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Global Structure of the Turbulent Solar Wind during 24 Solar Activity Maxima from IPS Observations with the Multibeam Radio Telescope BSA LPI at 111 MHz

  • Radio Heliophysics: Science and Forecasting
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Acknowledgement

This work was supported by RFBR grant 10-02-00078 and by the Program “Experimental and theoretical investigations of the solar system objects” of the Russian Academy of Sciences.

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Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia

    I. V. Chashei, V. I. Shishov, S. A. Tyul’bashev, I. A. Subaev, V. V. Oreshko & S. V. Logvinenko

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  1. I. V. Chashei
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  2. V. I. Shishov
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  3. S. A. Tyul’bashev
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  4. I. A. Subaev
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  5. V. V. Oreshko
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  6. S. V. Logvinenko
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Corresponding author

Correspondence to I. V. Chashei.

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Radio Heliophysics: Science and Forecasting

Guest Editors: Mario M. Bisi, Bernard V. Jackson, and J. Americo Gonzalez-Esparza

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Chashei, I.V., Shishov, V.I., Tyul’bashev, S.A. et al. Global Structure of the Turbulent Solar Wind during 24 Solar Activity Maxima from IPS Observations with the Multibeam Radio Telescope BSA LPI at 111 MHz . Sol Phys 290, 2577–2587 (2015). https://doi.org/10.1007/s11207-015-0703-2

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  • DOI: https://doi.org/10.1007/s11207-015-0703-2

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