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Publication Details
AFRICAN RESEARCH NEXUS
SHINING A SPOTLIGHT ON AFRICAN RESEARCH
earth and planetary sciences
The modelling of the latitude dependence of cosmic ray protons and electrons in the inner heliosphere
Advances in Space Research, Volume 19, No. 6, Year 1997
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Description
Observations during the fast latitude scan of Ulysses show that the latitude dependence of cosmic ray protons is significantly less than predicted by drift models which were based on the Parker geometry for the heliospheric magnetic field (HMF) and diffusion coefficients ∞ 1/Bp. Recent modeling with a modified HMF and enhanced turbulence in the polar zones of the heliosphere can reproduce the observed latitude dependence for protons reasonably well at high rigidities. It is shown here that incorporating enhanced perpendicular diffusion in the polar direction in a drift model also gives a latitude dependence for protons, over a wide range of rigidities, and a latitude dependence for electrons and therefore a charge-dependence that are compatible with observations. © 1997 COSPAR. Published by Elsevier Science Ltd.
Authors & Co-Authors
Potgieter, Marius S.
South Africa, Potchefstroom
North-west University
Haasbroek, L. J.
South Africa, Potchefstroom
North-west University
Ferrando, Philippe
France, Gif-sur-yvette
Astrophysique, Instrumentation et Modélisation de Paris-saclay
Heber, Berndt
Germany, Kiel
Christian-albrechts-universität zu Kiel
Statistics
Citations: 65
Authors: 4
Affiliations: 3
Identifiers
Doi:
10.1016/S0273-1177(97)00302-5
ISSN:
02731177