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Titlebook: Cosmic Rays in the Heliosphere; Volume Resulting fro L. A. Fisk,J. R. Jokipii,K.-P. Wenzel Book 1998 Springer Science+Business Media Dordre

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The Theory of Anomalous Cosmic Raystion or the solar wind, and are subsequently accelerated to very high energies, greater than 1 GeV. Current thinking has the hulk of the acceleration to very-high energies taking place, by the mechanism of diffusive shock acceleration, at the termination shock of the solar wind. Detailed two-dimensi
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Modeling of 3-D Corotating Cosmic-Ray Structures in the Heliospherecurrent sheet and Corotating Interaction Regions (CIRs). We find that present models can qualitatively account for the observed extension of recurrent 26-day cosmic-ray variations to high heliospheric latitudes if perpendicular diffusion is significant. The recurrent enhancement of low-energy (MeV)
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The Inner Heliosphere — Outer Heliosphere Comparison for Cosmic Ray Modulation 1996 at the end of solar cycle 22. These data come from the IMP spacecraft in the inner heliosphere and the Voyager and Pioneer spacecraft in the outer heliosphere. In the inner heliosphere, the cosmic ray intensities at all energies in 1996 have recovered to almost the same maximum values they had
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A Brief History of Recurrent Solar Modulation of the Galactic Cosmic Rays (1937–1990)that was believed to have its origin in recurrent variations of the geomagnetic field. However, with the introduction of neutron monitor analysis of the nucleonic component, it was shown in the 1940s and 1950s that this cosmic ray intensity variation arose from interplanetary dynamical phenomena. Be
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Recurrent Solar Modulation of the Galactic Cosmic Rays and the Anomalous Nuclear Component in Three nteraction region shocks. Also included are some unpublished measurements that will need to he taken into account in any model for the 26-day modulation phenomena. This report is a brief summary of the principal results from the solar wind, magnetic field and charged particle investigations, and their alternate interpretations.
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Cosmic Ray Electronsd it is probable that the difference in net charge sign from that of nuclei is responsible for many of the observed differences in the behavior of electrons and nuclei under modulation. A consistent picture of the cosmic positron abundance and its time variation may be emerging from the world dataset.
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1385-7525 the state of the field. Such is the case for the study of the behavior of cosmic rays in the heliosphere. We are just passing through solar minimum conditions, when the heliosphere has a well-ordered and relatively simple configuration. We have been fortunate to have an array of spacecraft - unprece
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