Radio spectral evolution of an X-ray-poor impulsive solar flare: Implications for plasma heating and electron acceleration

Keyphrases

• Decay Phases 16%
• Decreasing Frequency 16%
• Electron Acceleration 100%
• Flux Density 16%
• Hard X-ray 16%
• Maximum Density 16%
• Model Fitting 16%
• Owens Valley 16%
• Parametric Trend 16%
• Plasma Heating 100%
• Polarimeter 16%
• Radio 100%
• Radio Emission 33%
• Radio Frequency 16%
• Radio Spectrum 16%
• Radioheliograph 16%
• Relatively Dense 16%
• Solar Array 16%
• Solar Flares 100%
• Source Model 16%
• Spectral Coverage 16%
• Spectral Evolution 100%
• Stochastic Acceleration 16%
• Thermal Plasma 16%
• Wavelength Band 16%
• X-ray 100%
• X-ray Emission 33%
• X-ray Observations 16%

Earth and Planetary Sciences

• Electron Acceleration 100%
• Electron Energy 50%
• Emissions 100%
• Flux Density 50%
• GOES 50%
• Plasma Heating 100%
• Polarimeter 50%
• Radio Emission 100%
• Radio Frequency 50%
• Radio Spectra 50%
• Solar Array 50%
• Solar Flare 100%
• Thermal Plasma 50%
• Time Series 50%

Physics

• Electron Acceleration 100%
• Electron Energy 50%
• Flux Density 50%
• Plasma Heating 100%
• Polarimeter 50%
• Radio Emission 100%
• Radio Spectra 50%
• Radioheliographs 50%
• Solar Array 50%
• Solar Flare 100%
• Thermal Plasma 50%