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

Yasyukevich, Yu. V.; Vasiliev, R. V.; Rubtsov, A. V.; Alsatkin, S. S.; Artamonov, M. F.; Beletsky, A. B.; Belinskaya, A. Yu.; Berngardt, O. I.; Vesnin, A. M.; Ganitsky, D. A.; Egorov, Ya. I.; Zherebtsov, G. A.; Zolotukhina, N. A.; Ivanova, V. A.; Ivonin, V. A.; Isaeva, E. S.; Kim, A. G.; Kravtsova, M. V.; Kurkin, V. I.; Kushnarev, D. S.; Lebedev, V. P.; Marchuk, R. A.; Medvedev, A. V.; Mikhalev, A. V.; Oinats, A. V.; Olemskoy, S. V.; Podlesny, A. V.; Podlesny, S. V.; Ponomarchuk, S. N.; Ratovsky, K. G.; Sdobnov, V. E.; Setov, A. G.; Syrenova, T. E.; Tashlykov, V. P.; Tkachev, I. D.; Feinstein, V. G.; Cedric, M. V.; Yazev, S. A.

doi:10.7868/S3034506525030161

PII

S30345065S2686739725030161-1

DOI

10.7868/S3034506525030161

Publication type

Article

Status

Published

Authors

Yu. V. Yasyukevich

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

R. V. Vasiliev

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. V. Rubtsov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

S. S. Alsatkin

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

M. F. Artamonov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. B. Beletsky

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. Yu. Belinskaya

Affiliation: Profinnik Institute of Petroleum Geology and Geophysics of Siberian Branch of the Russian Academy of Sciences

O. I. Berngardt

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. M. Vesnin

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

D. A. Ganitsky

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

Ya. I. Egorov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

G. A. Zherebtsov

Occupation: Academician of the RAS
Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

N. A. Zolotukhina

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. A. Ivanova

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. A. Ivonin

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

E. S. Isaeva

Affiliation: Irkutsk state university

A. G. Kim

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

M. V. Kravtsova

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. I. Kurkin

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

D. S. Kushnarev

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. P. Lebedev

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

R. A. Marchuk

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. V. Medvedev

Occupation: Corresponding Member of the RAS
Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. V. Mikhalev

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. V. Oinats

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

S. V. Olemskoy

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. V. Podlesny

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

S. V. Podlesny

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

S. N. Ponomarchuk

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

K. G. Ratovsky

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. E. Sdobnov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

A. G. Setov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

T. E. Syrenova

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. P. Tashlykov

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

I. D. Tkachev

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

V. G. Feinstein

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

M. V. Cedric

Affiliation: Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences

S. A. Yazev

Affiliation:
Institute of solar-terrestrial physics, Siberian Branch of the Russian Academy of Sciences
Irkutsk state university

Volume/ Edition

Volume 521 / Issue number 1

Pages

123-135

Abstract

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.

Keywords

магнитная буря ионосфера Национальный гелиогеофизический комплекс ионозонд радар некогерентного рассеяния интерферометр Фабри—Перо свечение атмосферы распространение радиоволн температура атмосферы

Date of publication

13.11.2024

Year of publication

2024

Number of purchasers

Views

References

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GOST	Alsatkin S., Artamonov M., Beletsky A., Belinskaya A., Berngardt O., Cedric M., Egorov Y., Feinstein V., Ganitsky D., Isaeva E., Ivanova V., Ivonin V., Kim A., Kravtsova M., Kurkin V., Kushnarev D., Lebedev V., Marchuk R., Medvedev A., Mikhalev A., Oinats A., Olemskoy S., Podlesny A., Podlesny S., Ponomarchuk S., Ratovsky K., Rubtsov A., Sdobnov V., Setov A., Syrenova T., Tashlykov V., Tkachev I., Vasiliev R., Vesnin A., Yasyukevich Y., Yazev S., Zherebtsov G., Zolotukhina N. EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS // Doklady Earth Sciences. – 2025. – V. 521. – Issue number 1 C. 123-135 . URL: https://danearthras.ru/s30345065s2686739725030161-1/?version_id=119176. DOI: 10.7868/S3034506525030161
MLA	Alsatkin, S. S, Artamonov, M. F, Beletsky, A. B, Belinskaya, A. Yu, Berngardt, O. I, Cedric, M. V, Egorov, Ya. I, Feinstein, V. G, Ganitsky, D. A, Isaeva, E. S, Ivanova, V. A, Ivonin, V. A, Kim, A. G, Kravtsova, M. V, Kurkin, V. I, Kushnarev, D. S, Lebedev, V. P, Marchuk, R. A, Medvedev, A. V, Mikhalev, A. V, Oinats, A. V, Olemskoy, S. V, Podlesny, A. V, Podlesny, S. V, Ponomarchuk, S. N, Ratovsky, K. G, Rubtsov, A. V, Sdobnov, V. E, Setov, A. G, Syrenova, T. E, Tashlykov, V. P, Tkachev, I. D, Vasiliev, R. V, Vesnin, A. M, Yasyukevich, Yu. V, Yazev, S. A, Zherebtsov, G. A, Zolotukhina, N. A "EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS." Doklady Earth Sciences. 521.1 (2025).:123-135. DOI: 10.7868/S3034506525030161
APA	Alsatkin S., Artamonov M., Beletsky A., Belinskaya A., Berngardt O., Cedric M., Egorov Y., Feinstein V., Ganitsky D., Isaeva E., Ivanova V., Ivonin V., Kim A., Kravtsova M., Kurkin V., Kushnarev D., Lebedev V., Marchuk R., Medvedev A., Mikhalev A., Oinats A., Olemskoy S., Podlesny A., Podlesny S., Ponomarchuk S., Ratovsky K., Rubtsov A., Sdobnov V., Setov A., Syrenova T., Tashlykov V., Tkachev I., Vasiliev R., Vesnin A., Yasyukevich Y., Yazev S., Zherebtsov G., Zolotukhina N. (2025). EXTREME MAGNETIC STORM OF MAY 10–19, 2024: COUPLING BETWEEN NEUTRAL AND CHARGED COMPONENTS OF THE UPPER ATMOSPHERE AND THE EFFECT ON RADIO SYSTEMS. Doklady Earth Sciences. vol. 521, no. 1, pp.123-135 DOI: 10.7868/S3034506525030161

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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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