The Arrival Direction of EAS Observed by Kinki Array with Energy Around 10^<15> eV

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概要

• 論文の詳細を見る

• A search for the arrival direction of EAS has been studied for the data of Kinki array and the galactic coordinates with energy range between 10^<14> and 10^<17>eV at sea level. No strong statistical significance of deviation from isotropy was found for the galactic plane enhancement. Concerning on the galactic enhancement tactor fe a comparison with some other higher energy experiment is also presented. It seems that the distribution of arrival direction of EAS suggests very weak energy dependence of fe for EAS at low energy region. In this report, I will present some basic calculation results about the distribution of arrival distribution of EAS in the galactic coordinates.

• 近畿大学の論文
• 1996-02-20

著者

• Kato Y

  近畿大学

• Ohara S

  Faculty Of Economics Nara Industrial University

• Ohara Soji

  Faculty Of Science Hiroshima University:rigaku Denki Kogyo Co. Ltd.

• Ohara Soji

  Faculty Of Economics Nara Sangyo University

• Kitamura Takashi

  近畿大学理工学総合研究所

• Chikawa Michiyuki

  近畿大学理工学総合研究所

• Tsuji Katsufumi

  近畿大学理工学総合研究所

• Konishi Takeharu

  近畿大学理工学総合研究所

• 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

• Tsujies Katsufumi

  近畿大学

• Kato Yukihiro

  近畿大学

• Konishi Takeharu

  近畿大学

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