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Isotopic overabundances and the energetic particle model of solar flares
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Bravo, S. Perez-Enriquez, R. |
| Copyright Year | 1985 |
| Description | According to the energetic particle model of solar flares particles are efficiently accelerated in the magnetic field loop of an active region (AR) by hydromagnetic turbulence. It is demonstrated that the isotopic overabundances observed in some flares are not a consequence of the flare itself but are characteristic of the plasma in the AR. Only when a flare releases the plasma into the interplanetary space it is possible to observe this anomalous composition at spacecraft locations. |
| File Size | 268698 |
| Page Count | 4 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19850026483 |
| Archival Resource Key | ark:/13960/t07x1893f |
| Language | English |
| Publisher Date | 1985-08-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Plasma Turbulence Solar Flares Magnetohydrodynamic Turbulence Solar Atmosphere Flux Rate Particle Acceleration Magnetic Anomalies Magnetic Fields Solar Wind M Region Energetic Particles Interplanetary Space Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
