Observation and modeling of small spatial structures of solar radio noise storms using the UGMRT by S. Mondal et al. – European astronomer radio community
One of the most commonly observed solar radio sources in metric and decametric wavelengths are the so -called solar noise storms. These are generally associated with active regions and are believed to be driven by the plasma emission mechanism. Since plasma emission emits mainly in the fundamental and harmonic of the frequency of local plasma,…
