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Sharply concentrated cosmic-ray excess fluxes from heliomagnetospheric nose and tail boundaries observed with neutron monitors on the ground
Earth, Planets and Space volume 57, pages 1083–1091 (2005)
Abstract
Two kinds of sharply concentrated excess flux of cosmic rays from heliomagnetospheric nose and tail directions (right ascension α ∼ 18 hours and ∼ 6 hours) are found by the analysis of sidereal daily variation of neutron intensity (median energy Em ∼ 20 GeV) on the ground. These fluxes do not show any response to the polarity reversal of solar magnetic field at the north pole and is contradictory to the simulation of the solar modulation of galactic anisotropy, which produces sidereal variation at the Earth greater in the negative polarity state than in the positive state. This indicates that they are not of the galactic origin and would be produced on the heliomagnetospheric nose and tail boundaries where it is considered that the interaction between the galactic and solar magnetic fields could produce the cosmic-ray acceleration. The acceleration mechanism producing the polarity-independent sidereal variation against solar modulation will be discussed.
References
Bercovitch, M., The response of the cosmic ray sidereal diurnal variation to reversal of the solar magnetic field, Proc. International Symposium on Cosmic Ray Modulation in the Heliosphere, 329–336, Iwate Univ., Morioka, Japan, 1984.
Caballero-Lopez, R. A., H. Moraal, and F. B. McDonald, Galactic cosmic ray modulation: effects of the solar wind termination shock and the heliosheath, J. Geophys. Res., 109, A05105, doi:10.1029/2003JA010358, 2004.
Fenton, A. G., R. M. Jacklyn, and R. B. Taylor, Cosmic ray observations at 42 mwe underground at Hobart, Tasmania, Il. Nuovo Cimento, 22, 3985–3996, 1961.
Howard, R., Studies of solar magnetic fields I: The average field strength. Solar Phys., 38, 283–299, 1974.
Jacklyn, R. M., Evidence for a two-way sidereal anisotropy in the charged primary cosmic radiation, Nature, 211, 690–693, 1966.
Jacklyn, R. M., Galactic cosmic ray anisotropies in the energy range 1011–1014 eV., Proc. Astron. Soc. Australia, 6, 425–436, 1986.
Jokipii, J. R., J. Kota, and E. Merenyi, The gradient of galactic cosmic rays at the solar-wind termination shock, Astrophys. J., 405, 782–786, 1993.
Kiraly, P., J. Kota, J. L. Osborne, N. S. Stepley, and A.W. Wolfendale, The anisotropy of cosmic ray from 1011 to 1020 eV, Riv. Nuovo Cimento, 2(2), 1–46, 1979.
McDonald, F. B., E. C. Stone, A. C. Cummings, B. Heikkila, N. Lal, and W. R. Webber, Enhancements of energetic particles near the heliospheric termination shock, Nature, 426, 48–51, 2003.
Mori, S., S. Yasue, S. Sagisaka, M. Ichinose, K. Chino, S. Akahane, and T. Higuchi, Matsushiro underground cosmic-ray observation (220 m.w.e. depth) and the observation of high energy (#1012 eV) cosmic ray intensity variation, J. Fac. Sci., Shinshu Univ., Matsumoto, Japan., 24(1), 1989.
Nagashima, K. and S. Mori, Summary of general discussion on sidereal daily variation of high energy cosmic rays, Proceedings of International Cosmic Ray Symposium on High Energy Cosmic Ray Modulation, Tokyo Univ., Japan, 326–360, 1976.
Nagashima, K. and I. Morishita, Cosmic ray sidereal daily variation of galactic origin observable in the heliomagnetosphere, Rep. of Cosmic- Ray Research Laboratory, Nagoya Univ., Nagoya, Japan, no. 8, 1983.
Nagashima, K., I. Morishita, and S. Yasue, Asymptotic orbits of cosmic rays incident on the Earth from galactic space, Proc. 17th International Cosmic Ray Conference, 4, 189–192, 1981.
Nagashima, K., I. Morishita, and S. Yasue, Modulation of galactic cosmic ray anisotropy in the heliomagnetosphere: Average sidereal daily variation, Planet. Space Sci., 30, 879–896, 1982.
Nagashima, K., Y. Ishida, S. Mori, and I. Morishita, Cosmic ray sidereal diurnal variation of galactic origin observed by neutron monitors, Planet. Space Sci., 31, 1269–1278, 1983.
Nagashima, K., K. Fujimoto, and R. M. Jacklyn, The excess influx of galactic cosmic rays from the tailend side of the heliomagnetosphere, inferred from their sidereal daily variation, Proceedings of International Mini-Conference on Solar Particle Physics and Cosmic Ray Modulation, Solar-Terrestrial Environment Laboratory, Nagoya Univ., Nagoya, Japan, 93–98, 1995.
Nagashima, K., K. Fujimoto, and R. M. Jacklyn, Galactic and heliotail-in anisotropies of cosmic rays as the origin of sidereal daily variation in the energy region <104 GeV, J. Geophys. Res., 103, 17429–17440, 1998.
Nagashima, K., Z. Fujii, and K. Munakata, Solar modulation of galactic and heliotail-in anisotropies of cosmic rays at Sakashita underground station (320 ∼ 650 GeV), Earth Planets Space, 56, 479–483, 2004.
Parker, E. N., Interplanetary Dynamic Process, pp. 115–128, Interscience Division, John Wiley and Sons, New York, 1963.
Yasue, S., I. Morishita, and K. Nagashima, Modulation of galactic cosmic ray anisotropy in heliomagnetosphere: influence of cosmic ray scattering on sidereal daily variation, Planet. Space Sci., 33, 1057–1068, 1983.
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Nagashima, K., Kondo, I. & Fujii, Z. Sharply concentrated cosmic-ray excess fluxes from heliomagnetospheric nose and tail boundaries observed with neutron monitors on the ground. Earth Planet Sp 57, 1083–1091 (2005). https://doi.org/10.1186/BF03351887
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DOI: https://doi.org/10.1186/BF03351887