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

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概要

• 論文の詳細を見る
• 2010-06-01

著者

• Jacklyn R.

  Antarctic Division Department Of Science And Technology

• NAGASHIMA K.

  Solar-Terrestrial Environment Laboratory, Nagoya University

• KONDO I.

  Institute for Cosmic Ray Research, The University of Tokyo

• MORISHITA I.

  Dept. of Information Management, Asahi University

• Morishita I.

  Dept. Of Information Management Asahi University

関連論文

• 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

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