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.
|Title of host publication||Proceedings of Science|
|Publisher||Proceedings of Science (PoS)|
|Number of pages||8|
|Publication status||Published - 30 Jul 2015|
|Event||The 34th International Cosmic Ray Conference - The Hague, Netherlands|
Duration: 30 Jul 2015 → 6 Aug 2015
|Conference||The 34th International Cosmic Ray Conference|
|Period||30/07/15 → 6/08/15|
Bibliographical noteWe 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