107 citations · 1k across the 34 of their papers we have counts for
34 papers
Tracking solar radio bursts using Bayesian multilateration
L. A. Cañizares, S. T. Badman, S. A. Maloney +4
Solar radio bursts (SRBs), are emitted by electrons propagating through the corona and interplanetary space. Tracking such bursts is key to understanding the properties of accelera…
Imaging a large coronal loop using type U solar radio burst interferometry
Jinge Zhang, Hamish A. S. Reid, Eoin Carley +4
Solar radio U-bursts are generated by electron beams traveling along closed magnetic loops in the solar corona. Low-frequency ( 100 MHz) U-bursts serve as powerful diagnostic to…
The science behind SURROUND: a constellation of CubeSats around the Sun
D. M. Weigt, L. A. Cañizares, S. A. Maloney +6
One of the greatest challenge facing current space weather monitoring operations is forecasting the arrival of coronal mass ejections (CMEs) and Solar Energetic Particles (SEPs) wi…
Improved Type III solar radio burst detection using congruent deep learning models
Jeremiah Scully, Ronan Flynn, Peter Gallagher +2
Solar flares are energetic events in the solar atmosphere that are often linked with solar radio bursts (SRBs). SRBs are observed at metric to decametric wavelengths and are classi…
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…
Interferometric imaging of the type IIIb and U radio bursts observed with LOFAR on 22 August 2017
Bartosz Dabrowski, Katarzyna Mikula, Pawel Flisek +18
The Sun is the source of different types of radio bursts that are associated with solar flares, for example. Among the most frequently observed phenomena are type III solar bursts.…