37 citations · 106 across the 8 of their papers we have counts for
8 papers
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…
Coronal Signatures of Flare Generated Fast Mode Wave at EUV and Radio wavelengths
V. Vasanth
This paper presents a detailed study of the type II solar radio burst that occurred on 06 March 2014 using combined data analysis. It is a classical radio event consisting of type…
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…
An Eruptive Hot-Channel Structure Observed at Metric Wavelength as a Moving Type-IV Solar Radio Burst
V. Vasanth, Yao Chen, Shiwei Feng +5
Hot channel (HC) structure, observed in the high-temperature passbands of the AIA/SDO, is regarded as one candidate of coronal flux rope which is an essential element of solar erup…
Observation of a Metric Type N Solar Radio Burst
Xiangliang Kong, Yao Chen, Shiwei Feng +7
Type III and type-III-like radio bursts are produced by energetic electron beams guided along coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the…
Investigation on the Coronal Magnetic Field Using a Type II Solar Radio Burst
V. Vasanth, S. Umapathy, B. Vršnak +2
The Type-II solar radio burst recorded on 13 June 2010 by the radio spectrograph of the Hiraiso Solar Observatory was employed to estimate the magnetic-field strength in the solar…