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Acceleration of electrons in solar flares
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Cheng, C. |
| Copyright Year | 1971 |
| Description | Acceleration of electrons by Langmuir plasma turbulence and by the Fermi mechanism are suggested to explain the two-stage acceleration processes observed in hard X-rays from solar flares. A model for particle acceleration in flares is presented. |
| File Size | 632637 |
| Page Count | 18 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19720003185 |
| Archival Resource Key | ark:/13960/t3pw17w16 |
| Language | English |
| Publisher Date | 1971-10-01 |
| Access Restriction | Open |
| Subject Keyword | Space Radiation Solar Radio Emission X Rays Plasma Turbulence Solar Flares Fermi Surfaces Electron Density Concentration Electrostatic Probes Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |