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• W2005301849 abstract "The inner zone population of trapped α particles in the energy range 2.14–9.0 Mev was measured during 1969. The measurements show that inner zone α particles are strongly peaked in pitch angle and that the intensity decreases rapidly with decreasing L value. The α particle spectra are flat and closely resemble inner zone proton spectra at comparable energies. The α/p ratio is roughly independent of L (1.6 ≲ L ≲ 2.0) and energy (0.293–1.14 Mev/nucleon) and is ∼1–4 × 10−3. The computed α particle distribution function strongly suggests that the inner zone is populated by α particles that diffuse inward, conserving M and J. A value of the diffusion coefficient is derived, DLL = 1.2 × 10−8 L10 day−1, that is in good agreement with earlier proton studies." @default.
• W2005301849 created "2016-06-24" @default.
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• W2005301849 date "1973-09-01" @default.
• W2005301849 modified "2023-09-23" @default.
• W2005301849 title "Geomagnetically trapped alpha particles: 2. The inner zone" @default.
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• W2005301849 doi "https://doi.org/10.1029/ja078i025p05498" @default.
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