A MODEL FOR SOLAR POLAR JETS
By Etienne Pariat, S. Antiochos, C. R. DeVore. 2009
285 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/26e71451f3037767cb8db0b62a64b1b348b80899
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In Astronomy and Astrophysics
Citations in the corpus
- THE NATURE OF FLARE RIBBONS IN CORONAL NULL-POINT TOPOLOGY (2009, methodology): “In each domain a spine is present, which we refer to the inner (resp. outer) spine for the one confined below (resp. emerging away from) the fan surface (as in Figure 1 of Pariat et al. 2009).”
- A MODEL FOR MAGNETICALLY COUPLED SYMPATHETIC ERUPTIONS (2011, background): “…a sympathetic eruption by R1 requires the presence of a separator (or null point) above closed flux that stabilizes a pre-eruptive flux rope, which can be realized, in the simplest case, in a so-called “fan-spine” configuration (e.g., Antiochos 1998; Pariat et al. 2009; Török et al. 2009).”
- ON A CORONAL BLOWOUT JET: THE FIRST OBSERVATION OF A SIMULTANEOUSLY PRODUCED BUBBLE-LIKE CME AND A JET-LIKE CME IN A SOLAR EVENT (2011, methodology): “Numerical simulations of the blowout of the twisted jet core field by the breakout reconnection with ambient fields were also conducted (Pariat et al. 2009; Rachmeler et al. 2010).”
- Three-dimensional magnetic reconnection regimes: a review (2011, background): “3D null point reconnection, via the spine-fan reconnection mode, has been proposed as a mechanism for polar jets (Pariat et al., 2009) as well as for CMEs via the ‘magnetic breakout’ model (Antiochos et al., 1999; Lynch et al., 2008).”
- CIRCULAR RIBBON FLARES AND HOMOLOGOUS JETS (2012, methodology): “By flipping the outer spine field lines in M09 to open outward, one could arrive at an ax- isymmetrical null-point and fan-spine topology (see Figure 1), which Pariat et al. (2009) used to model solar polar jets.”
- THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS (2010, background): “1762 Recently, we (Pariat et al. 2009, hereafter PAD09) reported 3D numerical simulations demonstrating that impulsive 3D reconnection at a null point can generate a nonlinear Alfvénic wave, which transfers away the stored magnetic energy and helicity along reconnected field lines.”
- How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs (2012, methodology): “JetCMEs also contain helical structures as recent research has shown (Patsourakos et al., 2008; Pariat, Antiochos, and DeVore, 2009; Nisticò et al., 2010).”
- Characteristics of EUV Coronal Jets Observed with STEREO/SECCHI (2009, background): “It is usually assumed that the jet is the result of magnetic reconnection phenomena happening in the solar corona (Shibata et al., 1992; Yokoyama and Shibata, 1995; Yokoyama and Shibata, 1996; Moreno-Insertis, Galsgard, and Ugarte-Urra, 2008; Pariat, Antiochos, and DeVore, 2009).”