Simulation of heavy ion spectra for the solar event of October 5, 2002

Details Simulation of heavy ion spectra for the solar event of October 5, 2002 Simulation of heavy ion spectra for the solar event of October 5, 2002

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sosyr..45..557l&link_type=abstract

Solar System Research, Volume 45, Issue 6, pp.557-561

Physics

Scientific paper

The results of numerical simulation of stochastic acceleration of the heavy ions (3He, 4He, 16O, and 56Fe) are presented for the impulsive solar event of October 5, 2002. The energy spectra of the aforementioned particles have peculiarities (depressions) in the low-energy region (≤1 MeV nucleon-1). Coulomb losses in the flare plasma and adiabatic losses during interplanetary propagation are considered in the study as possible causes of such peculiarities.

Affiliated with

Also associated with

No associations

Rating

Simulation of heavy ion spectra for the solar event of October 5, 2002 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 Simulation of heavy ion spectra for the solar event of October 5, 2002, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulation of heavy ion spectra for the solar event of October 5, 2002 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1439961