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Prediction of geoeffective solar wind streams near earth according to solar observational data

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Abstract

A semi-empirical model for predicting solar wind (SW) streams is developed based on satellite images of the Sun and corona using a hierarchical approach. The model allows simultaneous calculation of the parameters of all three SW components, i.e., slow SW, high-speed streams from coronal holes, and interplanetary coronal mass ejections, as well as the detection of their possible interaction in the heliosphere.

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Authors and Affiliations

  1. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991, Russia

    Yu. S. Shugay & I. S. Veselovsky

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

    V. A. Slemzin & D. G. Rodkin

  3. Space Research Institute, Russian Academy of Sciences, Profsoyuznaya ul. 84/32, Moscow, 117810, Russia

    I. S. Veselovsky

Authors
  1. Yu. S. Shugay
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  2. V. A. Slemzin
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  3. D. G. Rodkin
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  4. I. S. Veselovsky
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Corresponding author

Correspondence to V. A. Slemzin.

Additional information

Original Russian Text © Yu.S. Shugay, V.A. Slemzin, D.G. Rodkin, I.S. Veselovsky, 2017, published in Kratkie Soobshcheniya po Fizike, 2017, Vol. 44, No. 10, pp. 43–50.

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Shugay, Y.S., Slemzin, V.A., Rodkin, D.G. et al. Prediction of geoeffective solar wind streams near earth according to solar observational data. Bull. Lebedev Phys. Inst. 44, 303–307 (2017). https://doi.org/10.3103/S1068335617100074

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  • DOI: https://doi.org/10.3103/S1068335617100074

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