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Astronomical & Astrophysical Transactions
The Journal of the Eurasian Astronomical Society
Volume 26, 2007 - Issue 6: International Colloquium ‚Scattering and Scintillation in Radioastronomy’, June 19–23 2006, Pushchino, Moscow Region, Russia
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Original Articles

Diagnostics of solar wind streams

N. A. Lotova Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region, 142190, RussiaCorrespondence[email protected]
,
K. V. Vladimirskii Lebedev Physical Institute, Russian Academy of Sciences, Moscow, 117924, Russia
&
V. N. Obridko Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region, 142190, Russia
Pages 501-505 | Received 19 Jul 2007, Published online: 13 Dec 2007
 
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Abstract

Up-to-date methods of investigation of solar wind generation are applied to study the types of the streams that form the inhomogeneous jet structure of circumsolar plasma. The particularities of this structure are analysed at the maximum and transition to the declining phase of cycle 23.

Acknowledgements

The work was supported by the Russian Foundation for Basic Research (project no. 06-02-34013).

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