We estimated the coronal magnetic field strength (BB) during the 23 July 2016 coronal mass
ejection (CME) event using i) the flux rope structure of the CME in the white-light …

We report observations of the high frequency type II radio burst (≈ 430–30 MHz) that
occurred in the solar corona on 2015 November 4. The drift rate of the burst, estimated close …

Forty-one solar type II radio bursts located close to the solar limb (projected radial distance
r≳ 0.8 R☉) were observed at 109 MHz by the radioheliograph at the Gauribidanur …

It is well known that magnetic field strength (B) in the solar corona can be calculated using
the Alfvén Mach number (MA) and Alfvén speed (v A) of the magnetohydrodynamic shock …

We report a solar coronal split-band type II radio burst that was observed on 2016 March 16
with the Gauribidanur Radio Spectro-Polarimeter in the frequency range≈ 90–50 MHz, and …

We carried out a statistical study of twenty-six type II radio bursts from the Sun observed with
the Gauribidanur Low-frequency Solar Spectrograph in the frequency range 85–35 MHz …

Using temporal observations of circular polarized harmonic plasma emission from a split-
band type II solar radio burst at 80 MHz, we separately estimated the coronal magnetic field …

Radio bursts from the solar corona can provide clues to forecast space-weather hazards.
After recent technology advancements, regular monitoring of radio bursts has increased and …

Logarithmic periodic dipole antenna (LPDA) was constructed for monitoring Sun in the
range of (45-870) MHz to precisely match the solar monitoring requirements. In our work, we …

We report on the first long baseline interferometer (length≈ 8 km) observations of the solar
corona at 37 MHz that were carried out recently with an angular resolution of $\approx …