An Emerging Flux Trigger Mechanism for Coronal Mass Ejections

By P. Chen, Kazunari Shibata. 2000

466 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b44b8ca8de0c39502ee89c8e594de27ece099509

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. M. Temmer
2. G. Aulanier
3. Brigitte Schmieder
4. Nat Gopalswamy
5. J. Zhang
6. M. Janvier
7. P. Chen
8. Xin Cheng

In Molecular Biology

1. G. Aulanier
2. Brigitte Schmieder
3. Nat Gopalswamy
4. M. Janvier
5. J. Zhang
6. A. Sterling
7. R. Moore
8. Xin Cheng

Citations in the corpus

• Solar Flares: Magnetohydrodynamic Processes (2011, background): “Figure 39: Destabilizing mechanism for the eruption of a flux rope, known as the emerging flux trigger mechanism presented in Chen and Shibata (2000). The solid lines correspond to the magnetic field, the arrows to the velocity, and the color map to the temperature.”
• DIFFERENTIAL EMISSION MEASURE ANALYSIS OF MULTIPLE STRUCTURAL COMPONENTS OF CORONAL MASS EJECTIONS IN THE INNER CORONA (2012, methodology): “…that the hot channel plays in the eruption process appears similar to that of flux ropes in the modeling and simulations of CMEs (e.g., Chen 1996; Chen & Shibata 2000; Lin & Forbes 2000; Török & Kliem 2005; Kliem & Török 2006; Aulanier et al. 2010; Fan & Gibson 2007; Fan 2010; Olmedo & Zhang…”
• Observations of the Failed Eruption of a Filament (2003, background): “The eruption may be caused by slow reduction of the overlying flux (Forbes & Priest 1995; Priest & Forbes 1990), by loss of equilibrium by reconnection beneath the filament (Chen & Shibata 2000) or viscous relaxation (Amari et al. 2000).”
• 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).”
• MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS (2012, background): “…of magnetic field (Schrijver 2007), emerging magnetic fluxes (Heyvaerts, Priest & Rust 1977; Moore & Roumeliotis 1992; Feynman & Martin 1995; Chen & Shibata 2000; Fan & Gibson 2004; Chifor, et al. 2007; Wallace et al. 2010; Moore et al. 2011; Archontis & Hood 2012), multipolar topologies…”
• Evidence of EIT and Moreton Waves in Numerical Simulations (2002, background): “Also, the inferred starting time of the EIT wave, extrapolated from the later evolution back to the flare site, would be earlier than the CME onset since its velocity is larger near the flare site than farther away, as shown in Figure 2.”
• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…free energy as well as helicity can be accumulated gradually via various ways, e.g., flux emergence (see, e.g. Heyvaerts, Priest, and Rust, 1977, Chen and Shibata, 2000), shearing/rotational motion (see, e.g., Manchester, 2003, Brown et al., 2003, Kusano et al., 2004, Zhang, Liu, and Zhang,…”
• Slow-Rise and Fast-Rise Phases of an Erupting Solar Filament, and Flare Emission Onset (2005, methodology): “We can compare our filament rise trajectory of Figure 8 with the rise trajectory calculated for an erupting flux rope in the model of Chen & Shibata (2000) shown in Figure 9.”
• The Magnetic Connection between the Convection Zone and Corona in the Quiet Sun (2007, unknown): “Admittedly, our numerical resolution could be improved around current sheets, and we have yet to experiment with more sophisticated, depth-dependent or current-dependent coefficients of magnetic resistivity (see, e.g., Chen & Shibata 2000; Otto 2001).”
• A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections (2006, background): “These models usually show a transition from slow to fast motion of the erupting magnetic structure (Mikic & Linker 1994; Lin & Forbes 2000; Chen & Shibata 2000; MacNeice et al. 2004).”
• A Global Picture of CMEs in the Inner Heliosphere (2004, background): “…and Longcope, 2001), a flux rope with overlying restraining field (Low and Zhang, 2002; Forbes et al., 1994; Linker et al., 2001; Wu et al., 2000), a combination of bipoles (Machado et al., 1988) or multipolar structure (Antiochus et al., 1999; Chen and Shibata, 2000; Feynman and Martin, 1995).”