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arxiv: 0902.2967 · v1 · submitted 2009-02-17 · 🌌 astro-ph.GA · astro-ph.HE

10-100 TeV cosmic ray anisotropy measured at Baksan EAS "Carpet" array

classification 🌌 astro-ph.GA astro-ph.HE
keywords anisotropyenergyresultsamplitude-phaseamplitudesanalysisanotherapproach
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Preliminary results of one year anisotropy measurement in the energy range 10^{13} -10^{14} eV as a function of energy are presented. The results are compared for two methods of data analysis: the standard one with meteo correction approach in use and another one so-called "East minus West" method. Amplitudes and phases of anisotropy for three median energies E = 25 TeV, E = 75 TeV and E = 120 TeV are reported. Brief consideration of amplitude-phase dependence of anisotropy on energy is expounded.

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    Direct measurements reveal charge-dependent spectral softenings in primary cosmic rays at a common rigidity of ~15 TV, rejecting mass-dependent softening at >99.999% confidence.