activity
20032022
most citedObservational Evidence for Gentle Chromospheric Evaporation During the Impulsive Phase of a Solar Flare

125 citations · 962 across the 26 of their papers we have counts for

collaborators
Showing 2018Show all

8 papers · 1 filter

astro-ph.SR2018

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

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

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

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

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

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…