EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS

Y. V. Yasyukevich; Ясюкевич Ю. В.; R. V. Vasiliev; Васильев Р. В.; A. V. Rubtsov; Рубцов А. В.; S. S. Alsatkin; Алсаткин С. С.; M. F. Artamonov; Артамонов М. Ф.; A. B. Beletsky; Белецкий А. Б.; A. Y. Belinskaya; Белинская А. Ю.; O. I. Berngardt; Бернгардт О. И.; A. M. Vesnin; Веснин А. М.; D. A. Ganitsky; Ганицкий Д. А.; Y. I. Egorov; Егоров Я. И.; G. A. Zherebtsov; Жеребцов Г. А.; N. A. Zolotukhina; Золотухина Н. А.; V. A. Ivanova; Иванова В. А.; V. A. Ivonin; Ивонин В. А.; E. S. Isaeva; Исаева Е. С.; A. G. Kim; Ким А. Г.; M. V. Kravtsova; Кравцова М. В.; V. I. Kurkin; Куркин В. И.; D. S. Kushnarev; Кушнарев Д. С.; V. P. Lebedev; Лебедев В. П.; R. A. Marchuk; Марчук Р. А.; A. V. Medvedev; Медведев А. В.; A. V. Mikhalev; Михалев А. В.; A. V. Oinats; Ойнац А. В.; S. V. Olemskoy; Олемской С. В.; A. V. Podlesny; Подлесный А. В.; S. V. Podlesny; Подлесный С. В.; S. N. Ponomarchuk; Пономарчук С. Н.; K. G. Ratovsky; Ратовский К. Г.; V. E. Sdobnov; Сдобнов В. Е.; A. G. Setov; Сетов А. Г.; T. E. Syrenova; Сыренова Т. Е.; V. P. Tashlykov; Ташлыков В. П.; I. D. Tkachev; Ткачёв И. Д.; V. G. Fainshtein; Файнштейн В. Г.; M. V. Cedric; Цедрик М. В.; S. A. Yazev; Язев С. А.

doi:10.31857/S2686739725030161

EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS

作者: Yasyukevich Y.V.¹, Vasiliev R.V.¹, Rubtsov A.V.¹, Alsatkin S.S.¹, Artamonov M.F.¹, Beletsky A.B.¹, Belinskaya A.Y.², Berngardt O.I.¹, Vesnin A.M.¹, Ganitsky D.A.¹, Egorov Y.I.¹, Zherebtsov G.A.¹, Zolotukhina N.A.¹, Ivanova V.A.¹, Ivonin V.A.¹, Isaeva E.S.³, Kim A.G.¹, Kravtsova M.V.¹, Kurkin V.I.¹, Kushnarev D.S.¹, Lebedev V.P.¹, Marchuk R.A.¹, Medvedev A.V.¹, Mikhalev A.V.¹, Oinats A.V.¹, Olemskoy S.V.¹, Podlesny A.V.¹, Podlesny S.V.¹, Ponomarchuk S.N.¹, Ratovsky K.G.¹, Sdobnov V.E.¹, Setov A.G.¹, Syrenova T.E.¹, Tashlykov V.P.¹, Tkachev I.D.¹, Fainshtein V.G.¹, Cedric M.V.¹, Yazev S.A.¹^,3
隶属关系:
1. Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences
2. Trofimuk Institute of Petroleum Geology and Geophysics of Siberian Branch of the Russian Academy of Sciences
3. Irkutsk state university
期: 卷 521, 编号 1 (2025)
页面: 123-135
栏目: ATMOSPHERIC AND HYDROSPHERIC PHYSICS
##submission.dateSubmitted##: 20.08.2025
##submission.datePublished##: 15.12.2025
URL: https://journals.rcsi.science/2686-7397/article/view/305240
DOI: https://doi.org/10.31857/S2686739725030161
EDN: https://elibrary.ru/ftjnye
ID: 305240

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Active exploration of space for communication, navigation, and Earth remote sensing in recent decades has drawn increased attention to the study of the Sun’s impact on the Earth and requires creating effective models for space weather forecast. Magnetic storms that produce disturbances in the ionosphere and atmosphere are the strongest manifestation of space weather. Among such events is the magnetic storm that started on May 10, 2024, during which the auroral oval reached 19° N. Over the past 20 years since the last magnetic storm of similar intensity was observed, new scientific facilities have been put into operation as part of the National Heliogeophysical Complex of the Russian Academy of Sciences. A huge decrease in the electron density (by a factor of five relative to the background level) and record-breaking airglow of the upper atmosphere (the atomic oxygen red line airglow exceeded 25 kR) compared to the strongest storms in solar cycle 23 were recorded. The combined optical and radio-physical measurements in Eastern Siberia, supported by data from global networks, demonstrated the correlation between the temperature increase in the upper atmosphere and a strong decrease in the ionospheric electron density at mid-latitudes due to increased recombination during the storm. Combined measurements from ionosonde and high-frequency radar networks have shown a significant deterioration in the conditions of radio wave propagation. The complementarity of the currently deployed scientific instruments opens up new opportunities for monitoring the state of the near-Earth space, as well as for studying and modeling dynamic processes during such extreme phenomena with unprecedented detail.

关键词

magnetic storm, ionosphere, National Heliogeophysical Complex, ionosonde, incoherent scatter radar, Fabry–Pérot interferometer, airglow, radio wave propagation, atmosphere temperature

参考

Pilipenko V. Space weather impact on ground-based technological systems // Sol.-Terr. Phys. 2021. V. 7. № 3. P. 68–104. https://doi.org/10.12737/stp-73202106
Meng X., Tsurutani B.T., Mannucci A.J. The Solar and Interplanetary Causes of Superstorms (Minimum Dst ≤ −250 nT) During the Space Age // J. Geophys. Res. Space Phys. 2019. V. 124. № 6. P. 3926–3948. https://doi.org/10.1029/2018JA026425.
Wang C., Xu J., Liu L. et al. Contribution of the Chinese Meridian Project to space environment research: Highlights and perspectives // Sci. China Earth Sci. 2023. V. 66. № 7. P. 1423–1438. https://doi.org/10.1007/s11430-022-1043-3
Zherebtsov G. Complex of heliogeophysical instruments of new generation // Sol.-Terr. Phys. 2020. V. 6. № 2. P. 3–13. https://doi.org/10.12737/stp-62202001
Gonzalez W.D., Joselyn J.A., Kamide Y. et al. What is a geomagnetic storm? // J. Geophys. Res. Space Phys. 1994. V. 99. № A4. P. 5771–5792. https://doi.org/10.1029/93JA02867
Pi X., Mannucci A.J., Lindqwister U.J., Ho C.M. Monitoring of global ionospheric irregularities using the Worldwide GPS Network // Geophys. Res. Lett. 1997. V. 24. № 18. P. 2283–2286. https://doi.org/10.1029/97GL02273
Jia H., Yang Z., Li B. ROTI-based statistical regression models for GNSS precise point positioning errors associated with ionospheric plasma irregularities // GPS Solut. 2024. V. 28. № 3. P. 105. https://doi.org/10.1007/s10291-024-01648-0
Reinisch B.W., Galkin I.A. Global Ionospheric Radio Observatory (GIRO) // Earth Planets Space. 2011. V. 63. № 4. P. 377–381. https://doi.org/10.5047/eps.2011.03.001
Vasilyev R., Artamonov M., Beletsky A. et al. Scientific goals of optical instruments of the National Heliogeophysical Complex // Sol.-Terr. Phys. 2020. V. 6. № 2. P. 84–97. https://doi.org/10.12737/stp-62202008
Vasilyev R., Artamonov M., Beletsky A. et al. Registering upper atmosphere parameters in East Siberia with Fabry–Perot Interferometer KEO Scientific “Arinae” // Sol.-Terr. Phys. 2017. V. 3. № 3. P. 61–75. https://doi.org/10.12737/stp-33201707
Ratovsky K.G., Medvedev A.V., Tolstikov M.V., Kushnarev D.S. Case studies of height structure of TID propagation characteristics using cross-correlation analysis of incoherent scatter radar and DPS-4 ionosonde data // Adv. Space Res. 2008. V. 41. № 9. P. 1454–1458. https://doi.org/10.1016/j.asr.2007.03.008
Themens D.R., Elvidge S., McCaffrey A. et al. The High Latitude Ionospheric Response to the Major May 2024 Geomagnetic Storm: A Synoptic View // Geophys. Res. Lett. 2024. V. 51. № 19. e2024GL111677. https://doi.org/10.1029/2024GL111677
Bilitza D., Pezzopane M., Truhlik V. et al. The International Reference Ionosphere Model: A Review and Description of an Ionospheric Benchmark // Rev. Geophys. 2022. V. 60. № 4. P. 1–11. https://doi.org/10.1029/2022RG000792
Evans J.S., Correira J., Lumpe J.D. et al. GOLD Observations of the Thermospheric Response to the 10–12 May 2024 Gannon Superstorm // Geophys. Res. Lett. 2024. V. 51. № 16. e2024GL110506. https://doi.org/10.1029/2024GL110506
Zherebtsov G.A., Tashchilin A.V., Perevalova N.P., Ratovsky K.G., Medvedeva I.V. Modeling the Influence of Changes in the Parameters of a Neutral Atmosphere on the Ionospheric Electron Density // Dokl. Earth Sci. 2024. V. 517. № 2. P. 1371–1376. https://doi.org/10.1134/S1028334X2460227X
Подлесный А.В., Брынько И.Г., Березовский В.А., Киселёв А.М., Петухов Е.В. Многофункциональный ЛЧМ-ионозонд для мониторинга ионосферы // Гелиогеофизические Исследования. 2013. № 4. C. 24–31.
Berngardt O., Kurkin V., Kushnarev D. et al. ISTP SB RAS decameter radars // Sol.-Terr. Phys. 2020. V. 6. № 2. P. 63–73. https://doi.org/10.12737/stp-62202006
Bland E.C., Heino E., Kosch M.J., Partamies N. SuperDARN Radar-Derived HF Radio Attenuation During the September 2017 Solar Proton Events // Space Weather. 2018. V. 16. № 10. P. 1455–1469. https://doi.org/10.1029/2018SW001916
Ratovsky K.G., Klimenko M.V., Vesnin A.M., Belyuchenko K.V., Yasyukevich Y.V. Comparative Analysis of Geomagnetic Events Identified According to Different Indices // Bull. Russ. Acad. Sci. Phys. 2024. V. 88. № 3. P. 296–302. https://doi.org/10.1134/S1062873823705433
Mikhalev A.V., Beletsky A.B., Kostyleva N.V., Chernigovskaya M.A. Midlatitude auroras in the south of Eastern Siberia during strong geomagnetic storms on October 29-31, 2003 and November 20-21, 2003 // Cosm. Res. 2004. V. 42. № 6. P. 591–596. https://doi.org/10.1007/s10604-005-0006-8

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EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS

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