148 citations · 1.5k across the 48 of their papers we have counts for
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astro-ph.SR2014★ 61 cited
Observational Characteristics of CMEs without Low Coronal Signatures
E. D'Huys, D. B. Seaton, S. Poedts +1
Solar eruptions are usually associated with a variety of phenomena occurring in the low corona before, during, and after onset of eruption. Though easily visible in coronagraph obs…
astro-ph.SR2014★ 66 cited
Observational evidence of torus instability as trigger mechanism for coronal mass ejections: the 2011 August 4 filament eruption
Francesco P. Zuccarello, Daniel B. Seaton, Marilena Mierla +4
Solar filaments are magnetic structures often observed in the solar atmosphere and consist of plasma that is cooler and denser than their surroundings. They are visible for days --…