A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation

By A. Warmuth, B. Vršnak, Jasmina Magdalenic, A. Hanslmeier, W. Otruba. 2004

148 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/1fef2e76c726bdde17c0d41f2350cc81aff43e5c

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In Astronomy and Astrophysics

Citations in the corpus

NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “However, the field of view only starts at 1.3 R⊙, and the domain where coronal waves are observed, below 2 200 Mm (e.g. Warmuth et al. 2004a, 2005; Vršnak et al. 2005; Wills-Davey et al. 2007; Patsourakos et al. 2009) is blocked by the coronagraph occulting disk.”
A multiwavelength study of solar flare waves. I. Observations and basic properties (2004, methodology): “In Paper II (Warmuth et al. 2004), we will combine these results with studies of the perturbation characteristics and the associated metric type II radio bursts to derive a consistent physical interpretation of the flare wave phenomenon.”
OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “In several events, the S-waves coincide spatially with Moreton waves observed at the same time (Khan et al. 2002; Warmuth et al. 2004), which would imply that at least S-waves are the long-sought coronal counterpart to Moreton waves.”
On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “The attempt to associate Moreton and EIT waves (Warmuth et al. 2001, 2004a,b) is also based on high values of β.”
Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “Warmuth et al. (2004a, 2004b) and Cliver et al. (2004) argue for a unified view embracing many of the different types of largescale solar disturbances (favoring flare- and CME-driven, respectively), including Moreton, EIT, Hei 10830 , soft X-rayÅ waves, and type II radio bursts.”
Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, methodology): “Moreover, chromospheric Moreton waves were given the specific terminology flare waves (e.g. Zirin and Werner 1967; Warmuth et al. 2001; Warmuth et al. 2004a; Warmuth et al. 2004b).”