Origin of Coronal Shock Waves
223 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/5208a25d2aea4f8578cb24acca4ade90f2ce233c
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In Astronomy and Astrophysics
Citations in the corpus
- Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, methodology): “E.g. Chen et al. (2002) replace the blast wave (initiated by the solar-flare pressure pulse) by a piston-driven shock wave from a CME (see Vršnak and Cliver 2008 and §2.2 of Warmuth 2015 for further details).”
- COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “…the large-scale CME acceleration and the energy release process in the associated flare (e.g. Lin 2004; Maričić et al. 2007; Temmer et al. 2008; Vršnak & Cliver 2008): After the magnetic structure looses equilibrium and starts rising, a current sheet is formed below the rising structure…”
- OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, methodology): “For detailed discussions of the different models and supporting observations, we refer to the recent reviews by Warmuth (2007, 2010); Vršnak & Cliver (2008); Wills-Davey & Attrill (2009), and Gallagher & Long (2010).”
- Space weather: the solar perspective (2021, background): “More details are found in, e.g., Chen and Krall (2003), Vršnak et al. (2007), Vršnak (2008), Jang et al. (2017).”
- Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…and Zhukov (2011) for updates with early STEREO observations, to Patsourakos and Vourlidas (2012) for a synthesized view from SOHO, STEREO, Hinode, and SDO in its first year of operation, and to Vršnak and Cliver (2008) and Chen (2011) for related subjects of coronal shocks and CMEs, respectively.”
- An Observational Overview of Solar Flares (2011, background): “The following recent reviews of observations of flare and related phenomena, including theory, are also recommended for further reading: Priest & Forbes (2002); Aschwanden (2002); Benz (2008); Krucker et al. (2008a); Vršnak & Cliver (2008); Schrijver (2009).”
- NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “In these models, the wave front may be freely propagating (generated by an initial pressure pulse), or piston-driven where the wave is constantly supplied by energy from the expanding CME (e.g. Vršnak & Cliver 2008).”
- Solar Orbiter (2012, background): “Shocks in the lower corona can also be driven by flares, and in the case of CME/eruptive flare events it may be difficult to unambiguously identify the driver (Vršnak and Cliver, 2008).”