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Titlebook: Magnetospheric Particles and Fields; Proceedings of the S B. M. McCormac Conference proceedings 1976 D. Reidel Publishing Company, Dordrech

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楼主: collude
发表于 2025-3-25 04:54:54 | 显示全部楼层
Waves in the Vicinity of the Magnetopause, orbit to orbit. The appearance of the local magnetopause is determined largely by the boundary conditions imposed by the interplanetary field and the geomagnetic dipole. Magnitude changes across the magnetopause are frequently absent, and if concurrently the magnetosheath and magnetosphere fields a
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Magnetotail Model,osphere one has to use simplifying assumptions. Unfortunately, the same simplifying factors are not uniformly applicable to the entire magnetosphere, so that the existing quantitative results have fairly limited ranges of applicability. This is the reason why this paper deals with the theory of the
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Anomalous Resistivity and Parallel Electric Fields, fundamental plasma physics, to fusion studies, and to the dynamics of astrophysical plasmas. The fundamental plasma physics interest stems from the incomplete experimental and theoretical understanding of the variety of instability and saturation mechanisms possible under different conditions. The
发表于 2025-3-26 02:24:52 | 显示全部楼层
Explorer 45 Observations of the Proton Ring Current,ements of the pitch angle distributions of trapped ring current protons from 1 to 800 keV along with simultaneous measurements of the geomagnetic field. In this paper, I summarize some analyses of Explorer 45 observation that have added to our understanding of the stormtime ring current.
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Geomagnetically Trapped Alpha Particles,vailable. The early measurements dealt almost exclusively with particles in the outer zone which were mirroring far from the geomagnetic equator. Those studies showed that the relative abundance of .-particles to protons, ../.., was ~ 10. for ./. ≥ 0.5 MeV per nucleon, and that ../.. increased with
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The Structure and Stability of Radiation Belt Electrons as Controlled by Wave-Particle Interactionseractions. Rates of precipitation loss to the atmosphere are consistent with anticipated pitch angle diffusion due to parasitic resonant scattering by naturally generated whistler mode hiss. During the recovery phase of magnetic storms such emissions intensify causing relatively rapid electron preci
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Substorm Generated Fluxes of Heavy Ions at the Geostationary Orbit,irst definitive measurements of energetic heavy ions present in the vicinity of the geostationary orbit. In a single reasonably isolated injection event which occurred on June 18, 1974, the following has been found:
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