Evolution of Two EIT/Hα Moreton Waves

By A. Warmuth, B. Vršnak, H. Aurass, A. Hanslmeier. 2001

161 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/113927381c79570cb70f283c44e24ad266a4c2b6

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Citations in the corpus

On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “It was shown (Warmuth et al. 2001, 2002, 2004a) that although EIT and Moreton wave fronts have different speeds, they lie on the same kinematic curves (if the curves are approximated by a parabolic fit).”
Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “…bright front (Biesecker et al. 2002), often high velocity (greater than several hundred kilometers per second) and sometimes cospatial with a Moreton wave (Thompson et al. 2000b; Warmuth et al. 2001; Khan & Aurass 2002) and those with a more diffuse bright front (e.g., Thompson et al. 1998, 1999).”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “Wave models interpret EIT waves as true waves, most likely fast-mode magnetosonic waves (Thompson et al., 1999; Wang, 2000; Wu et al., 2001; Warmuth et al., 2001; Ofman and Thompson, 2002).”
EUV WAVE REFLECTION FROM A CORONAL HOLE (2009, background): “EUV waves with metric type II radio bursts are also associated with Hα Moreton waves (Smith and Harvey 1971), which are assumed to be the chromospheric counterparts of the EUV waves (Thompson et al. 1999, Warmuth et al. 2001, Veronig et al. 2006).”
A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, result): “Furthermore, all flare waves are decelerating, which confirms the results obtained by Warmuth et al. (2001).”
A multiwavelength study of solar flare waves. I. Observations and basic properties (2004, background): “This allows us to check the conclusions reached in Warmuth et al. (2001) and derive more convincing and extensive results.”
Interaction of EIT Waves with Coronal Active Regions (2001, methodology): “EIT waves were interpreted as fast magnetosonic waves (Wang 2000; Murawski, Nakariakov, & Pelinovsky 2001; Warmuth et al. 2001) and associated with Moreton waves observed in the photosphere (Moreton 1961).”
Evidence of EIT and Moreton Waves in Numerical Simulations (2002, background): “This may have been observed by Warmuth et al. (2001), although the temporal resolution ofSOHO/EIT (∼15 minutes) is not sufficiently high.”
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).”