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  • 1
    Publication Date: 2019-06-28
    Description: Cosmic ray neutron data from the cosmic ray stations from the worldwide network in 1966, 1967 and 1969 are analyzed by means of the three dimensional analysis method by Nagashima. The variations of the north-south anisotropy, which is the first zonal harmonic component obtained from the analysis are studied. The result obtained confirms earlier findings. Relationship of the anisotropy to the interplanetary magnetic field sector polarity is also studied.
    Keywords: SPACE RADIATION
    Type: SH-4.3-13 , 19th Intern. Cosmic Ray Conf - Vol. 5; p 19-22; NASA-CP-2376-VOL-5
    Format: application/pdf
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  • 2
    Publication Date: 2019-06-28
    Description: The spherical harmonic analysis of cosmic ray neutron data from the worldwide network neutron monitor stations during the years, 1966 to 1969 was carried out. The second zonal harmonic component obtained from the analysis corresponds to the Pole-Equator anisotropy of the cosmic ray neutron intensity. Such an anisotropy makes a semiannual variation. In addition to this, it is shown that the Pole-Equator anisotropy makes a variation depending on the interplanetary magnetic field (IMF) sector polarities around the passages of the IMF sector boundary. A mechanism to interpret these results is also discussed.
    Keywords: SPACE RADIATION
    Type: SH-4.3-12 , 19th Intern. Cosmic Ray Conf - Vol. 5; p 15-18; NASA-CP-2376-VOL-5
    Format: application/pdf
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