Origin and Evolution of Filament-Prominence Systems
By P. Martens, C. Zwaan. 2001
156 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/33b28fe738e32a26213ba06cb60f5de0d1bbba0c
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Citations in the corpus
- Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, methodology): “Therefore, in contrast to van Ballegooijen and Martens (1989) and Martens and Zwaan (2001), DeVore and Antiochos (2000) do not rely on convergence and cancellation of flux to produce the helical field.”
- QUIESCENT PROMINENCE DYNAMICS OBSERVED WITH THE HINODE SOLAR OPTICAL TELESCOPE. I. TURBULENT UPFLOW PLUMES (2010, background): “MHD and analytical models (Magara 2007; Aulanier et al. 1998, 2006; Welsch et al. 2005; Galsgaard & Longbottom 1999; Low & Hundhausen 1995; Martens & Zwaan 2001) have also been successful in replicating both static prominence structure as well as details such as the footpoint locations and observed…”
- Emergence of a Helical Flux Rope under an Active Region Prominence (2008, background): “…Low & Hundhausen 1995; Low 1996; Lites 2005; Zhang & Low 2005) and sheared-arcade models (e.g., Pneuman 1983; van Ballegooijen & Martens 1989, 1990; Antiochos et al. 1994; DeVore & Antiochos 2000; Martens & Zwaan 2001; Aulanier et al. 2002; Karpen et al. 2003; Mackay & van Ballegooijen 2005, 2006).”
- Hinode SOT Observations of Solar Quiescent Prominence Dynamics (2008, unknown): “Current models (Malherbe & Priest 1983; Low & Hundhausen 1995; Martens & Zwaan 2001; Aulanier et al. 2002; Karpen et al. 2006; Petrie et al. 2007) propose that prominences are formed by relatively low-b plasma trapped in locally horizontal magnetic field line “dips.””