Multiscaling of galactic cosmic ray flux

Details Multiscaling of galactic cosmic ray flux Multiscaling of galactic cosmic ray flux

2003-05-23

arxiv.org/abs/astro-ph/0305453v1

Phys.Rev.Lett. 90 (2003) 041101

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1103/PhysRevLett.90.041101

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.

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