Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18

By J. Lin, Y. Ko, L. Sui, J. C. Raymond, Guillermo Stenborg, Y. Jiang, S. Mancuso. 2005

297 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/9e5147a546385d78259255bac9a35f10c530e053

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

Citations in the corpus

RECONNECTION OUTFLOWS AND CURRENT SHEET OBSERVED WITH HINODE/XRT IN THE 2008 APRIL 9 “CARTWHEEL CME” FLARE (2010, background): “Outflow pairs much higher in the corona have been previously observed primarily with LASCO (see for example Sheeley & Wang 2007, Lin et al. 2005, and Sheeley, Warren, & Wang 2004).”
Magnetic Reconnection in Astrophysical and (2009, background): “From Lin et al. (2005). an energy of 1031–1032 ergs is released into fast particles over the duration of a large flare.”
Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares (2011, background): “…et al. 2003), the Large Angle and Spectrometric Coronagraph (LASCO) and the Ultraviolet Coronagraph Spectrometer (UVCS) on SOHO (Ko et al. 2003; Lin et al. 2005), RHESSI (Sui et al. 2005b), and TRACE (Sui et al. 2006a) have all provided direct evidence for the presence of an extended, vertical…”
PLASMOID EJECTIONS AND LOOP CONTRACTIONS IN AN ERUPTIVE M7.7 SOLAR FLARE: EVIDENCE OF PARTICLE ACCELERATION AND HEATING IN MAGNETIC RECONNECTION OUTFLOWS (2013, background): “…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; Savage et al. 2012).”
SIMULTANEOUS OBSERVATION OF RECONNECTION INFLOW AND OUTFLOW ASSOCIATED WITH THE 2010 AUGUST 18 SOLAR FLARE (2011, background): “Spectroscopic observation of reconnection region is necessary to quantitatively address the flow velocity (Lin et al. 2005; Hara et al. 2006; Wang et al. 2007).”
Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet (2018, background): “…sheet are mostly limited by the wavelength window that only responds to relatively narrow and low temperatures and/or the field of view that is not large enough (Lin et al. 2005, 2009; Ciaravella et al. 2003; Ciaravella & Raymond 2008; Savage et al. 2010; Ling et al. 2014; Seaton et al. 2017).”
Reconnection-driven plasmoids in blazars: fast flares on a slow envelope (2012, background): “Besides the global reconnection timescale, much shorter timescale variability and eruptive events are evidnt both observationally and experimentally highlighting the verydynamical nature of the process( ee e.g., Lin et al. 2005; Park et al. 2006; Karlický & Kliem 2010).”