22 citations · 42 across the 5 of their papers we have counts for
6 papers
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…
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…
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…
Tracking a beam of electrons from the low solar corona into interplanetary space with the Low Frequency Array, Parker Solar Probe and 1 au spacecraft
Samuel T. Badman, Eoin P. Carley, Luis Alberto Cañizares +7
Type III radio bursts are the result of plasma emission from mildly relativistic electron beams propagating from the low solar corona into the heliosphere where they can eventually…
First Results from the REAL-time Transient Acquisition backend (REALTA) at the Irish LOFAR station
P. C. Murphy, P. Callanan, J. McCauley +27
Modern radio interferometers such as the LOw Frequency ARray (LOFAR) are capable of producing data at hundreds of gigabits to terabits per second. This high data rate makes the ana…
An Improved Orbital Period for GY Cancri Based on Two K2 Campaigns
Luis Alberto Canizares, Peter Garnavich, Colin Littlefield +4
GY Cnc is a deeply eclipsing cataclysmic variable star with an orbital period of 4.21 hours that has shown several dwarf nova outbursts. The variable was continuously observed by t…