January 2022 – Community of European Solar Radio Astronomers

Radio Probing of Solar Wind Sources in Coronal Magnetic Fields
by A. Koval et al.*

2022-01-18 223 views

The magnetic fields of the Sun govern the solar corona structure where the solar wind emanates and further accelerates supersonically. Therefore, the accurate observational data about the topology, and more significantly, quantities of the coronal magnetic field are pivotal for identifying the solar wind sources as well as for the Space Weather modeling where these data specify initial conditions. Magnetic-field strength values in the solar wind sources are derived from […]

Characterising coronal turbulence using snapshot imaging of radio bursts in 80 – 200 MHz
by Atul Mohan

2022-01-04 184 views

Metrewave solar type-III radio bursts offer a unique means to study the properties of turbulence across coronal heights. Theoretical models have shown that the apparent intensity and size of the burst sources evolve at sub-second scales due to turbulent scattering of radio waves close to their generation sites (Arzner & Magun, 1999; Kontar et al., 2019). The advent of high cadence snapshot spectroscopic imaging capabilities in meter wavebands have made […]