A multiwavelength study of solar flare waves. I. Observations and basic properties

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

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/41db08d1473ebf678576a9aa67d2b32371973559

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Citations in the corpus

A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, methodology): “In the previous paper of the series (Warmuth et al. 2004; henceforth Paper I) we have described morphological Send offprint requests to: A. Warmuth, e-mail: awarmuth@aip.de characteristics and kinematics of 12 flare waves, using imaging data from five spectral bands (Hα, EUV, helium I, SXR and…”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “Counterparts of EIT waves at other wavelengths have been imaged in soft X-rays (Narukage et al., 2002; Hudson et al., 2003) and microwave and metric radio bands (Warmuth et al., 2004; White and Thompson, 2005; Vršnak et al., 2005).”
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.”
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.”
The Kinematics of a Globally Propagating Disturbance in the Solar Corona (2008, methodology): “In contrast, Moreton waves are observed to be strongly defined, narrow semi-circular fronts (Warmuth et al. 2004a).”
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).”
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.”