CLEAR
发表于 2025-3-26 23:25:27
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doxazosin
发表于 2025-3-27 02:08:22
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Ondines-curse
发表于 2025-3-27 08:35:42
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享乐主义者
发表于 2025-3-27 09:30:02
New Observations of the Proton Population of the Radiation Belt Between 1.5 and 104 Mevesting theoretical concepts has been the incompleteness of the available data. Several surveys of the trapped proton population have been performed previously (Davis and Williamson, 1963; Freden ., 1965; Fillius, 1966; Gabbe and Brown, 1966; Mihalov and White, 1966; Vernov ., 1967; De Forest, 1970;
送秋波
发表于 2025-3-27 14:37:47
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LAIR
发表于 2025-3-27 18:35:35
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antedate
发表于 2025-3-28 00:33:40
Electron Intensities over Auroral Arcsm these measurements is that both the auroral arcs occurred at the boundary between two magnetospheric plasmas. This conclusion is based on the fact that some of the observed changes in electron energy spectrum are unlike the changes to be expected on grounds of continuity from a single source plasm
Suppository
发表于 2025-3-28 03:28:49
The Pre-Midnight Asymmetry in the 40 keV Electron Flux Profiles and Its Relation to Magnetospheric Sboundary, often reveal striking asymmetric deviations of the electron flux levels from the average longitudinal or LT distributions. Among these, the most prominent recurrent asymmetric deviation involves an electron flux profile in the dusk-midnight sector which is terminated by a narrow steep spik
regale
发表于 2025-3-28 06:26:06
https://doi.org/10.1007/978-94-010-2896-7Planet; Population; Variation; magnetosphere; solar
单独
发表于 2025-3-28 12:28:21
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