Interaction of EIT Waves with Coronal Active Regions

By L. Ofman, Barbara J. Thompson. 2001

167 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/6a26bead4b4f17d75a0d30f2e7eb117375d6ca21

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In Astronomy and Astrophysics

Citations in the corpus

Waves in the Magnetized Solar Atmosphere. II. Waves from Localized Sources in Magnetic Flux Concentrations (2003, background): “Fully three-dimensional problems are tackled by Wu et al. (2001) and Ofman & Thompson (2002).”
EUV WAVE REFLECTION FROM A CORONAL HOLE (2009, background): “Stopping of EUV waves by an active region has also been reported by Ofman and Thompson (2002).”
A multiwavelength study of solar flare waves II. Perturbation characteristics and physical interpretation (2004, background): “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).”
OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “…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 shell or successive…”
Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review) (2014, unknown): “…result from persistent heating and/or compression produced by wave or non-wave mechanisms, such as localized energy release 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…”
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).”
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).”
Coronal “Wave”: Magnetic Footprint of a Coronal Mass Ejection? (2007, unknown): “…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 phenomena as…”
The Kinematics of a Globally Propagating Disturbance in the Solar Corona (2008, methodology): “This interpretation has been used to create numerical simulations which closely imitate the observed data (Wu et al. 2001; Ofman & Thompson 2002; Ofman 2007).”
Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, background): “Such perturbations can be external to a loop system (e.g. Ofman and Thompson 2002; McLaughlin and Ofman 2008) or internal to a loop system.”
Line-of-sight effects on observability of kink and sausage modes in coronal structures with imaging telescopes (2002, unknown): “Fast magnetoacoustic waves are possibly responsible for events such as coronal Moreton (or EIT) waves (Thompson et al. 1998; Ofman & Thompson 2002).”
Hinode observations of transverse waves with flows in coronal loops (2008, methodology): “…was applied to TRACE and SOHO data (e.g., Nakariakov et al. 1999; Nakariakov & Ofman 2001; Ofman 2002; De Moortel et al. 2002; Ofman & Wang 2002; Ofman & Thompson 2002; Verwichte et al. 2004; Wang & Solanki 2004; Aschwanden 2005), with recent advances (e.g., Ofman 2007; Wang et al. 2007; Van…”