Computer Science
Scientific paper
Aug 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...1e..38z&link_type=abstract
Cosmic Particle Acceleration, 26th meeting of the IAU, Joint Discussion 1, 16-17 August, 2006, Prague, Czech Republic, JD01, #38
Computer Science
Scientific paper
Electron and proton acceleration by a super-Dricer electric field is further investigated in the non-neutral reconnecting current sheet (RCS) with the tangential B_z and transverse magnetic field components Bx varying linearly and exponentially with the distances x and z from the X null-point, respectively. We present semi-analytical estimations of the particle distributions in energy gained at acceleration in an RCS with a strong or weak guiding field By. The accelerated particle spectral indices and their the lower cutoff energies are shown to be dependent on the ratio of the magnetic field components By/Bx and on the exponent index of the transversal magnetic field variations with distance z. This is used for a statistical diagnostics of preferential magnetic field topologies in solar flares in the eras of SMM and RHESSI.
No associations
LandOfFree
Hard X-ray spectral indices in solar flares as probes of the variations of magnetic field topology during a solar cycle. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Hard X-ray spectral indices in solar flares as probes of the variations of magnetic field topology during a solar cycle., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hard X-ray spectral indices in solar flares as probes of the variations of magnetic field topology during a solar cycle. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1781585