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

Grace D Ihongo, Charles H T Wang

Research output: Chapter in Book/Report/Conference proceedingConference 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 languageEnglish
Title of host publicationProceedings of Science
PublisherProceedings of Science (PoS)
Pages1-8
Number of pages8
Volume190
Publication statusPublished - 30 Jul 2015
EventThe 34th International Cosmic Ray Conference - The Hague, Netherlands
Duration: 30 Jul 20156 Aug 2015

Conference

ConferenceThe 34th International Cosmic Ray Conference
CountryNetherlands
CityThe Hague
Period30/07/156/08/15

Keywords

  • cosmic ray
  • space science

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    Ihongo, G. D., & Wang, C. H. T. (2015). A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux. In Proceedings of Science (Vol. 190, pp. 1-8). [PoS(ICRC2015)190] Proceedings of Science (PoS).