Onset of the Magnetic Explosion in Solar Flares and Coronal Mass Ejections

By R. Moore, A. Sterling, H. Hudson, J. Lemen. 2001

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In Astronomy and Astrophysics

Citations in the corpus

Numerical Simulations of Three-dimensional Coronal Magnetic Fields Resulting from the Emergence of Twisted Magnetic Flux Tubes (2004, background): “Several observations have found transient brightening and sharpening of X-ray sigmoids during the onset of eruptive flares and coronal mass ejections (e.g., Sterling & Hudson 1997; Moore et al. 2001).”
MAGNETIC FIELD STRUCTURES TRIGGERING SOLAR FLARES AND CORONAL MASS EJECTIONS (2012, background): “These results are consistent with the observations of internal reconnection (Moore et al. 2001).”
RESPONSE OF THE PHOTOSPHERIC MAGNETIC FIELD TO THE X2.2 FLARE ON 2011 FEBRUARY 15 (2011, background): “We suggest that the tether-cutting reconnection (Moore et al. 2001) between the loops FP3–FP2 and FP4–FP1 produces the short and low-lying loops FP1–FP2, which could explain the enhanced Bh as well as S̃ and S̊ at the region R (Melrose 1997).”
Homologous Confined Filament Eruptions via Magnetic Breakout (2008, background): “Observational studies of confined (or ‘‘failed’’) eruptions have shown that their only certain signature is the absence of an associated coronalmass ejection (Moore et al. 2001; Choudhary & Moore 2003).”
A Global Picture of CMEs in the Inner Heliosphere (2004, background): “This could be a simple bipole with a core-envelope structure (Moore et al., 2001; Ma- 32 gara 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…”
COEXISTING FLUX ROPE AND DIPPED ARCADE SECTIONS ALONG ONE SOLAR FILAMENT (2010, background): “…at the onset of, an eruption (e.g., Forbes & Isenberg 1991; Török & Kliem 2005; Fan & Gibson 2007), whereas others assume that the preeruptive configuration is that of an arcade, and that a flux rope is formed later on, during the eruption process (e.g., Antiochos et al. 1999; Moore et al. 2001).”
Particle acceleration and kinematics in solar flares – A Synthesis of Recent Observations and Theoretical Concepts (Invited Review) (2002, methodology): “…Hudson, and McKenzie 1999, 6) Van Ballegooijen and Martens 1989, Moore and Roumeliotis 1992, Canfield et al. 1994, Canfield and Reardon 1998, Moore et al. 2001, 7) Antiochos 1998, Antiochos, DeVore, and Klimchuk 1999, Aulanier et al. 2000, 8) Yokoyama et al. 2001, Blackman 1997. release…”
The standard flare model in three dimensions - I. Strong-to-weak shear transition in post-flare loops (2012, methodology): “Thus, the three-dimensional geometry of the early flare reconnection fits the cartoon of the so-called tethercutting model by Moore et al. (2001).”
TIME-RESOLVED PROPERTIES AND GLOBAL TRENDS IN dMe FLARES FROM SIMULTANEOUS PHOTOMETRY AND SPECTRA (2013, background): “Possible scenarios are an unstable flux rope that erupts sequentially along a flare arcade (the “tether-cutting scenario” Moore et al. 2001) and magnetoacoustic slow waves that propagate away from the initial flare site (Nakariakov & Zimovets 2011).”
Plasma Beta above a Solar Active Region: Rethinking the Paradigm (2001, background): “These SXT cusps are interpreted within the standard magnetic eruption models to represent reconnection sites as a current sheet with open field lines above the cusp (e.g., Moore et al., 2001; Yokoyama et al., 2001; McKenzie and Hudson, 1999).”
The Interaction of Successive Coronal Mass Ejections: A Review (2016, methodology): “The tether-cutting model (Moore et al., 2001) and magnetic breakout model (Antiochos, DeVore, and Klimchuk, 1999) are both of this type.”
Photospheric flux cancellation and associated flux rope formation and eruption (2010, background): “In a small number of cases, the eruption from a sigmoidal active region has been observed as the rise of a faint, nearly linear feature in the soft X-ray emission, suggested to be formed near the magnetic axis of a flux rope (Moore et al. 2001; McKenzie & Canfield 2008).”
Solar filament eruptions and their physical role in triggering Coronal Mass Ejections (2012, background): “, 2008), reconnection of field lines below the flux rope (the tether-cutting model, Moore and Roumeliotis, 1992; Moore et al., 2001), or reconnection above the flux rope (the breakout model, Antiochos et al.”