Study of sudden magnetic storm commencement from observations with second time resolution

The article presents the results of a studying detection of the sudden commencement (SC) and main impulse (MI) of a magnetic storm as a function of the geographic coordinates of magnetic observatories and Universal Time, using modern data with second time resolution. The analysis was carried out for two events in which an interplanetary shock wave impacting the magnetosphere was associated with interplanetary coronal mass ejections (CMEs) with sources in different hemispheres of the Sun. The authors propose an approach to determine the time points of SC and MI detection. It is concluded that the SC and MI detection times may differ by several seconds to more than a minute at magnetic observatories located at different geographic latitudes and longitudes. For the studied events, the graphs of SC and MI detection as functions of the geographic coordinates of magnetic observatories and Universal Time revealed trends according to which, on average, the higher station the latitude, the later SC and MI are detected at the station.

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Publication Details

Journal
Геомагнетизм и аэрономия
Published
2024-12-26
DOI
https://doi.org/10.31857/s0016794024030034
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
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article

Study of sudden magnetic storm commencement from observations with second time resolution

L. I. Gromova, Ю. С. Загайнова, S. V. Gromov, В. Г. Файнштейн
Геомагнетизм и аэрономия
Ionosphere and magnetosphere dynamics
article

Study of sudden magnetic storm commencement from observations with second time resolution

L. I. Gromova, Ю. С. Загайнова, S. V. Gromov, В. Г. Файнштейн
article en

Abstract

The article presents the results of a studying detection of the sudden commencement (SC) and main impulse (MI) of a magnetic storm as a function of the geographic coordinates of magnetic observatories and Universal Time, using modern data with second time resolution. The analysis was carried out for two events in which an interplanetary shock wave impacting the magnetosphere was associated with interplanetary coronal mass ejections (CMEs) with sources in different hemispheres of the Sun. The authors propose an approach to determine the time points of SC and MI detection. It is concluded that the SC and MI detection times may differ by several seconds to more than a minute at magnetic observatories located at different geographic latitudes and longitudes. For the studied events, the graphs of SC and MI detection as functions of the geographic coordinates of magnetic observatories and Universal Time revealed trends according to which, on average, the higher station the latitude, the later SC and MI are detected at the station.

Геомагнетизм и аэрономияVol. 64(3)
Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation (RU), Institute of Solar-Terrestrial Physics (RU)
Life below water
Openalex Percentile: Top 82%
Ionosphere and magnetosphere dynamics
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