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ULF Disturbances Caused by the Turbulent Sheath of Interplanetary Magnetic Clouds

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

Abstract

Simultaneous disturbances of the total electron content and the horizontal component of geomagnetic field in the range of Pc6 are registered during periods of magnetospheric substorms. Such disturbances arise in intervals of interaction between Earth’s magnetosphere and the turbulent sheath of magnetic clouds. Wavelet analysis of disturbances in the interplanetary magnetic field and the velocity and density of solar wind plasma testify to the existence of oscillations with similar periods in the interplanetary medium.

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Authors and Affiliations

  1. Nizhny Novgorod State University of Architecture and Civil Engineering, 603000, Nizhny Novgorod, Russia

    O. M. Barkhatova

  2. Polar Geophysical Institute, 184209, Apatity, Russia

    V. G. Vorobjev

  3. Nizhny Novgorod State Pedagogical University, 603002, Nizhny Novgorod, Russia

    N. A. Barkhatov & S. E. Revunov

Authors
  1. O. M. Barkhatova
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  2. V. G. Vorobjev
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  3. N. A. Barkhatov
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  4. S. E. Revunov
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Corresponding author

Correspondence to O. M. Barkhatova.

Additional information

Translated by M. Samokhina

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Barkhatova, O.M., Vorobjev, V.G., Barkhatov, N.A. et al. ULF Disturbances Caused by the Turbulent Sheath of Interplanetary Magnetic Clouds. Bull. Russ. Acad. Sci. Phys. 85, 238–241 (2021). https://doi.org/10.3103/S1062873821030060

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  • DOI: https://doi.org/10.3103/S1062873821030060

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