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 proceedingPublished conference contribution

13 Downloads (Pure)


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)
Number of pages8
Publication statusPublished - 30 Jul 2015
EventThe 34th International Cosmic Ray Conference - The Hague, Netherlands
Duration: 30 Jul 20156 Aug 2015


ConferenceThe 34th International Cosmic Ray Conference
CityThe Hague

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


  • cosmic ray
  • space science


Dive into the research topics of 'A Time-dependent and Anisotropic Force Field Model For Galactic Cosmic Ray Flux'. Together they form a unique fingerprint.

Cite this