228 citations · 3.6k across the 86 of their papers we have counts for
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The energetics of a global shock wave in the low solar corona
David M. Long, Deborah Baker, David R. Williams +3
As the most energetic eruptions in the solar system, coronal mass ejections (CMEs) can produce shock waves at both their front and flanks as they erupt from the Sun into the helios…
Solar Hard X-ray Source Sizes in a Beam-Heated and Ionised Chromosphere
A. O'Flannagain, J. C. Brown, P. T. Gallagher
Solar flare hard X-rays (HXRs) are produced as bremsstrahlung when an accelerated population of electrons interacts with the dense chromospheric plasma. HXR observations presented…
LOFAR tied-array imaging of Type III solar radio bursts
D. E. Morosan, P. T. Gallagher, P. Zucca +82
The Sun is an active source of radio emission which is often associated with energetic phenomena such as solar flares and coronal mass ejections (CMEs). At low radio frequencies (<…
Quasiperiodic acceleration of electrons by a plasmoid-driven shock in the solar atmosphere
Eoin P. Carley, David M. Long, Jason P. Byrne +4
Cosmic rays and solar energetic particles may be accelerated to relativistic energies by shock waves in astrophysical plasmas. On the Sun, shocks and particle acceleration are ofte…
The formation heights of coronal shocks from 2D density and Alfvén speed maps
Pietro Zucca, Eoin P. Carley, D. Shaun Bloomfield +1
Super-Alfvénic shock waves associated with coronal mass ejections (CMEs) can produce radio emission known as Type II bursts. In the absence of direct imaging, accurate estimates of…
The Compatibility of Flare Temperatures Observed with AIA, GOES, and RHESSI
Daniel F. Ryan, Aidan M. O'Flannagain, Markus J. Aschwanden +1
We test the compatibility and biases of multi-thermal flare DEM (differential emission measure) peak temperatures determined with AIA with those determined by GOES and RHESSI using…