Statistics, Morphology, and Energetics of Ellerman Bombs

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Sunrise: INSTRUMENT, MISSION, DATA, AND FIRST RESULTS (2010, methodology): “The 80 cm diameter Flare Genesis telescope, equipped with a sophisticated Fabry-Pérot based vector magnetograph (Rust et al. 1996), flew in 1996 and in 2000, achieving a spatial resolution of roughly 0.5 arcsec (Georgoulis et al. 2002) during the second flight.”
Resistive Emergence of Undulatory Flux Tubes (2004, methodology): “Using the same FGE data set, Georgoulis et al. 2002 (hereafter GRBS02) and Bernasconi et al. (2002) have shown that many small-scale, intermittent H brightenings, called Ellerman bombs (EBs), occurred during the emergence phase.”
25 Years of Self-Organized Criticality: Solar and Astrophysics (2014, background): “…(1998), McIntosh and Gurman (2005); 17) Parnell and Jupp (2000), Aschwanden et al. (2000b), Benz and Krucker (2002), Aschwanden and Parnell (2002), Georgoulis et al. (2002); 18) Aschwanden and Shimizu (2013), Aschwanden et al. (2013a); 19) Uritsky et al. (2002); 20) Akabane (1956), Kundu (1965),…”
THE NATURE OF FLARE RIBBONS IN CORONAL NULL-POINT TOPOLOGY (2009, background): “These brightenings are likely to be associated with Ellerman bombs (e.g., Georgoulis et al. 2002; Pariat et al. 2007) and are indicated as Ellerman Bombs (EBs) in Figure 1.”