Observation of high energy solar particles on September 29, 1989 by neutron monitors with high time resolution.
スポンサーリンク
概要
著者
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Wada Masami
Institute Of Physical And Chemical Research
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MATSUOKA Masaru
Institute of Physical and Chemical Research
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Takahashi Kazuyoshi
Institute Of Physical And Chemical Reseach
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MUNAKATA Kazuoki
Department of Physics, Faculty of Science, Shinshu University
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MUNAKATA Kazuoki
Department of Physics, Shinshu University
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SAKAMOTO Emiko
Institute of Physical and Chemical Research
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KONDO Ichiro
Institute for Cosmic-Ray Research, University of Tokyo
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TAKAHASHI Kazuyoshi
Institute of Physical and Chemical Research
関連論文
- Observation of the North-South Asymmetry of Sidereal Anisotropy of Cosmic Rays at Matsushiro Underground
- Power Spectral Analysis of Cosmic Ray Time Series Data over a Wide Rigidity Range
- Accelerator Beam Experiments of a Prototype Cosmic Ray Heavy Ion Telescope
- Remote sensing of atmospheric temperature profile using three cosmicray muon components (extended abstract)
- Possible contribution of X-rays to energetic electrons measured by proportional counter during auroral substorm
- Rocket Measurements of Auroral-Zone Energetic Electrons at Syowa Station, Antarctica. II. Characteristics of Electrons under Active Auroral Conditions
- Rocket Measurements of Auroral-Zone Energetic Electrons at Syowa Station, Antarctica I. Characteristics of Electrons under no Geomagnetic Disturbance
- Deduction of Solar Neutron Fluences from Large Gamma-Ray Flares
- Observation of high energy solar particles on September 29, 1989 by neutron monitors with high time resolution.