Cosmic ray latitudinal effects predicted by a three-dimensional drift model

Advances in Space Research

Volumn 19, Issue 6, 1997, Pages 893-896

  Hattingh, M ^a   Burger, R A ^a   Potgieter, M S ^a   Haasbroek, L J ^a  

^a NORTH WEST UNIVERSITY   (South Africa)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0004512845     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00298-6     Document Type: Article

References (9)

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4. Hattingh, M., and R. A. Burger, Some Properties of a Fully Three-dimensional Drift Model for the Modulation of Galactic Cosmic Rays, Proc. 24th ICRC, Rome, 4, 337 (1995).
5. Heber, B., W. Dröge, H. Kunow, R. Müller-Mellin, and G. Wibberenz, Spatial Variation of >106 MeV Proton Fluxes Observed during the Ulysses Rapid Latitude Scan: Ulysses COSPIN/KET Results, Geophys. Res. Lett. 23, 1513 (1996).
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7. Kóta, J. and J. R. Jokipii, Interpretation and Consequences of Large-scale Magnetic Variances Observed at High Heliographic Latitude, Geophys. Res. Lett. 22, 3385 (1995b).
8. Simpson, J. A., M. Zhang, and S. Bame, A Solar Polar North-South Asymmetry for Cosmic Ray Propagation in the Heliosphere: the Ulysses Pole-to-pole Rapid Transit, Ap. J. Lett. 465, L1 (1996).
9. Smith, C. W., and J. W. Bieber, Solar Cycle Variation of the Interplanetary Magnetic Field Spiral, Ap. J., 370, 435 (1991).