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Cosmic ray intensity dynamics in the region ahead of the interplanetary shock front

  • Proceeding of the 31st Russian Conference on Cosmic Rays
  • Published:
Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

The galactic cosmic rays intensity dynamics prior to the onset of the geomagnetic storm of September 9, 1992, are calculated using a new kinetic method. A comparison of the calculation results and the observational data from ground-level detectors shows satisfactory agreement on both amplitude and time.

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Authors and Affiliations

  1. Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences, Yakutsk, 677980, Russia

    I. S. Petukhov & S. I. Petukhov

Authors
  1. I. S. Petukhov
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  2. S. I. Petukhov
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Corresponding author

Correspondence to I. S. Petukhov.

Additional information

Original Russian Text © I.S. Petukhov, S.I. Petukhov, 2011, published in Izvestiya Rossiiskoi Akademii Nauk. Seriya Fizicheskaya, 2011, Vol. 75, No. 6, pp. 842–844.

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Petukhov, I.S., Petukhov, S.I. Cosmic ray intensity dynamics in the region ahead of the interplanetary shock front. Bull. Russ. Acad. Sci. Phys. 75, 793–795 (2011). https://doi.org/10.3103/S1062873811060360

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  • DOI: https://doi.org/10.3103/S1062873811060360

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