A review on the genesis of coronal mass ejections

By T. Forbes. 2000

576 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/ebf82422e143342cebebbd2d1f9c572d5491d9e6

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In Astronomy and Astrophysics

1. M. Temmer
2. G. Aulanier
3. Nat Gopalswamy
4. A. Vourlidas
5. P. Démoulin
6. B. Vršnak
7. W. Manchester IV
8. Yuhong Fan

In Molecular Biology

1. G. Aulanier
2. S. Gibson
3. P. Démoulin
4. Yuhong Fan
5. M. Temmer
6. Nat Gopalswamy
7. Tibor Török
8. T. Wiegelmann

Citations in the corpus

• The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “A range of models have demonstrated how CMEs can arise from an initial flux rope configuration (see, e.g., Forbes 2000 and references therein).”
• Coronal mass ejections, magnetic flux ropes, and solar magnetism (2001, unknown): “…MacQueen et al., 2001; Fisher, 1984; Howard et al., 1985, 1997; Hund-hausen, 1987, 1993, 1999; Hundhausen, Burkepile, and St. Cyr, 1994; Low, 1990, 1996; Kahler, 1992; Burkepile and St. Cyr, 1993; St. Cyr et al., 1999; St. Cyr et al., 2000; Crooker et al., 1997; Dere et al., 1999; Forbes, 2000].”
• A Three-dimensional Flux Rope Model for Coronal Mass Ejections Based on a Loss of Equilibrium (2003, methodology): “As seen in Figure 2, the slope of the speed curve for the O-point is initially shallow, just as expected for a loss of equilibrium (Lin & Forbes 2000).”
• The Role of Magnetic Reconnection in the Observable Features of Solar Eruptions (2004, methodology): “For B0 ¼ 100 G, at the time when h ¼ l ¼ L, Ĩ is given by equation (18) of Lin & Forbes (2000), and we find that Ĩ ¼ 0:92.”
• A Global Picture of CMEs in the Inner Heliosphere (2004, background): “The current level of sophistication of CME models is less than adequate to account for all the observed characteristics (see e.g., Forbes, 2000; Klimchuk, 2000).”
• On the probability of occurrence of extreme space weather events (2012, background): “The initiation of coronal mass ejections, for example, may occur through flux cancelation, “break out,” the kink instability, flux emergence, or some other mechanism [Forbes, 2000], each of which could produce CMEs with different distributions of speeds.”
• Elemental Abundances and Post-Coronal Mass Ejection Current Sheet in a Very Hot Active Region (2002, methodology): “As Lin & Forbes (2000) give the most detailed treatment of the flux rope, we compare the UVCS observations with their models.”
• Global Forces in Eruptive Solar Flares: The Lorentz Force Acting on the Solar Atmosphere and the Solar Interior (2010, background): “First, from energetic considerations, the magnetic field is believed to be the source of energy for eruptive flares and coronal mass ejections: Forbes (2000) and Hudson (2007) SOLA: SOLA1560R2_Fisher.tex; 6 December 2011; 2:56; p. 5 have argued that no other known source of energy can provide the…”
• Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, methodology): “55 from (Schwenn et al. 2006a) and derived from the model of Lin and Forbes (2000).”
• Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts (2008, background): “In the “standard” model, the erupting filament or CME stretches the coronal magnetic field lines to build up a vertical current sheet where magnetic reconnection sets in and releases vast amounts of energy (e.g., Forbes 2000).”
• MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS (2012, background): “…observations suggested that these properties tend to correlate with the solar eruption productivity, the triggering mechanism for solar eruptions is still debated (Forbes 2000), and we do not yet well understand what determines the onset of solar eruptions (Leka & Barnes 2007; Welsch et al. 2011).”
• Homologous Confined Filament Eruptions via Magnetic Breakout (2008, background): “A number of theories have been developed to account for solar eruptions (for reviews, see Forbes 2000; Klimchuk 2001; Lin et al. 2003; Forbes et al. 2006; Mikić & Lee 2006).”
• The Partial Expulsion of a Magnetic Flux Rope (2006, methodology): “INTRODUCTION Magnetic flux rope models are often used to describe coronal mass ejections (CMEs) in eruption (Forbes 2000).”
• The Origin, Early Evolution and Predictability of Solar Eruptions (2018, background): “…from strongly non-potential fields where the photospheric magnetic field is nearly parallel to the polarity inversion line (PIL), a so called magnetic shear (e.g. Forbes, 2000; Schrijver, 2009), which stands in contrast to a potential field that runs perpendicular to the PIL and has no free energy.”
• DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE (2012, background): “Mechanical loss of equilibrium of a flux rope once it reaches a critical height (e.g., Forbes & Isenberg 1991; Forbes 2000; Vršnak 2008) is another possible trigger for the observed eruption.”
• On the three-dimensional configuration of coronal mass ejections (2004, background): “…in the low corona before its eruption will suffer an enormous expansion once it is triggered to lift off (see theories on CME initiation in e.g. Forbes 2000) as supported by the often directly visible self-similarity of the magnetic features in the studied events, as seen in the low corona and…”