EIT Waves and Fast-Mode Propagation in the Solar Corona

By Y. Wang. 2000

193 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/64c1d9240ebed883b77e81867e4c25423db0c0d3

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Nat Gopalswamy
2. M. Temmer
3. B. Vršnak
4. A. Vourlidas
5. S. Yashiro
6. R. Howard
7. Valery M. Nakariakov
8. A. Zhukov

In Molecular Biology

1. Nat Gopalswamy
2. M. Temmer
3. L. Ofman
4. A. Zhukov
5. F. Auchère
6. A. Vourlidas
7. B. Vršnak
8. R. Howard

Citations in the corpus

• Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “The same approach was adopted in the modern observational context of EIT waves (Wang, 2000; Patsourakos et al., 2009).”
• 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).”
• Solar Phenomena Associated with “EIT Waves” (2002, methodology): “Moreton waves have been modeled by Uchida (1968, 1974) as a fast-mode MHD wave, and additional modeling has shown this description may work equally well or better for EIT waves (Wang 2000; Wu et al. 2001).”
• The Kinematics of a Globally Propagating Disturbance in the Solar Corona (2008, background): “Fast magnetoacoustic waves can reproduce the brightenings observed in EUV images as well as explaining some of the characteristics of EIT waves, including their slow expansion rates (Wang 2000).”
• Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “…that has permitted their discovery (Thompson et al. 1999), and were immediately interpreted as the manifestation of a fast-magnetoacoustic mode, i.e. a compressive wave propagating quasi-perpendicularly to the direction of the local magnetic field (e.g. Wang 2000; Ofman and Thompson 2002).”
• A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, methodology): “Several numerical simulations of EIT waves have been carried out showing that the assumption of a fast-mode MHD wave as the cause of EIT waves is reasonable (Wang 2000; Wu et al. 2001; Ofman & Thompson 2002).”
• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “…only the expanding flux tube, neglecting interaction with the surroundings (Delannée et al. 2008), simulated the interaction of coronal waves with only a local active region (Uchida 1974; Ofman & Thompson 2002), or they drove the coronal wave by a pressure pulse (Wang 2000; Wu et al. 2001).”
• On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “It should be stressed, however, that to account for the low EIT wave velocities both models (Wang 2000; Wu et al. 2001) had to adopt values of the coronal magnetic field resulting in high values of the plasma parameter beta (β > 1).”
• EUV WAVE REFLECTION FROM A CORONAL HOLE (2009, methodology): “This is confirmed by numerical simulations (Wang, 2000; Wu et al. 2001).”
• Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “…sound speed in the corona and the intrinsic characteristics of a fast-mode shock are capable of producing brightening in EUV images, authors such as Wang (2000), Ofman & Thompson (2002), Warmuth et al. (2004b, and references therein), and Ballai et al. (2005) endorse the interpretation of these…”
• Evidence of EIT and Moreton Waves in Numerical Simulations (2002, methodology): “Contrary to the model of Wang (2000) and Wu et al. (2001), which requires high-plasmab in the corona, only a small value ofb in our model can reproduce the observed velocities of EIT waves.”
• OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “…nature of the more common diffuse EUV waves is still being debated as to whether they are fastmode MHD waves (e.g., Wills-Davey & Thompson 1999; Wang 2000; Wu et al. 2001; Ofman & Thompson 2002; Schmidt & Ofman 2010), slow-mode MHD waves (Wang et al. 2009), or non-waves related to a current…”
• Evolution of Two EIT/Hα Moreton Waves (2001, background): “Both Mann et al. (1999; also discussed in Klassen et al. 2000) and Wang (2000) find fast-mode speeds of a few hundred kilometers per second in the low corona outside of active regions.”