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Correction to: Solar Phys https://doi.org/10.1007/s11207-017-1175-3
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Comparison of the peak soft X-ray and 3.6 cm radio luminosity of solar and stellar flares. The upper limits derived from these preflare observations are shown by red arrows. Two peaks in the early main flare phase are indicated with a lowercase red x, the main peak with an uppercase X. We also show nanoflares in quiet regions (Krucker and Benz, 2000), microflares in active regions (Benz et al., 1981; Fürst, Benz, and Hirth, 1982; Gary, Hartl, and Shimizu, 1997), impulsive and gradual flares (Benz and Güdel, 1994), quiescent BY Dra, dMe, and dKe stars (Güdel et al., 1993), and a long-duration flare on the dMe star EQ Peg (Kundu et al., 1988). The dashed line presents the relation given in Equation 1. (Graphics adapted from Benz and Güdel, 2010, and based on Krucker and Benz, 2000.)
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Combined Radio and Space-based Solar Observations: From Techniques to New Results
Guest Editors: Eduard Kontar and Alexander Nindos
The online version of the original article can be found under https://doi.org/10.1007/s11207-017-1175-3.
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Benz, A.O., Battaglia, M. & Güdel, M. Correction to: Observations of a Radio-Quiet Solar Preflare. Sol Phys 293, 32 (2018). https://doi.org/10.1007/s11207-018-1256-y
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DOI: https://doi.org/10.1007/s11207-018-1256-y