Arrival Time Series in Chaotic Cosmic Ray Air Showers

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概要

• 論文の詳細を見る

• Chaotic features detected in the arrival time series of cosmic ray air showers are rediscussed. Chaotic series of air showers observed in the same time period among distant observing sites cannot be explained by the hypothesis of stochastic noise mixture proposed by the Torino group.

• 1997-03-05

著者

• Kitamura T

  Shinshu Univ. Nagano Prefecture Jpn

• Unno W.

  近畿大学

• Ohara S.

  Nara Indust. University

• Urata K.

  Himeji College

• Masaki I.

  Faculty of Letters, Kokugakuin University

• Kitamura T.

  近畿大学

• Konishi T.

  近畿大学

• Tsuji K.

  近畿大学

• Chikawa M.

  近畿大学

• Kato Y.

  近畿大学

• Chikawa Michiyuki

  近畿大学

• Chikawa M

  Kinki Univ. Higashi‐osaka Jpn

• Tsuji K

  近畿大学

• Konishi T

  近畿大学

関連論文

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• Spherically Statistical Tests on the Angular Distributions of Electrons of the IMB events associated with SN 1987A
• A Search for Consecutive Events of Extensive Air Showers with Energy above 0.1 PeV at Sea Level : general properties of the data in phase IV run
• STUDY OF BIOLUMINESCENCE IN DEEP SEA
• Statistical Tests as Spherical Data for Angular Distributions of Neutrinos Burst from SN 1987A
• Expected Reconstruction Error of Arrival Direction in Observation by Water Cerenkov Detector
• Scattering Angle of Cosmic Ray Muons with Energy Loss Deep Underground
• A study of a phenomena deviated from random feature in EAS energy around 100TeV with new Kinki Array
• The Arrival Direction of EAS Observed by Kinki Array with Energy Around 10^ eV (II)
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• Search for bursts of extensive air showers arriving successively over a short period
• A Search for Successive Air Showers with the Same Arrival Direction
• An Investigation of Non-Random Component in Extensive Air Showers Energy above 0.1 PeV at Sea Level
• A Statistical Test on the Spatial Angular Distributions of Electrons from Neutrino Burst from SN 1987A of IMB and Kamiokande Groups
• An Analysis of a Candedate of Non-Random Component in Extensive Air Showers above 0.1PeV
• A New Eperimental System for Observation of Short Arriving Time of Extensive Air Showers Using Computer Controlled Electronic Camac
• The Arrival Direction of EAS Observed by Kinki Array with Energy around 1015〔10の15乗〕eV(2)
• The Arrival Direction of EAS Determined by Kinki Array with Energy Around 1015eV

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