For decades, observations of Faraday rotation have provided unique insights into the
plasma density and magnetic field structure of the solar wind. Faraday rotation (FR) is the …

The structure of the upper solar atmosphere, on all observable scales, is intimately governed
by the magnetic field. The same holds for a variety of solar phenomena that constitute solar …

Context. Meter-wavelength type II solar radio bursts are thought to be the signatures of
shock-accelerated electrons in the corona. Studying these bursts can give information about …

Context. The Sun produces the most powerful explosions in the Solar System, solar flares,
which can also be accompanied by large eruptions of magnetised plasma, coronal mass …

Context. Type II radio bursts are a type of solar radio bursts associated with coronal shocks.
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …

Measuring the physical parameters of coronal mass ejections (CMEs), particularly their
entrained magnetic field, is crucial for understanding their physics and for assessing their …

Type II solar radio bursts are caused by magnetohydrodynamic (MHD) shocks driven by
solar eruptive events such as coronal mass ejections (CMEs). Often, both fundamental and …

Context. One of the most prominent sources for energetic particles in our Solar System are
huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections …

We present spectropolarimetric imaging observations of the solar corona at low frequencies
(80–240 MHz) using the Murchison Widefield Array (MWA). These images are the first of …

The Sun is an active star that often produces numerous bursts of electromagnetic radiation
at radio wavelengths. Low frequency radio bursts have recently been brought back to light …