Newly available high-resolution imaging of solar radio emission at many closely spaced
frequencies and times provides new physical insight into the processes, structure, and …

Solar type III radio bursts are the most common impulsive radio signatures from the Sun,
stimulated by electron beams traveling through the solar corona and solar wind. Type III …

Solar radio observations provide a unique diagnostic of the outer solar atmosphere.
However, the inhomogeneous turbulent corona strongly affects the propagation of the …

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

Magnetic reconnection, the central engine that powers explosive phenomena throughout the
universe, is also perceived to be one of the principal mechanisms for accelerating particles …

The low frequency array (LOFAR) is a phased array interferometer currently consisting of 13
international stations across Europe and 38 stations surrounding a central hub in the …

Context. Type II radio bursts are evidence of shocks in the solar atmosphere and inner
heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These …

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 …

Coronal mass ejections (CMEs) are believed to be effective in producing shocks in the solar
corona and interplanetary space. One of the important signatures of shocks and shock …

Abstract We present low-frequency (80–240 MHz) radio imaging of type III solar radio bursts
observed by the Murchison Widefield Array on 2015 September 21. The source region for …