Flux cancellation and coronal mass ejections

By Jon A. Linker, Zoran Mikic, Roberto Lionello, Pete Riley, Tahar Amari, D. Odstrcil. 2003

158 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a83399c1c32eb6cbb95efb4a5cb922f8cdab966a

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In Astronomy and Astrophysics

Citations in the corpus

The Partial Expulsion of a Magnetic Flux Rope (2006, background): “…a filament with its cavity into a socalled three-part CME is also consistent with a pre-CME flux rope (Wolfson et al. 1987; Low & Hundhausen 1995; Linker et al. 2003; Gibson et al. 2006), as are transient sigmoid brightenings (Rust & Kumar 1996; Fan & Gibson 2003, 2004; Kliem et al. 2004) and…”
The Heliospheric Magnetic Field (2013, methodology): “In principle, the MHD approach allows for a time-dependent inner boundary condition, though at present this involves an ad-hoc manipulation of the photospheric magnetic field and has only been possible for specific event studies (e.g., Linker et al., 2003).”
Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, background): “This phase of the breakout mechanism is the standard CHSKP flare reconnection (Carmichael 1964; Hirayama 1974; Sturrock 1968; Kopp & Pneuman 1976), which is common to all models of CME initiation (e.g., Linker et al. 2003; Forbes & Lin 2000; Roussev et al. 2004, 2007).”
The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “As an equilibrium state it is likely to be temporary, so that as conditions change within and around the flux rope, the equilibrium is eventually lost, and the rope expends its stored magnetic energy and erupts outward as a CME (Linker et al. 2003; Fan 2006).”
Adaptive numerical algorithms in space weather modeling (2012, methodology): “For example in the CISM framework the solar corona, the heliosphere and the magnetosphere are modeled by the MAS [10], the ENLIL [11] and the LFM [12] codes, respectively.”
The standard flare model in three dimensions - I. Strong-to-weak shear transition in post-flare loops (2012, methodology): “Several 2.5D MHD simulations for flares and CME early phases have calculated the magnetic and thermal properties of this standard model (e.g. Amari et al. 1996; Chen & Shibata 2000; Linker et al. 2003; Reeves & Forbes 2005; Shiota et al. 2005; Jacobs et al. 2006).”
The Physical Processes of CME/ICME Evolution (2017, background): “After this additional relaxation, the eruption of the flux rope was triggered by imposing sub-Alfvénic flows at the inner boundary that converge toward the PIL (e.g., Linker et al. 2003; Mikić et al. 2013b).”
Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “…mimicking the emergence of a subphotospheric flux rope, or as arising from a combination of photospheric shearing flows and the emergence or submergence of opposite polarities (which is equivalent to flux cancellation) [van Ballegooijen and Martens, 1999; Amari et al., 2000; Linker et al., 2003].”
Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18 (2005, methodology): “Of course, the configuration in Figure 1 could also be produced in the processes described by other CME models, such as the sheared-arcade and breakout models (Mikić et al. 1988; Mikić & Linker 1994; Antiochos et al. 1999; Amari et al. 2003; Linker et al. 2003).”