Motion of Flare Footpoint Emission and Inferred Electric Field in Reconnecting Current Sheets
By J. Qiu, Jeongwoo Lee, D. Gary, Haimin Wang. 2002
191 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/1e4c5181976735dd2b6943206e5e6b61eaaa1440
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In Astronomy and Astrophysics
Citations in the corpus
- Slip-Running Reconnection in Quasi-Separatrix Layers (2006, background): “…those estimated at large scales during intense solar flares, using transversal flare ribbon motions (Poletto and Kopp, 1986; Forbes and Lin, 2000; Qiu et al., 2002), and even smaller than those required to accelerate particles to the observed range of energies (as modeled by e.g. Turkmani et…”
- On the Magnetic Flux Budget in Low-Corona Magnetic Reconnection and Interplanetary Coronal Mass Ejections (2007, background): “The magnetic reconnection rate has been inferred from flare observations by a number of research groups (Poletto & Kopp 1986; Isobe et al. 2002, 2005; Fletcher & Hudson 2001; Qiu et al. 2002, 2004; Fletcher et al. 2004; Qiu & Yurchyshyn 2005; Saba et al. 2006).”
- An Observational Overview of Solar Flares (2011, methodology): “…reconnection:The product of the footpoint apparent speed and the line-of-sight magnetic field, expressed asa flux transfer rateΦ̇ , has been used as a measure of the coronal reconnection rate by variousuthors (e.g., Qiu et al. 2002; Fletcher et al. 2004; Jing et al. 2005; Temmer et al. 2007).”
- Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18 (2005, background): “…indirectly by observing the dynamic behavior of the products of magnetic reconnection: the separating flare ribbons on the solar surface (Poletto & Kopp 1986; Qiu et al. 2002; Wang et al. 2003; Qiu et al. 2004), the growing flare loops in the corona (Sui & Holman 2003; Sui et al. 2004), and so on.”
- Magnetic Reconnection and Mass Acceleration in Flare-Coronal Mass Ejection Events (2004, background): “…of a bipolar arcade, the electric field inside the RCS can be inferred by measuring the expansion speed of the well-defined ribbon fronts and the magnetic fields that the ribbons sweep through (Forbes & Priest 1984; Forbes & Lin 2000; Poletto & Kopp 1986; Qiu et al. 2002; Wang et al. 2003).”