Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection?
By G. Attrill, L. Harra, L. van Driel-Gesztelyi, P. Démoulin. 2007
211 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/d227636c2a7a2592f0de7498822b021640b6cf47
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In Astronomy and Astrophysics
- Nat Gopalswamy
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Citations in the corpus
- 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).”
- Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…triggered by MHD waves (Ofman and Thompson, 2002; Terradas and Ofman, 2004), opening of magnetic-field lines (Delannée, 2000; Chen, Fang, and Shibata, 2005), Joule heating in current sheets (Delannée, Hochedez, and Aulanier, 2007), and continual magnetic reconnection (Attrill et al., 2007).”
- Magnetohydrodynamic Oscillations in the Solar Corona and Earth’s Magnetosphere: Towards Consolidated Understanding (2016, background): “…of the coronal plasma at the surface of the expanding CME flux-rope (Delannée and Aulanier 1999), or due to the result of progressing magnetic restructuring via a series of reconnections between the magnetic field lines of the CME flux-rope and the quiet-Sun region (Attrill et al. 2007).”
- EUV WAVE REFLECTION FROM A CORONAL HOLE (2009, background): “Attrill et al. (2007) propose that successive flare-like brightenings due to the interaction of CME flux rope with low-lying coronal loops might be seen as the EUV transients.”
- NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “Attrill et al. (2007a) suggested that magnetic reconnections between the expanding CME and favorably oriented surrounding quiet Sun magnetic field drive weak flare-like brightenings making up the bright front.”