Author: Unno W. Ohara S. Urata K. Masaki I. Kitamura T. Konishi T. Tsuji K. Chikawa M. Kato Y.
Publisher: Edp Sciences
E-ISSN: 1286-4854|39|4|465-468
ISSN: 0295-5075
Source: EPL (EUROPHYSICS LETTERS), Vol.39, Iss.4, 2010-03, pp. : 465-468
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Chaotic features in the arrival times of cosmic-ray air showers are detected. The observed chaotic series of air showers measured in distant sites for the same time period cannot be explained by the hypothesis of a stochastic noise mixture as proposed by the Torino group.
Related content
Journal de Physique et le Radium, Vol. 10, Iss. 1, 1939-01 ,pp. :
Journal de Physique et le Radium, Vol. 7, Iss. 11, 1936-11 ,pp. :
Radio emission from cosmic ray air showers
Astronomy & Astrophysics, Vol. 412, Iss. 1, 2003-12 ,pp. :
Radio pulses from cosmic ray air showers
Astronomy & Astrophysics, Vol. 480, Iss. 1, 2008-03 ,pp. :
Radio emission from cosmic ray air showers
Astronomy & Astrophysics, Vol. 430, Iss. 3, 2005-02 ,pp. :