ORIGIN OF BACKGROUND EVENTS IN THE KAMIOKANDE MEASUREMENT
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概要
- 論文の詳細を見る
The observed number of background 5958±87 in 1036 days of the Kamiokande III measurement is not inconsistent with contribution of neutron flux generated in showers initiated by underground muons, whereas the contribution of atmospheric ν_e is less than 0.1 events.
- 近畿大学の論文
- 1998-02-28
著者
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Kitamura Takashi
近畿大学理工学総合研究所
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Konishi Takeharu
近畿大学理工学総合研究所
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Konishi Takeharu
近畿大学
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Nakatsuka T
Okayama Shoka University
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Nakatsuka Takao
Okayama Shoka University
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- 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
- 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)
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- ON THE KAMIOKANDE ^8B SOLAR NEUTRINO MEASUREMENT
- ORIGIN OF BACKGROUND EVENTS IN THE KAMIOKANDE MEASUREMENT
- On the Kamiokande 8B Solar Neutrino Measurement
- Origin of Background Events in the Kamiokande Measurement
- Background Events on the Kamiokande Observation of Solar Neutrino Flux
- Background Events on the Kamiokande Observation of Solar Neutrino Flux
- An Evaluation of Scattered Angular Distributions of Low Energy Electrons to a Solar Neutrino Flux of the Kamiokande Observation
- A STUDY OF THE "LEADING" PARTICLE EFFECT IN HADRON PHYSICS OVER A WIDE ENERGY RANGE