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

Department of Space Science and Engineering

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

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.

Original language	English
Pages (from-to)	229-232
Number of pages	4
Journal	Cosmic Research
Volume	43
Issue number	4
DOIs	https://doi.org/10.1007/s10604-005-0040-6
State	Published - Jul 2005

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title = "An empirical model of the radiation belt of helium nuclei",

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.

UR - http://www.scopus.com/inward/record.url?scp=24144454178&partnerID=8YFLogxK

U2 - 10.1007/s10604-005-0040-6

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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