Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs

Details Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..672k&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 672-6

Computer Science

Particle Emission, Solar Wind, Particle Acceleration, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A model for the acceleration and transport of suprathermal ions associated with interplanetary coronal mass ejections (CMEs) is presented. The combined mechanisms of stochastic acceleration in the turbulence near interplanetary shocks, first-order Fermi acceleration, stationary spatial diffusion in field irregularities of magnetic clouds, and time-dependent propagation in the upstream solar wind are described. Ions from the bulk solar wind are considered as source populations of suprathermal ions. The results of the model are compared to the spectra of suprathermal ions observed with SOHO/CELIAS/HSTOF during the Bastille Day CME of 14-16 July 2000.

Affiliated with

Also associated with

No associations

Rating

Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs 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 Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Charge-to-mass Fractionation of Suprathermal Ions Associated with Interplanetary CMEs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1149810