activity
20032023
most citedA Comparison of Flare Forecasting Methods, I: Results from the "All-Clear" Workshop

228 citations · 3.6k across the 86 of their papers we have counts for

collaborators
Showing 2018Show all

8 papers · 1 filter

astro-ph.SR2018★ 20 cited

Expansion of High Speed Solar Wind Streams from Coronal Holes through the Inner Heliosphere

Tadhg M. Garton, Sophie A. Murray, Peter T. Gallagher

Coronal holes (CHs) are regions of open magnetic flux which are the source of high speed solar wind (HSSW) streams. To date, it is not clear which aspects of CHs are of most influe…

physics.space-ph2018★ 32 cited

A Detailed Model of the Irish High Voltage Power Network for Simulating GICs

Seán P. Blake, Peter T. Gallagher, Joan Campanyà +5

Constructing a power network model for geomagnetically induced current (GIC) calculations requires information on the DC resistances of elements within a network. This information…

astro-ph.SR2018★ 20 cited

Photospheric Shear Flows in Solar Active Regions and Their Relation to Flare Occurrence

Sung-Hong Park, Jordan A. Guerra, Peter T. Gallagher +2

Solar active regions (ARs) that produce major flares typically exhibit strong plasma shear flows around photospheric magnetic polarity inversion lines (MPILs). It is therefore impo…

astro-ph.SR2018★ 1 cited

Three-dimensional magnetic reconnection in a collapsing coronal loop system

Aidan M. O'Flannagain, Shane A. Maloney, Peter T. Gallagher +2

Magnetic reconnection is believed to be the primary mechanism by which non-potential energy stored in coronal magnetic fields is rapidly released during solar eruptive events. Unfo…

astro-ph.SR2018★ 42 cited

CMEs in the Heliosphere: I. A Statistical Analysis of the Observational Properties of CMEs Detected in the Heliosphere from 2007 to 2017 by STEREO/HI-1

R. A. Harrison, J. A. Davies, D. Barnes +10

We present a statistical analysis of coronal mass ejections (CMEs) imaged by the Heliospheric Imager (HI) instruments aboard NASAs twin-spacecraft STEREO mission between April 2007…

astro-ph.SR2018★ 85 cited

Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

P. Zucca, D. E. Morosan, A. P. Rouillard +62

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 shocks may be ass…

astro-ph.SR2018★ 33 cited

Connecting Coronal Mass Ejections to their Solar Active Region Sources: Combining Results from the HELCATS and FLARECAST Projects

Sophie A. Murray, Jordan A. Guerra, Pietro Zucca +5

Coronal mass ejections (CMEs) and other solar eruptive phenomena can be physically linked by combining data from a multitude of ground-based and space-based instruments alongside m…

astro-ph.SR2018★ 3 cited

Characteristics of type III radio bursts and solar S bursts

D. E. Morosan, P. T. Gallagher

The Sun is an active source of radio emission which is often associated with the acceleration of electrons arising from processes such as solar flares and coronal mass ejections (C…