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Titlebook: Cosmic Rays and Earth; Proceedings of an IS J. W. Bieber,E. Eroshenko,R. Kallenbach Conference proceedings 2000 Springer Science+Business M

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41#
發(fā)表于 2025-3-28 15:51:58 | 只看該作者
Conference proceedings 2000ontribu- tions of all participants. Following a general summary of the workshop prepared by the editors, the volume leads off with a keynote article by Professor John Simpson describing his invention of the neutron monitor in 1948 and the early scientific discoveries made with this instrument.
42#
發(fā)表于 2025-3-28 20:28:26 | 只看該作者
43#
發(fā)表于 2025-3-28 22:57:49 | 只看該作者
osphere and describes models and software that have been developed that provide quantitative information about the cosmic radiation exposure at flight altitudes. The discussion is extended to include the cosmic radiation exposure to manned spacecraft.
44#
發(fā)表于 2025-3-29 06:39:29 | 只看該作者
45#
發(fā)表于 2025-3-29 08:31:04 | 只看該作者
46#
發(fā)表于 2025-3-29 12:53:20 | 只看該作者
The Cosmic Ray Nucleonic Component: The Invention and Scientific Uses of the Neutron Monitoreonic component cascade in the atmosphere had a huge geomagnetic latitude dependence. For example, between 0° and 60° this dependence was a ~ 200–400% effect — depending on altitude — thus opening the opportunity to measure the intensity changes in the arriving cosmic-ray nuclei down to ~ 1–2 GeV nu
47#
發(fā)表于 2025-3-29 18:42:50 | 只看該作者
48#
發(fā)表于 2025-3-29 20:57:48 | 只看該作者
Coronal Mass Ejections and Forbush Decreaseserplanetary medium. Such regions, and the shocks which they may generate, have pronounced effects on cosmic ray densities both locally and at some distance away. These energetic particle effects can often be used to identify CMEs in the interplanetary medium, where they are usually called ‘ejecta’.
49#
發(fā)表于 2025-3-30 00:24:14 | 只看該作者
50#
發(fā)表于 2025-3-30 04:52:37 | 只看該作者
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