21 citations · 38 across the 6 of their papers we have counts for
6 papers
The SKA as a Probe of Heliospheric Turbulence and Radio-wave Propagation Effects
Nicolina Chrysaphi, Eduard P. Kontar, Hamish A. S. Reid +3
Density turbulence in the heliosphere can impact traversing radio photons originating from anywhere in the universe, leading to distortions of both the spectroscopic and imaging pr…
Multiple shocks generated by the 2024 May 14 coronal mass ejection
Mohamed Nedal, Catherine Cuddy, David M. Long +3
This study characterises a series of type~II radio bursts associated with a CME that occurred on 14 May, focusing on the coronal conditions during the event and identifying the lik…
Bursty acceleration and 3D trajectories of electrons in a solar flare
Shilpi Bhunia, Laura A. Hayes, Karl Ludwig Klein +3
During a solar flare, electrons are accelerated to non-thermal energies as a result of magnetic reconnection. These electrons then propagate upwards and downwards from the energy r…
Electron Beam Propagation and Radio-Wave Scattering in the Inner Heliosphere using Five Spacecraft
Luis Alberto Cañizares, Sam T. Badman, Nicolina Chrysaphi +4
Solar energetic particles such as electrons can be accelerated to mildly-relativistic velocities in the solar corona. These electrons travel through the turbulent corona generating…
Imaging-spectroscopy of a band-split type II solar radio burst with the Murchison Widefield Array
Shilpi Bhunia, Eoin P. Carley, Divya Oberoi +1
Type II solar radio bursts are caused by magnetohydrodynamics (MHD) shocks driven by solar eruptive events such as Coronal Mass Ejections (CMEs). Often both fundamental and harmoni…
Robust absolute solar flux density calibration for the Murchison Widefield Array
Devojyoti Kansabanik, Surajit Mondal, Divya Oberoi +2
Sensitive radio instruments are optimized for observing faint astronomical sources, and usually need to attenuate the received signal when observing the Sun. There are only a handf…