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On reflecting boundary behind the earth's orbit at propagation of fast particles from solar flares
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Filippov, A. T. Nishkovskikh, A. S. |
| Copyright Year | 1985 |
| Description | The flares of solar cosmic rays (SCR) associated with the presence of shocks in interplanetary magnetic field and with their propagation at significant heliocentric distances were always of great interest. Some events and problems concerning the peculiarities of propagation of flare CR in the interplanetary medium are considered. The distinguishing feature of such events is the presence of shock front behind the Earth's orbit having formed either directly in the process of shock generation on the Sun or at large heliocentric distances as a result of the interaction of fast and slow quasistationary recurrent solar wind (SW) streams. Based on the experimental material it is shown that the significant nonlinear disturbances in IMF behind the Earth's orbit can yield the occurrence of the additional SCR flux from shock front region as a result of the interaction of flare flux with shock and a partial reflection from it. |
| File Size | 292817 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850026514 |
| Archival Resource Key | ark:/13960/t78s9m87z |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Interplanetary Medium Particle Flux Density Solar Flares Shock Wave Propagation Shock Fronts Solar Protons Solar Cosmic Rays Solar Wind Wave Reflection Earth Orbits Interplanetary Magnetic Fields Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
