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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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樓主: Concave
21#
發(fā)表于 2025-3-25 07:03:11 | 只看該作者
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發(fā)表于 2025-3-25 09:57:58 | 只看該作者
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發(fā)表于 2025-3-25 13:46:16 | 只看該作者
14–16: Austrians and the Holocaust (2)ground and rocket. Observations of differential absorption and phase are discussed in some more detail than other techniques. The possible importance of in-coherent scatter observations also in the D region is pointed out. Better spatial resolution is obtained with probes carried on rockets. Some pr
24#
發(fā)表于 2025-3-25 18:34:48 | 只看該作者
25#
發(fā)表于 2025-3-25 23:38:07 | 只看該作者
Hayek: A Collaborative Biographylar cap processes. The ISIS2 satellite, which is in a circular orbit 1400 km above the earth’s surface, has provided monochromatic optical images of the high latitude region since April 1971. The 5577? emission from atomic oxygen and the 3914 ? emission from the First Negative bands of N.. have been
26#
發(fā)表于 2025-3-26 02:22:19 | 只看該作者
27#
發(fā)表于 2025-3-26 04:29:50 | 只看該作者
Pigou and the Pigouvian Legacy,of some important F-region emissions in the polar regions are reviewed. The importance of optical emissions for the determination of the quantum yields and quenching coefficients is illustrated for the 0.(.P), 0.(.D), N(.D), n(.P) and 0(.D) states and a set of values deduced from recent experiments
28#
發(fā)表于 2025-3-26 10:37:40 | 只看該作者
https://doi.org/10.1007/978-3-319-78069-6bility of the assumptions made in the reduction of data from a single station. Examples of observations made in the Auroral Zone indicating substantial wind gradients and vertical winds are given. Such observations indicate the importance of small scale disturbances in the Polar thermosphere. Data f
29#
發(fā)表于 2025-3-26 13:19:41 | 只看該作者
30#
發(fā)表于 2025-3-26 17:55:41 | 只看該作者
Hayek: A Collaborative Biographydistinct plasma regions, features two important characteristics: (1) As one proceeds from the main particle, energy and momentum source on the sun through the solar wind, the magnetosheath, magnetosphere and ionosphere to the sinks in the neutral atmosphere, one observes an increasingly important fe
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