Evidence of EIT and Moreton Waves in Numerical Simulations

By P. Chen, S. Wu, Kazunari Shibata, Cheng Fang. 2002

283 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/9128ab46c7cc7c25ff1cb7bba8a1bfdf29cad3a5

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In Astronomy and Astrophysics

Citations in the corpus

The Kinematics of a Globally Propagating Disturbance in the Solar Corona (2008, background): “The net result is that EIT waves are not real “waves”, but are the propagation of perturbation sources due to a CME lift-off (Delannée & Aulanier 1999; Chen et al. 2002, 2005).”
OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “…2001; Ofman & Thompson 2002; Schmidt & Ofman 2010), slow-mode MHD waves (Wang et al. 2009), or non-waves related to a current shell or successive restructuring of field lines during the coronal mass ejection (CME; Delannée 2000; Delannée et al. 2008; Chen et al. 2002, 2005; Attrill et al. 2007).”
Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, methodology): “The mechanism described by Chen et al. (2002, 2005) takes into account the propagation of stretching of magnetic field lines in a dipolar region due to the expansion of a CME.”
NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, methodology): “Chen et al. (2002, 2005) showed that stretching of the overlying magnetic field leads to compression of plasma in the legs of the CME, producing an intensity enhancement.”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…2DMHDmodels of EIT waves in Cartesian geometries, although simple, were able to capture some essential features, such as the bimodal composition of a fast-mode (shock) wave ahead of a CME driven compression (Chen et al., 2002; Chen, Fang, and Shibata, 2005; Pomoell, Vainio, and Kissmann, 2008).”
A multiwavelength study of solar flare waves. I. Observations and basic properties (2004, background): “Indeed, there have been claims that Moreton and EIT waves are distinct phenomena (Eto et al. 2002; Chen et al. 2002).”
On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “The bright front appears due to the plasma compression in the process of successive opening of magnetic field lines during the CME lift-off (Delannée & Aulanier 1999; Chen et al. 2002).”
Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, methodology): “This review focuses on QPPs, but other types of waves and pulsations associated with solar and stellar flares are discussed briefly in the appendices, where Appendix A considers global waves generated by CMEs and flares (including shock waves, blast waves, EIT waves, Moreton waves and ‘flare waves’)”
Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “Our model does not require a preexisting giant bipolar arcade to span the diameter of the observed coronal wave (as in Chen et al. 2002), since this is naturally created by the displacement of the expanding CME footpoints, through the successive small-scale reconnection events between the erupting…”
A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, methodology): “In some recent models (Delannée 2000; Chen et al. 2002), the CMEs themselves are identified as the driver of the waves, so in these views the term “flare wave” would actually be a misnomer.”