-band and below to propagate from ground to ground over very large distances, and that it influences quite considerably the ground-to-space and space-to-ground propagation of radio waves of hig
48#
發(fā)表于 2025-3-29 20:58:51 | 只看該作者
Propagation through the ionosphere the ultraviolet ranges. In fact, absorption sets the decisive limits to groundbased optical astronomy. The situation is quite different with radio waves. While strong absorption occurs only in certain frequency ranges and at certain hours (e.g. for LF and MF waves during daylight hours), the most i
49#
發(fā)表于 2025-3-30 01:20:21 | 只看該作者
Propagation in the Earth-ionosphere waveguide (Kilometric and longer waves)low, in the D-layer. Our considerations in Section 3.3 and Chapter 6 were for small . (= ./.) so that the collisional influence remained weak. The reflection mechanism was “refractive” because an electron made many oscillations before it was stopped by a collision. It was justified to consider (in C
50#
發(fā)表于 2025-3-30 06:09:44 | 只看該作者
The real ionosphere: Irregularities and acoustic-gravity waves depending only on the vertical coordinate. This, however, is an oversimplification because the actual conditions in the terrestrial ionosphere are more involved. Since the ionosphere is under solar control, all ionospheric parameters vary with local time so that large-scale horizontal gradients exi
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