The Hall fields and fast magnetic reconnection

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A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES (2009, background): “The rate of magnetic reconnection and structure of the outflow exhaust are insensitive to this ratio (Shay & Drake 1998; Hesse et al. 1999; Shay et al. 2007; Drake et al. 2008).”
Ion heating resulting from pickup in magnetic reconnection exhausts (2009, background): “Near the x-line the electric field Ex accelerates the ions in the outflow direction [Drake et al., 2008] but this field is small in the downstream region (Figure 3).”
The Search-Coil Magnetometer for MMS (2016, background): “Yet, in the smallest (electron) diffusion region, the dynamics is thought to be controlled by whistler or kinetic Alfvén waves (KAW) depending on the presence of a finite guide field (Mandt et al. 1994; Rogers et al. 2001; Drake et al. 2008).”
Average properties of the magnetic reconnection ion diffusion region in the Earth's magnetotail: The 2001–2005 Cluster observations and comparison with simulations (2009, background): “Figure 8a shows the out of plane Hall magnetic field and Figure 8b shows the normal (Hall) electric field which except at the central current sheet is due to Hall physics [Karimabadi et al., 2007; Shay et al., 2007; Phan et al., 2007; Drake et al., 2008].”