KONDO I. | Institute for Cosmic Ray Research, The University of Tokyo
スポンサーリンク
概要
関連著者
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NAGASHIMA K.
Solar-Terrestrial Environment Laboratory, Nagoya University
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KONDO I.
Institute for Cosmic Ray Research, The University of Tokyo
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FUJII Z.
Solar-Terrestial Environment Laboratory, Nagoya University
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Jacklyn R.
Antarctic Division Department Of Science And Technology
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MORISHITA I.
Dept. of Information Management, Asahi University
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Morishita I.
Dept. Of Information Management Asahi University
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Nagashima K.
Nagoya Univ. Nagoya Jpn
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Morishita I.
Department Of Engineering University Of Tokyo
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MORI S.
Physics Department, Shinshu University
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MORISHITA I.
Department of Information Management, Asahi University
著作論文
- The influence of the sidereal cosmic-ray anisotropies originated on the tail- and nose-boundaries of the heliomagnetosphere (HMS) upon the solar cosmic-ray anisotropy produced inside the HMS
- Sharply concentrated cosmic-ray excess fluxes from heliomagnetospheric nose and tail boundaries observed with neutron monitors on the ground
- The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10^4 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar