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Titlebook: Geospace Electromagnetic Waves and Radiation; James W. LaBelle,Rudolf A. Treumann Book 2006 Springer-Verlag Berlin Heidelberg 2006 auroral

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樓主: 欺騙某人
31#
發(fā)表于 2025-3-27 00:38:29 | 只看該作者
32#
發(fā)表于 2025-3-27 03:01:09 | 只看該作者
33#
發(fā)表于 2025-3-27 09:10:36 | 只看該作者
Auroral Acceleration and Radiationcesses taking place at the tailward reconnection site. It is shown that most of the acceleration in the aurora is due to local field-aligned electric potentials which are located in vertically narrow double layers along the magnetic field of the order of ~10 km and which are the site of preferential
34#
發(fā)表于 2025-3-27 11:21:24 | 只看該作者
The Influence of Plasma Density Irregularities on Whistler-Mode Wave Propagations, present in all parts of the magnetosphere, occur at scale lengths ranging from a few meters to several hundred kilometers and larger. Given the spatial sizes of FAI and typical wavelength of W-mode waves found in the magnetosphere, it is convenient to classify FAI into three broad categories: lar
35#
發(fā)表于 2025-3-27 17:24:24 | 只看該作者
Dipole Measurements of Waves in the Ionosphere OEDIPUS C (OC). The transmission of electromagnetic signals over a 1-km distance in the ionosphere has been used to substantiate the theory of emission, propagation and detection of waves in a cold magnetoplasma. Confirmations and insights about the dipole theory arising from the OC research result
36#
發(fā)表于 2025-3-27 19:50:57 | 只看該作者
Mode Conversion Radiation in the Terrestrial Ionosphere and Magnetospherethat they result from generation of electrostatic waves by unstable particle populations followed by conversion of some fraction of the wave energy to electromagnetic modes which then propagate relatively long distances. In particular, we address the complex frequency structure observed in terrestri
37#
發(fā)表于 2025-3-27 23:32:31 | 只看該作者
38#
發(fā)表于 2025-3-28 05:56:12 | 只看該作者
Plasma Waves Near Reconnection Sites electron plasma frequency. Here we explore the observations near the reconnection sites of high frequency waves, frequencies well above the ion gyrofrequency. We concentrate on in situ satellite observations, particularly on recent observations by the Cluster spacecraft and, where possible, compare
39#
發(fā)表于 2025-3-28 06:33:38 | 只看該作者
Tests of Time Evolutions in Deterministic Models, by Random Sampling of Space Plasma Phenomenalarly useful for interpreting data from instrumented spacecraft. These “new methods” are applied to examples of localized bursts of lower-hybrid waves and correlated density depletions observed on the FREJA satellite. In particular, lower-hybrid wave collapse is investigated. The statistical argumen
40#
發(fā)表于 2025-3-28 13:16:03 | 只看該作者
Propagation Analysis of Electromagnetic Waves: Application to Auroral Kilometric Radiationasurements of the magnetic and electric field fluctuations. One class of analysis methods is based on the assumption of the presence of a single plane wave and can be used to determine the direction of the wave vector. If the wave field is more complex, containing waves which simultaneously propagat
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