Abstract

The north-south asymmetry for cosmic-ray particles was measured with one instrument of the PAMELA satellite-borne experiment in the period June 2006-May 2009. The analysis has been performed by two independent methods: by comparing the count rates in regions with identical geomagnetic conditions and by comparing the experimental distribution of particle directions with the simulated distribution that would be in the case of an isotropic particle flux. The dependences of the asymmetry on energy release in the PAMELA calorimeter and on time have been constructed. The asymmetry (N n - N s )/(N n + N s ) is 0.06 ± 0.004 at the threshold energy release in the calorimeter and gradually decreases with increasing energy release. The observed effect is shown to be produced by electrons in the energy range 10-100 GeV.

Autore Pugliese

• Bellotti Roberto

Tutti gli autori

• BELLOTTI R.

Titolo volume/Rivista

Non Disponibile

Anno di pubblicazione

2013

ISSN

1063-7761

ISBN

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Numero di citazioni Wos

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Settori ERC

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Codici ASJC

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