A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux

Grace D Ihongo; Charles H T Wang

A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux

Research output: Chapter in Book/Report/Conference proceeding › Published conference contribution

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Abstract

Galactic cosmic ray flux calculated at 1au within the energy range (0.2-88) Ge V using the model is presented. The relationship between the calculated flux and solar wind is analyzed and presented. Short-time variation of the flux at a fixed energy range is also calculated, and this is used to predict galactic cosmic ray intensity variation at earth.

Original language	English
Title of host publication	Proceedings of Science
Publisher	Proceedings of Science (PoS)
Pages	1-8
Number of pages	8
Volume	190
Publication status	Published - 30 Jul 2015
Event	The 34th International Cosmic Ray Conference - The Hague, Netherlands Duration: 30 Jul 2015 → 6 Aug 2015

Conference

Conference	The 34th International Cosmic Ray Conference
Country/Territory	Netherlands
City	The Hague
Period	30/07/15 → 6/08/15

Bibliographical note

We sincerely appreciate the following people /groups for their useful contributions.
• Members of the QG2 University of Aberdeen, UK.
• H. Moraal, School of Physics, Potchefstroom University, Potchefstroom, 2520, South Africa.
• R. A. Caballero-Lopez, Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA

Keywords

cosmic ray
space science

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A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux
Copyright owned by the author(s). Given the Open Access nature of this proceedings collection, PoS has chosen to apply the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. http://creativecommons.org/licenses/by-nc-nd/4.0/
Final published version, 614 KBLicence: CC BY-NC-ND

Cite this

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title = "A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux",

abstract = "Galactic cosmic ray flux calculated at 1au within the energy range (0.2-88) Ge V using the model is presented. The relationship between the calculated flux and solar wind is analyzed and presented. Short-time variation of the flux at a fixed energy range is also calculated, and this is used to predict galactic cosmic ray intensity variation at earth.",

keywords = "cosmic ray, space science",

author = "Ihongo, {Grace D} and Wang, {Charles H T}",

note = "We sincerely appreciate the following people /groups for their useful contributions. • Members of the QG2 University of Aberdeen, UK. • H. Moraal, School of Physics, Potchefstroom University, Potchefstroom, 2520, South Africa. • R. A. Caballero-Lopez, Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA ; The 34th International Cosmic Ray Conference ; Conference date: 30-07-2015 Through 06-08-2015",

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day = "30",

language = "English",

volume = "190",

pages = "1--8",

booktitle = "Proceedings of Science",

publisher = "Proceedings of Science (PoS)",

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TY - GEN

T1 - A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux

AU - Ihongo, Grace D

AU - Wang, Charles H T

N1 - We sincerely appreciate the following people /groups for their useful contributions. • Members of the QG2 University of Aberdeen, UK. • H. Moraal, School of Physics, Potchefstroom University, Potchefstroom, 2520, South Africa. • R. A. Caballero-Lopez, Institute for Physical Science and Technology, University of Maryland, College Park, MD 20742, USA

PY - 2015/7/30

Y1 - 2015/7/30

N2 - Galactic cosmic ray flux calculated at 1au within the energy range (0.2-88) Ge V using the model is presented. The relationship between the calculated flux and solar wind is analyzed and presented. Short-time variation of the flux at a fixed energy range is also calculated, and this is used to predict galactic cosmic ray intensity variation at earth.

AB - Galactic cosmic ray flux calculated at 1au within the energy range (0.2-88) Ge V using the model is presented. The relationship between the calculated flux and solar wind is analyzed and presented. Short-time variation of the flux at a fixed energy range is also calculated, and this is used to predict galactic cosmic ray intensity variation at earth.

KW - cosmic ray

KW - space science

M3 - Published conference contribution

VL - 190

SP - 1

EP - 8

BT - Proceedings of Science

PB - Proceedings of Science (PoS)

T2 - The 34th International Cosmic Ray Conference

Y2 - 30 July 2015 through 6 August 2015

ER -

A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux

Abstract

Conference

Bibliographical note

Keywords

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Cite this