4 papers · 1 filter
Shock Signatures of the Successive Type-II Solar Radio Bursts at Meter Wavelength
V. Vasanth
The successive type-II solar radio bursts observed on 31 July 2012 by the Bruny Island Radio Spectrometer (BIRS) in the frequency range between 62 - 6 MHz is reported and analyzed.…
Observations of Successive CMEs and their Successive Type II Solar Radio Bursts in the Corona
V. Vasanth
This paper reports the observations of two coronal shocks from two Coronal Mass Ejections (CMEs) for the Successive type II Solar radio bursts observed on 02 May 2021 in the freque…
A Wide-band High-frequency Type-II Solar Radio Burst
V. Vasanth, Yao Chen, G. Michalek
Type-II radio bursts are typically observed below ~ 400 MHz, with narrow-band slowly-drifting fundamental and harmonic structures. Here we report an unusual high-frequency wide-ban…
Source Imaging of a Moving Type-IV Solar Radio Burst and its Role in Tracking Coronal Mass Ejection From the Inner to the Outer Corona
V. Vasanth, Yao Chen, Maoshui Lv +5
Source imaging of solar radio bursts can be used to track energetic electrons and associated magnetic structures. Here we present a combined analysis of data at different wavelengt…