Monte Carlo Simulation of Scattering of Solar Radio Emissions

摘要: We present Monte Carlo simulation techniques which are used to study the scattering of solar and interplanetary radio emissions, both thermal non-thermal, by random density fluctuations. examine what extent is responsible for (1) anomalous time delays, large source sizes, increased heights, widespread visibilities type III II bursts, (2) low brightness temperatures quiet sun emission apparent sizes. Using empirically derived models electron densities, fluctuations, we show that mostly unusual behavior nonthermal can be extract characteristics beams CME driven shocks from burst observations observations.