Dynamical and Physical Properties of a Post-Coronal Mass Ejection Current Sheet
By Y. Ko, J. C. Raymond, Jun Lin, G. Lawrence, Jing Li, A. Fludra. 2003
206 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/d2603abd62cfdef795f8f063a4c19e4eb2d0f928
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In Astronomy and Astrophysics
- V. Petrosian
- J. C. Raymond
- Wei Liu
- Guillermo Stenborg
- E. P. Kontar
- A. A. Ballegooijen
- Y. Ko
- Qingrong Chen
Citations in the corpus
- Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18 (2005, background): “…Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO) together with other remote-sensing data, Ciaravella et al. (2002) and Ko et al. (2003) have conducted comprehensive analyses of various aspects of several eruptive processes that clearly manifested both coronal mass…”
- AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT? (2008, background): “Ample observational and numerical evidence proves their existence and dynamics observed as bursty outflow (e.g. Ko et al. 2003; Webb et al. 2003; Riley et al. 2007; Ciaravella et al. 2002; Bemporad et al. 2006, and references therein).”
- Evidence for the Formation of a Large-Scale Current Sheet in a Solar Flare (2003, background): “There is some further observational evi- 1 Department of Physics, Catholic University of America, 620 Michigan Avenue, Washington, DC 20064. dence of current sheets associated with CMEs (Webb et al. 2003; Ciaravella et al. 2002; Ko et al. 2003).”
- The Role of Magnetic Reconnection in the Observable Features of Solar Eruptions (2004, background): “…details of CME processes in a realistic plasma environment, and the results regarding the dynamic behavior of the current sheet are fairly consistent with observations (see Švestka 1996; Švestka et al. 1997; Švestka & Fárnı́k 1998; Ciaravella et al. 2002; Ko et al. 2003; and Webb et al. 2003).”
- Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares (2011, background): “In this direction, TRACE and SOHO/LASCO1 C2 images reveal dynamically evolving magnetoplasma structures in an erupting arcade (Aurass et al. 2006).”
- PLASMOID EJECTIONS AND LOOP CONTRACTIONS IN AN ERUPTIVE M7.7 SOLAR FLARE: EVIDENCE OF PARTICLE ACCELERATION AND HEATING IN MAGNETIC RECONNECTION OUTFLOWS (2013, background): “…revealed bi-directional magnetic reconnection inflows (Yokoyama et al. 2001; Milligan et al. 2010; Liu et al. 2010), outflows (Innes et al. 1997; Ko et al. 2003; Wang et al. 2007; Nishizuka et al. 2010; Hara et al. 2011; Watanabe et al. 2012), or both (Lin et al. 2005; Takasao et al. 2012;…”