Energetic particle fluxes data base of "CORONAS-I" satellite observations

A. Dmitriev; S. Kuznetsov; M. Panasyuk; S. Ryumin

doi:10.1016/S0273-1177(98)00012-X

Energetic particle fluxes data base of "CORONAS-I" satellite observations

A. Dmitriev, S. Kuznetsov, M. Panasyuk, S. Ryumin

Department of Space Science and Engineering

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

Abstract

The data hase DB SCR uses data obtained by the SCR instrument package on the CORONAS-I satellite. DB SCR contains information about fluxes of relativistic electrons (0.5-124 MeV), protons (1-300 MeV), nuclei (1-19 MeV/nucl) and γ-radiation (0.1-7 MeV) in the low altitude region (500 km). The time resolution of the data is 2.5 s. Magnetic field parameters (B, magnetic latitude and longitude), L-shell and local times (LT and MLT) are included in DB SCR. Since all parameters are equivalents it is possible to perform the multidimensional analysis for any set of DB SCR parameters. The additional DB SCR software packages may be used to develop different semi-empirical models.

Original language	English
Pages (from-to)	1669-1674
Number of pages	6
Journal	Advances in Space Research
Volume	21
Issue number	12
DOIs	https://doi.org/10.1016/S0273-1177(98)00012-X
State	Published - 1998

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title = "Energetic particle fluxes data base of {"}CORONAS-I{"} satellite observations",

abstract = "The data hase DB SCR uses data obtained by the SCR instrument package on the CORONAS-I satellite. DB SCR contains information about fluxes of relativistic electrons (0.5-124 MeV), protons (1-300 MeV), nuclei (1-19 MeV/nucl) and γ-radiation (0.1-7 MeV) in the low altitude region (500 km). The time resolution of the data is 2.5 s. Magnetic field parameters (B, magnetic latitude and longitude), L-shell and local times (LT and MLT) are included in DB SCR. Since all parameters are equivalents it is possible to perform the multidimensional analysis for any set of DB SCR parameters. The additional DB SCR software packages may be used to develop different semi-empirical models.",

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T1 - Energetic particle fluxes data base of "CORONAS-I" satellite observations

AU - Dmitriev, A.

AU - Kuznetsov, S.

AU - Panasyuk, M.

AU - Ryumin, S.

PY - 1998

Y1 - 1998

N2 - The data hase DB SCR uses data obtained by the SCR instrument package on the CORONAS-I satellite. DB SCR contains information about fluxes of relativistic electrons (0.5-124 MeV), protons (1-300 MeV), nuclei (1-19 MeV/nucl) and γ-radiation (0.1-7 MeV) in the low altitude region (500 km). The time resolution of the data is 2.5 s. Magnetic field parameters (B, magnetic latitude and longitude), L-shell and local times (LT and MLT) are included in DB SCR. Since all parameters are equivalents it is possible to perform the multidimensional analysis for any set of DB SCR parameters. The additional DB SCR software packages may be used to develop different semi-empirical models.

AB - The data hase DB SCR uses data obtained by the SCR instrument package on the CORONAS-I satellite. DB SCR contains information about fluxes of relativistic electrons (0.5-124 MeV), protons (1-300 MeV), nuclei (1-19 MeV/nucl) and γ-radiation (0.1-7 MeV) in the low altitude region (500 km). The time resolution of the data is 2.5 s. Magnetic field parameters (B, magnetic latitude and longitude), L-shell and local times (LT and MLT) are included in DB SCR. Since all parameters are equivalents it is possible to perform the multidimensional analysis for any set of DB SCR parameters. The additional DB SCR software packages may be used to develop different semi-empirical models.

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U2 - 10.1016/S0273-1177(98)00012-X

DO - 10.1016/S0273-1177(98)00012-X

M3 - 期刊論文

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AN - SCOPUS:0032228197

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JO - Advances in Space Research

JF - Advances in Space Research

IS - 12

ER -

Energetic particle fluxes data base of "CORONAS-I" satellite observations

Abstract

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