3-D Modelling of cosmetic-ray transport in the heliosphere: Toward solar maximum

Advances in Space Research

Volumn 27, Issue 3, 2001, Pages 529-534

  Kota J ^a   Jokipii, J R ^a  

^a UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ACCELERATION; COOLING; COSMIC RAYS; DIFFUSION; GALAXIES; MAGNETIC FIELDS;

MULTIPLE CURRENT SHEETS;

SPACE RESEARCH;

COSMIC RAY;

EID: 0034923195     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00090-4     Document Type: Article

References (20)

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5. Mechanism for latitudinal transport of energetic particles in the heliosphere
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7. Modulation of galactic cosmic rays at solar minimum
8. Epilogue: Cosmic rays in the active heliosphere
9. The role of corotating interaction regions in cosmic-ray modulation
10. Modeling of 3-D corotating cosmic-ray structures in the heliosphere
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15. The modulation of cosmic rays in the heliosphere: Theory and models
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18. 22-year dependence in the size of near ecliptic corotating cosmic-ray depressions during five solar minima
19. Recurrent solar modulation of the galactic cosmic rays and the anomalous nuclear component in three dimensions of the heliosphere
20. Cosmic ray and solar particle investigations over the South polar regions of the sun