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.
Physical review letters. 2003 Jan 31;90(4):041101. doi: 10.1103/PhysRevLett.90.041101 Q18.12024
Multiscaling of galactic cosmic ray flux
银河宇宙射线通量的多尺度性 翻译改进
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DOI: 10.1103/PhysRevLett.90.041101 PMID: 12570408
摘要 Ai翻译
Keywords:galactic cosmic ray; multiscaling
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