Multiscaling of galactic cosmic ray flux.
Multiscaling analysis of the 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 the ACE/CRIS spacecraft instrument for the year 2000. The analysis reveals strong (turbulencelike) intermittency of the flux dissipation rate for short-term intervals: 1-30 h. It is also found that the type of intermittency can be different in different energy ranges.
Bershadskii
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ICAR, Jerusalem 91000, Israel.
D016880:Anisotropy; D002244:Carbon; D003359:Cosmic Radiation; D005118:Extraterrestrial Environment; D020450:Heavy Ions; D018531:Spacecraft; D013057:Spectrum Analysis
D002244:Carbon