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Magnetic Reconnection Rate and RHESSI Hard X-Ray Imaging Spectroscopy of Well Resolved X-class Flares. Yan Xu, Ju Jing, Wenda Cao, and Haimin Wang. 2003 Oct. 29 X10. Red: NIR flare ribbons Blue: RHESSI HXR contours correspond to the 50 – 100 keV. Ding et al. 2003.
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Magnetic Reconnection Rate and RHESSI Hard X-Ray Imaging Spectroscopy of Well Resolved X-class Flares Yan Xu, Ju Jing, Wenda Cao, and Haimin Wang
2003 Oct. 29 X10 Red: NIR flare ribbons Blue: RHESSI HXR contours correspond to the 50 – 100 keV
According to Brown et al. 2002 Therefore, electrons with energy greater than 200 could reach 1022 cm-2 Loop length ~ 109 cm, number density in corona ~ 1011 cm-3 ==> Ncorona~ 1020cm-2
More complicate treatment: N ~ , b… Brown et al. 2002
Footpoint Asymmetric e e α
Footpoint Asymmetric e e α α ? RHESSI Visibility + Forward-fit
Footpoint Asymmetric B ?
Magnetic/Mirror Effect? = -2.80 = -2.53 = -2.72
Magnetic/Mirror Effect? = -2.74 = -2.50 = -2.60
Magnetic/Mirror Effect? Power Index B (Gauss)
Shear Angle 20:40:54 20:41:32 20:41:46 20:41:52 20:41:58 20:42:02 20:42:08 20:42:18
Shear Angle 20:40:54 20:41:32 20:41:46 20:41:52 20:41:58 20:42:02 20:42:08 20:42:18
Shear Angle 20:41:32 20:42:02
Shear Angle 20:41:32 20:42:02 Change Rate vs. ???
G-band ~ E field ~ Power-index Contrast Electric Field (V/cm)
G-band ~ E field ~ Power-index Contrast Electric Field (V/cm)
Electron Acceleration Rate RHESSI Observations: Total Number of particles inside the acceleration region Rate of acceleration of electrons (from spatially-integrated HXR intensity) Specific Acceleration Rate
Super-Dreicer Electric Field Acceleration E (Somov 1991) RHESSI observations ~ Vector Magnetograms B// B^ B//