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The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 104 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field

机译：能量低于104 GeV的银河系和太阳起源的宇宙射线恒星各向异性的存在以及它们的调制是由星际磁场中太阳磁层及其邻近气态的行为模式引起的

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K. Nagashima; I. Morishita; Z. Fujii; S. Mori; I. Kondo; R. M. Jacklyn;
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1. 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 magnetic field [J] . K. Nagashima, I. Morishita, Z. Fujii, Earth, planets and space: EPS . 2012,第7期

机译：能量低于10〜4 GeV的银河系和太阳系的宇宙射线恒星各向异性的存在以及它们的调制是由星际磁场中日磁层及其邻近气态的行为模式引起的
2. The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 10⁴ GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field [J] . K. Nagashima, I. Morishita, Z. Fujii, Earth, planets and space: EPS . 2012,第7期

机译：能量低于10 ^{4 GeV的银河系和太阳系的宇宙射线恒星各向异性的存在以及它们的调制是由星际磁场中日磁层及其邻近气态的行为模式引起的}
3. Coexistence of cosmic-ray sidereal anisotropies originating in galactic space and at the heliomagnetospheric nose and tail boundaries, observed with muon detectors in the energy region of 60 similar to 100 GeV [J] . Nagashima K, Fujii Z Earth, planets and space: EPS . 2006,第11期

机译：在60的能量区域（类似于100 GeV）中使用μ子探测器检测到的起源于银河空间以及日磁磁层的鼻子和尾巴边界的宇宙射线恒星各向异性的共存
4. Galactic cosmic ray modulation along with geomagnetic activity, interplanetary magnetic field and solar wind [C] . REKHA AGARWAL, RAJESH K. MI SHRA, S. K. PANDEY, Proceedings of the 32nd International Cosmic Ray Conference . 2011

机译：银河宇宙射线调制以及地磁活动，行星际磁场和太阳风
5. Coexistence of cosmic-ray sidereal anisotropies originating in galactic space and at the heliomagnetospheric nose and tail boundaries, observed with muon detectors in the energy region of 60∼100 GeV [O] . K. Nagashima, Z. Fujii 2014

机译：在60〜100 GeV的能量范围内使用μ子探测器观测到的起源于银河空间和日磁磁层鼻和尾边界的宇宙射线恒星各向异性的共存

The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 104 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field

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