An empirical model of the radiation belt of helium nuclei

I. V. Getselev; E. N. Sosnovets; A. S. Kovtyukh; A. V. Dmitriev; M. V. Podzolko; N. A. Vlasova; S. Ya Reizman

doi:10.1007/s10604-005-0040-6

An empirical model of the radiation belt of helium nuclei

I. V. Getselev, E. N. Sosnovets, A. S. Kovtyukh, A. V. Dmitriev, M. V. Podzolko, N. A. Vlasova, S. Ya Reizman

太空科學與工程學系

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

6 引文斯高帕斯（Scopus）

摘要

Based on satellite data, we present the results of modeling the spatial and energy distributions of integral fluxes of He nuclei (α particles) with E > 1, 2, 4, and 7 MeV at L = 1.1-6.6 in a broad range of B/B ₀ (E is the kinetic energy of particles, L is the drift shell parameter, and B/B ₀ is the magnetic field ratio). Some ways of practically applying the model are considered. The results of calculation of α-particle fluxes for a circular orbit with a height of 300 km and an inclination of 50° are presented.

原文	???core.languages.en_GB???
頁（從 - 到）	229-232
頁數	4
期刊	Cosmic Research
卷	43
發行號	4
DOIs	https://doi.org/10.1007/s10604-005-0040-6
出版狀態	已出版 - 7月 2005

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10.1007/s10604-005-0040-6

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abstract = "Based on satellite data, we present the results of modeling the spatial and energy distributions of integral fluxes of He nuclei (α particles) with E > 1, 2, 4, and 7 MeV at L = 1.1-6.6 in a broad range of B/B 0 (E is the kinetic energy of particles, L is the drift shell parameter, and B/B 0 is the magnetic field ratio). Some ways of practically applying the model are considered. The results of calculation of α-particle fluxes for a circular orbit with a height of 300 km and an inclination of 50° are presented.",

author = "Getselev, {I. V.} and Sosnovets, {E. N.} and Kovtyukh, {A. S.} and Dmitriev, {A. V.} and Podzolko, {M. V.} and Vlasova, {N. A.} and Reizman, {S. Ya}",

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T1 - An empirical model of the radiation belt of helium nuclei

AU - Getselev, I. V.

AU - Sosnovets, E. N.

AU - Kovtyukh, A. S.

AU - Dmitriev, A. V.

AU - Podzolko, M. V.

AU - Vlasova, N. A.

AU - Reizman, S. Ya

PY - 2005/7

Y1 - 2005/7

N2 - Based on satellite data, we present the results of modeling the spatial and energy distributions of integral fluxes of He nuclei (α particles) with E > 1, 2, 4, and 7 MeV at L = 1.1-6.6 in a broad range of B/B 0 (E is the kinetic energy of particles, L is the drift shell parameter, and B/B 0 is the magnetic field ratio). Some ways of practically applying the model are considered. The results of calculation of α-particle fluxes for a circular orbit with a height of 300 km and an inclination of 50° are presented.

AB - Based on satellite data, we present the results of modeling the spatial and energy distributions of integral fluxes of He nuclei (α particles) with E > 1, 2, 4, and 7 MeV at L = 1.1-6.6 in a broad range of B/B 0 (E is the kinetic energy of particles, L is the drift shell parameter, and B/B 0 is the magnetic field ratio). Some ways of practically applying the model are considered. The results of calculation of α-particle fluxes for a circular orbit with a height of 300 km and an inclination of 50° are presented.

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DO - 10.1007/s10604-005-0040-6

M3 - 期刊論文

AN - SCOPUS:24144454178

SN - 0010-9525

VL - 43

SP - 229

EP - 232

JO - Cosmic Research

JF - Cosmic Research

IS - 4

ER -

An empirical model of the radiation belt of helium nuclei

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