107 citations · 1k across the 34 of their papers we have counts for
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Evolution of the Alfvén Mach number associated with a coronal mass ejection shock
Ciara A. Maguire, Eoin P. Carley, Joseph McCauley +1
The Sun regularly produces large-scale eruptive events, such as coronal mass ejections (CMEs) that can drive shock waves through the solar corona. Such shocks can result in electro…
Comprehensive Characterization of Solar Eruptions With Remote and In-Situ Observations, and Modeling: The Major Solar Events on 4 November 2015
Iver H. Cairns, Kamen A. Kozarev, Nariaki V. Nitta +12
Solar energetic particles (SEPs) are an important product of solar activity. They are connected to solar active regions and flares, coronal mass ejections (CMEs), EUV waves, shocks…
Multiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection
Diana E. Morosan, Eoin P. Carley, Laura A. Hayes +8
The Sun is an active star that can launch large eruptions of magnetised plasma into the heliosphere, called coronal mass ejections (CMEs). These ejections can drive shocks that acc…
Variable emission mechanism of a Type IV radio burst
D. E. Morosan, E. K. J. Kilpua, E. P. Carley +1
Context. The Sun is an active star and the source of the largest explosions in the solar system, such as flares and coronal mass ejections (CMEs). Flares and CMEs are powerful part…
Properties and magnetic origins of solar S-bursts
Brendan P. Clarke, Diana E. Morosan, Peter T. Gallagher +3
Context. Solar activity is often accompanied by solar radio emission, consisting of numerous types of solar radio bursts. At low frequencies (<100 MHz) radio bursts with short dura…