Real-time monitoring of the behavior of the daily anisotropy vector of cosmic rays according to the data of neutron monitors at Yakutsk and Tiksi stations

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Abstract

Since 2022, the Institute of Cosmophysical Research and Aeronomy (SB RAS) for the first time has been continuously monitoring the forecast of terrestrial winds of space weather based on data from neutron monitors in Yakutsk and Tiksi. Preliminary studies during periods of geomagnetic disturbances in 2022. The peculiarity is that the results of this may provide an additional opportunity for their use for the purpose of forecasting large geomagnetic storms.

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About the authors

A. S. Zverev

Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences

Author for correspondence.
Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk

S. A. Starodubtsev

Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences

Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk

V. G. Grigoryev

Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences

Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk

P. Yu. Gololobov

Shafer Institute of Cosmophysical Research and Aeronomy of Siberian Branch of the Russian Academy of Sciences

Email: ZverevAS@ikfia.ysn.ru
Russian Federation, Yakutsk

References

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  7. Григорьев В.Г., Стародубцев С.А., Гололобов П.Ю. // Изв. РАН. Сер. физ. 2017. Т. 81. № 2. С. 219; Grigoryev V.G., Starodubtsev S.A., Gololobov P. Yu. // Bull. Russ. Acad. Sci. Phys. 2017. V. 81. No. 2. P. 200.
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Supplementary files

Supplementary Files
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2. Fig. 1. Behaviour of the Dst-index and daily anisotropy vectors before and after the onset of 4 geomagnetic storms from data of Yakutsk and Tiksi stations in the GSE system. The vertical axis shows the value of the azimuthal component a11 of the daily anisotropy vector

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