Coronal Mass Ejection: Initiation, Magnetic Helicity, and Flux Ropes. I. Boundary Motion-driven Evolution

By Tahar Amari, J. Luciani, J. Aly, Z. Mikić, Jon A. Linker. 2003

275 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/6ed1e364e899d858d95c7d845c212246a6aa59c3

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. G. Aulanier
2. P. Démoulin
3. Brigitte Schmieder
4. S. Gibson
5. Yuhong Fan
6. Tibor Török
7. P. Schuck
8. M. Janvier

In Molecular Biology

1. G. Aulanier
2. P. Démoulin
3. S. Gibson
4. P. Schuck
5. Yuhong Fan
6. Tibor Török
7. Brigitte Schmieder
8. B. Kliem

Citations in the corpus

• The standard flare model in three dimensions - III. Slip-running reconnection properties (2013, background): “S R ] 1 7 M ay 2 01 3 flux ropes (Shibata et al. 1995; Shiota et al. 2005; Priest & Forbes 2002; Amari et al. 2003a,b), and unstable flux ropes (Török et al. 2004; Aulanier et al. 2010).”
• The Role of Magnetic Reconnection in the Observable Features of Solar Eruptions (2004, methodology): “Other models (e.g., Mikić, Barnes, & Schnack 1988; Mikić & Linker 1994; Antiochos, DeVore, & Klimchuk 1999; Amari et al. 2003; Manchester 2003) begin with a sheared magnetic structure that becomes unstable as a result of reconnection (Gosling 1993).”
• The Partial Expulsion of a Magnetic Flux Rope (2006, background): “…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 their transition to cusped postflare loops (Amari et al. 2003b; To¨rök & Kliem 2005).”
• Confined and Ejective Eruptions of Kink-unstable Flux Ropes (2005, methodology): “They also demonstrate the importance of the height dependence of the overlying field for the evolution of the instability into a CME, while Amari et al. (2003b) found the amount of magnetic helicity to be essential.”
• ELECTRIC CURRENTS IN FLARE RIBBONS: OBSERVATIONS AND THREE-DIMENSIONAL STANDARD MODEL (2014, methodology): “As such, different mechanisms for eruptive flares have been proposed (see Forbes et al. 2006; Amari et al. 2003a, 2003b; Shibata & Magara 2011; Aulanier 2014 and references therein).”
• OBSERVING FLUX ROPE FORMATION DURING THE IMPULSIVE PHASE OF A SOLAR ERUPTION (2011, background): “Considerable efforts have also been made in numerical MHD simulations to study the formation and dynamic behavior of flux ropes (Amari et al. 2000, 2003; Aulanier et al. 2010; Fan & Gibson 2003, 2004).”
• MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS (2012, background): “In fact, the converging flow on the solar surface is believed to play the role of a trigger in the flux cancellation (FC) model (Inhester et al. 1992; Priest et al. 1994; Amari et al. 2003a).”
• 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).”
• The Origin, Early Evolution and Predictability of Solar Eruptions (2018, background): “Many examples exist including simulations by Steinolfson (1991); Mikic and Linker (1994); Wolfson (1995); Antiochos et al (1999); Amari et al (2003a); Lynch et al (2008); van der Holst et al (2009), which are successful in reproducing many characteristics of CMEs, filament eruptions and flares.”
• Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “D twisted flux rope configurations have also been shown in numerical simulations [Linker et al., 2001; Amari et al., 2000, 2003a, 2004a, 2004b; Toeroek and Kliem, 2003; Kusano et al., 2004; Roussev et al., 2004; Kusano, 2005; Fan, 2005; Toeroek and Kliem, 2005; Fan and Gibson, 2006; Gibson and Fan,…”
• The Physical Processes of CME/ICME Evolution (2017, unknown): “The pre-event magnetic field supporting the filament can also be well described by highly sheared magnetic arcades crossing the PIL (e.g., Mikić et al. 1988; Steinolfson 1991; Antiochos et al. 1999; Amari et al. 2003; Manchester 2003; Lynch et al. 2008; van der Holst et al. 2009).”
• Tracking Vector Magnetograms with the Magnetic Induction Equation (2008, background): “…flux cancellation of the overlying coronal field (Linker et al. 2001), flux injection (Chen 1989, 1996), the kink instability of filaments (Rust & Kumar 1996; Török et al. 2004; Kliem et al. 2004), and photospheric footpoint shearing (Amari et al. 2000, 2003a, 2003b; Schrijver et al. 2005).”
• The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “However, the question of whether the flux rope is formed during the eruption or whether the flux rope existed prior to the eruption remains controversial (Amari et al. 2003).”