EGU2020-9947, updated on 28 Apr 2023
https://doi.org/10.5194/egusphere-egu2020-9947
EGU General Assembly 2020
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

About determination of coordinates of sources of geomagnetic perturbations according to the world network of magnetic observatories

Beibit Zhumabayev1, Ivan Vassilyev2, Vladimir Protsenko2, and Saltanat Zhumabayeva1
Beibit Zhumabayev et al.
  • 1Institute of Ionosphere, Almaty, Kazakhstan
  • 2JSC Special Design and technology Bureau “Granite”, Almaty, Kazakhstan

A method for determining the coordinates of geomagnetic perturbation sources based on joint data processing of the world network of magnetic observatories is proposed. A large statistical material showed the relationship of large geomagnetic storms with the interaction of two or more magnetic clouds formed as a result of coronal mass ejections. To determine the coordinates of the sources of perturbations, it is proposed to use the data of magnetic observatories of the "INTERMAGNET" international network, which has more than 100 observation points distributed around the world and equipped with modern identical hardware. The results of geomagnetic field measurement obtained by magnetic observatories are brought to a single coordinate system. It was achieved by rotation of the axes of local stations, which allows determining the coordinates of the sources of perturbations and evaluating the accuracy of specifying the coordinate system of each local observatory.

How to cite: Zhumabayev, B., Vassilyev, I., Protsenko, V., and Zhumabayeva, S.: About determination of coordinates of sources of geomagnetic perturbations according to the world network of magnetic observatories, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-9947, https://doi.org/10.5194/egusphere-egu2020-9947, 2020.

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