On the limitations of using radiometric bursts as diagnostic tools for interplanetary coronal mass ejections by J. Kandekar et al. – Community of European Solar Radio Astronomers
Our Sun is constantly active and much of its activity, such as solar flares and coronal mass ejections, is driven by its magnetic fields. However, this magnetic field cannot be directly estimated; It is necessary to employ various observation and radio techniques to estimate these magnetic fields (White 2004; Gopalswamy 2006). While radio-based techniques have…
