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The influence of the earth's magnetosphere on the high-energy solar protons
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Makhmutov, V. S. Charakhchyan, T. N. Bazilevskaya, G. A. |
| Copyright Year | 1985 |
| Description | In the Earth's polar regions the intensity of the solar protons with the energy above the critical energy of geomagnetic cutoff is the same as in the interplanetary space. The penumbra in the polar regions is small and the East-West effect is also small. However the geomagnetic cutoff rigidity R sub c in polar regions is difficult to calculate because it is not sufficient to include only the internal sources of the geomagnetic field. During the magneto-quiescent periods the real value of R sub c can be less by 0.1 GV than the calculated value because of the external sources. During the geomagnetic storms the real value of R sub c is still lower. |
| File Size | 285551 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850026780 |
| Archival Resource Key | ark:/13960/t7cs0pz59 |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Geomagnetism Earth Atmosphere Energy Spectra Solar Protons High Energy Electrons Cosmic Rays Energetic Particles Penumbras Earth Magnetosphere Flux Density Flux Rate Magnetic Storms Polar Regions Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
