THE HYDROMAGNETIC NATURE OF SOLAR CORONAL MASS EJECTIONS
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Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/611f9b0c266cceeb06110f8c9b7363af5e43b9f4
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In Astronomy and Astrophysics
Citations in the corpus
- Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “Thus coronal fields will naturally produce a flux rope, rather than a potential field, as a metastable state (see, e.g., review by Zhang and Low [2005] ).”
- Emergence of a Helical Flux Rope under an Active Region Prominence (2008, background): “Two theories have been discussed: flux rope models (e.g., Rust & Kumar 1994; 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;…”