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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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樓主: commotion
11#
發(fā)表于 2025-3-23 12:59:00 | 只看該作者
itors, muon telescope systems use coincidence techniques to obtain directional information about the arriving particle. Neutron monitor observations require simple corrections for pressure variations to compensate for the varying mass of atmospheric absorber over a site. In contrast, muon observatio
12#
發(fā)表于 2025-3-23 14:15:33 | 只看該作者
Transferring Tests Across Web Applicationsability of cosmic radiation data from the early years to the present time. Information on the worldwide network of neutron monitor stations and the availability of these cosmic radiation records is included.
13#
發(fā)表于 2025-3-23 20:19:31 | 只看該作者
14#
發(fā)表于 2025-3-23 22:17:38 | 只看該作者
Andrea Gallidabino,Cesare Pautassosent about half of these are still active. Many of the original questions about the production of atmospheric secondaries, geomagnetic effects, and neutron monitor response in general, have been settled satisfactorily. Due to their long-term reliability and automated data acquisition, the remaining
15#
發(fā)表于 2025-3-24 05:25:07 | 只看該作者
Form Filling Based on Constraint Solvingem is that the trajectory-tracing process involves using mathematical equations that have ‘no solution in closed form’. This difficulty has forced researchers to use the ‘brute force’ technique of numerical integration of many individual trajectories to ascertain the behavior of trajectory families
16#
發(fā)表于 2025-3-24 09:55:33 | 只看該作者
Andrea Gallidabino,Cesare Pautassoy cosmic rays. Simpson (1948) discovered that the latitude variation of the secondary hadronic component was considerably larger than the muon component suggesting the response of a neutron monitor is more sensitive to lower energies in the primary spectrum. The different methods of determining the
17#
發(fā)表于 2025-3-24 12:49:50 | 只看該作者
18#
發(fā)表于 2025-3-24 15:32:18 | 只看該作者
Cosmic Rays and Earth978-94-017-1187-6Series ISSN 1385-7525
19#
發(fā)表于 2025-3-24 22:21:08 | 只看該作者
site of solar flares that are responsible for .-ray, .-ray and neutron emission and particles accelerated at high coronal altitudes and in interplanetary space by travelling disturbances such as coronal mass ejections. Special emphasis is placed on those particles directly or indirectly associated with neutron monitor signals.
20#
發(fā)表于 2025-3-25 03:02:18 | 只看該作者
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