摘要: One of the outstanding problems in solar flare theory is how to explain the 10-20keV and greater hard x-ray emissions by a thick target bremsstrahlung model. The model requires the acceleration mechanism to accelerate approximatel... 展开
作者 | Spicer, D. S. Bingham, R. Su, J. J. Shapiro, V. D. Shevchenko, V. | ||
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原报告号 | N9427953 | 总页数 | 31 |
报告类别/文献类型 | NASA / NTIS科技报告 | ||
关键词 | Bremsstrahlung Electron acceleration Particle acceleration Solar flares Xrays Electrostatic waves Ion distribution Ions Plasma turbulence Plasma waves Space plasmas Wave packets Cyclotron frequency Cyclotron radiation Electron beams Energet |