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Behavior of the intensity of galactic and anomalous cosmic rays in the outer heliosphere and large-scale electric fields

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The behavior of the intensity of anomalous and galactic cosmic rays in the outer heliosphere is compared. The previous hypothesis, according to which the lowest energy galactic cosmic rays affected by large-scale electric fields far beyond the termination shock wave of the solar wind may contribute to the behavior of the anomalous component intensity, is analyzed.

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Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia

    M. S. Kalinin & M. B. Krainev

Authors
  1. M. S. Kalinin
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  2. M. B. Krainev
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Additional information

Original Russian Text © M.S. Kalinin, M.B. Krainev, 2007, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2007, Vol. 71, No. 7, pp. 1015–1018.

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Kalinin, M.S., Krainev, M.B. Behavior of the intensity of galactic and anomalous cosmic rays in the outer heliosphere and large-scale electric fields. Bull. Russ. Acad. Sci. Phys. 71, 984–987 (2007). https://doi.org/10.3103/S1062873807070271

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  • DOI: https://doi.org/10.3103/S1062873807070271

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