Multiscaling of galactic cosmic ray flux
Astrophysics
2009-11-07 v1
Abstract
Multiscaling analysis of differential flux dissipation rate of galactic cosmic rays (Carbon nuclei) is performed in the energy ranges: 56.3-73.4 Mev/nucleon and 183.1-198.7 MeV/nucleon, using the data collected by ACE/CRIS spacecraft instrument for 2000 year. The analysis reveals strong (turbulence-like) intermittency of the flux dissipation rate for the short-term intervals: 1-30 hours. It is also found that type of the intermittency can be different in different energy ranges.
Cite
@article{arxiv.astro-ph/0305453,
title = {Multiscaling of galactic cosmic ray flux},
author = {A. Bershadskii},
journal= {arXiv preprint arXiv:astro-ph/0305453},
year = {2009}
}