| Issue |
J. Space Weather Space Clim.
Volume 15, 2025
Topical Issue - Severe space weather events of May 2024 and their impacts
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|---|---|---|
| Article Number | 51 | |
| Number of page(s) | 16 | |
| DOI | https://doi.org/10.1051/swsc/2025047 | |
| Published online | 28 November 2025 | |
- Aa, E, Chen Y, Luo B. 2024. Dynamic expansion and merging of the equatorial ionization anomaly during the 10–11 May 2024 super geomagnetic storm. Remote Sens 16: 4290. https://doi.org/10.3390/rs16224290. [Google Scholar]
- Abraham-Shrauner, B. 1972. Determination of magnetohydrodynamic shock normal. J Geophys Res 77: 736–739. https://doi.org/10.1029/JA077i004p00736. [Google Scholar]
- Akasofu, SI. 1981. Energy coupling between the solar wind and the magnetosphere. Space Science Rev 28: 121–190. https://doi.org/10.1007/BF00218810. [Google Scholar]
- Akasofu, SI. 1964. The development of the auroral substorm. Planet Space Sci 12: 273–282. https://doi.org/10.1016/0032-0633(64)90151-5. [Google Scholar]
- Akasofu, SI. 2015. Auroral substorms as an electrical discharge phenomenon. Prog Earth Planet Sci 2: 20. https://doi.org/10.1186/s40645-015-0050-9. [Google Scholar]
- Akasofu, SI. 2023. A new understanding of why the aurora has explosive characteristics. Month Not Royal Astronom Soc 518: 3286–3300. https://doi.org/10.1093/mnras/stac3187. [Google Scholar]
- Allen, J, Sauer H, Frank L, Reiff P. 1989. Effects of the March 1989 solar activity. Eos Trans AGU 70: 1479–1488. https://doi.org/10.1029/89EO00409. [Google Scholar]
- Axford, WI, Hines CO. 1961. A unifying theory of high-latitude geophyaical phenomena and geomagnetic storms. Canadian J Phys 39: 1433–1464. https://doi.org/10.1139/p61-172. [Google Scholar]
- Bojilova, R, Mukhtarov P, Pancheva D. 2024. Global ionospheric response during extreme geomagnetic storm in May 2024. Remote Sens 16: 4046. https://doi.org/10.3390/rs16214046. [Google Scholar]
- Bolduc, L. 2002. GIC observations and studies in the Hydro-Québec power system. J Atmos Sol Terr Phys 64: 1793–1802. https://doi.org/10.1016/S1364-6826(02)00128-1. [CrossRef] [Google Scholar]
- Boteler, DH. 2019. A 21st century view of the March 1989 magnetic storm. Space Weather 17: 1427–1441. https://doi.org/10.1029/2019SW002278. [CrossRef] [Google Scholar]
- Burlaga, L, Sittler E, Mariani F, Schwenn R. 1981. Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations. J Geophys Res Space Phys 86: 6673–6684. https://doi.org/10.1029/JA086iA08p06673. [CrossRef] [Google Scholar]
- Burton, RK, McPherron RL, Russell CT. 1975. An empirical relationship between interplanetary conditions and Dst. J Geophys Res 80: 4204–4214. https://doi.org/10.1029/JA080i031p04204. [Google Scholar]
- Caraballo, R, González-Esparza JA, Pacheco CR, Corona-Romero P, Arzate-Flores JA, et al. 2025. The impact of geomagnetically induced currents (GIC) on the Mexican power grid: numerical modeling and observations from the 10 May 2024, geomagnetic storm. Geophys Res Lett 52: e2024GL112749. https://doi.org/10.1029/2024GL112749. [Google Scholar]
- Carmo, CS, Dai L, Wrasse CM, Barros D, Takahashi H, et al. 2024. Ionospheric response to the extreme 2024 Mother’s Day geomagnetic storm over the latin American sector. Space Weather 22: e2024SW004054. https://doi.org/10.1029/2024SW004054. [Google Scholar]
- Chakraborty, SK, Hajra R, Paul A. 2008. Ionosphere near the anomaly crest in Indian zone during magnetic storm on 13–14 March 1989. Ind J Radio Space Phys 37: 396–407. http://nopr.niscpr.res.in/handle/123456789/2775. [Google Scholar]
- Chapman, S, Ferraro VCA. 1931. A new theory of magnetic storms. Terres Magn Atmos Electr 36: 77–97. https://doi.org/10.1029/TE036i002p00077. [Google Scholar]
- Clausen, LBN, Nickisch H. 2018. Automatic classification of auroral images from the oslo auroral themis (OATH) data set using machine learning. J Geophys Res Space Phys 123: 5640–5647. https://doi.org/10.1029/2018JA025274. [Google Scholar]
- Despirak, IV, Lyubchich AA, Kleimenova NG. 2019. Supersubstorms and conditions in the solar wind. Geomag Aeron 59: 170–176. https://doi.org/10.1134/S0016793219020075. [Google Scholar]
- Dessler, AJ, Parker EN. 1959. Hydromagnetic theory of geomagnetic storms. J Geophys Res 64: 2239–2252. https://doi.org/10.1029/JZ064i012p02239. [CrossRef] [Google Scholar]
- Dungey, JW. 1961. Interplanetary magnetic field and the auroral zones. Phys Rev Lett 6: 47–48. https://doi.org/10.1103/PhysRevLett.6.47. [CrossRef] [Google Scholar]
- Echer, E, Gonzalez WD, Tsurutani BT. 2008.. Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23. Geophys Res Lett 35: L06S03. https://doi.org/10.1029/2007GL031755. [Google Scholar]
- Foster, JC, Erickson PJ, Nishimura Y, Zhang SR, Bush DC, et al. 2024. Imaging the May 2024 extreme aurora with ionospheric total electron content. Geophys Res Lett 51: e2024GL111981. https://doi.org/10.1029/2024GL111981. [Google Scholar]
- Fu, WD, Fu HS, Zhang WZ, Yu Y, Cao JB. 2025. Compression of Earth’s magnetopause down to 5 RE during the superstorm on 10 May 2024. Geophys Res Lett 52: e2024GL114040. https://doi.org/10.1029/2024GL114040. [Google Scholar]
- Gjerloev, JW, Hoffman RA, Ohtani S, Weygand J, Barnes R. 2010. Response of the auroral electrojet indices to abrupt southward IMF turnings. Ann Geophys 28: 1167–1182. https://doi.org/10.5194/angeo-28-1167-2010. [Google Scholar]
- Gjerloev, JW. 2012. The SuperMAG data processing technique. J Geophys Res Space Phys 117: A09213. https://doi.org/10.1029/2012JA017683. [Google Scholar]
- Gonzalez, WD, Joselyn JA, Kamide Y, Kroehl HW, Rostoker G, et al. 1994. What is a geomagnetic storm? J Geophys Res Space Phys 99: 5771–5792. https://doi.org/10.1029/93JA02867. [CrossRef] [Google Scholar]
- Gonzalez, WD, Tsurutani BT. 1987. Criteria of interplanetary parameters causing intense magnetic storms (Dst < −100 nT). Planet Space Sci 35: 1101–1109. https://doi.org/10.1016/0032-0633(87)90015-8. [Google Scholar]
- Gonzalez-Esparza, JA, Sanchez-Garcia E, Sergeeva M, Corona-Romero P, Gonzalez-Mendez LX, et al. 2024. The Mother’s Day geomagnetic storm on 10 May 2024: Aurora observations and low latitude space weather effects in Mexico. Space Weather 22: e2024SW004111. https://doi.org/10.1029/2024SW004111. [Google Scholar]
- Gopalswamy, N, Yashiro S, Michalek G, Xie H, Lepping RP, Howard RA. 2005. Solar source of the largest geomagnetic storm of cycle 23. Geophys Res Lett 32: L12S09. https://doi.org/10.1029/2004GL021639. [Google Scholar]
- Grandin, M, Bruus E, Ledvina VE, Partamies N, Barthelemy M, et al. 2024. The Gannon Storm: Citizen science observations during the geomagnetic superstorm of 10 May 2024. Geosci Commun 7: 297–316. https://doi.org/10.5194/gc-7-297-2024. [CrossRef] [Google Scholar]
- Guo, J, Feng X, Emery BA, Zhang J, Xiang C, et al. 2011. Energy transfer during intense geomagnetic storms driven by interplanetary coronal mass ejections and their sheath regions: Energy transfer. J Geophys Res Space Phys 116: A05106. https://doi.org/10.1029/2011JA016490. [Google Scholar]
- Guo, X, Zhao B, Yu T, Hao H, Sun W, et al. 2024. East–West difference in the ionospheric response during the recovery phase of May 2024 super geomagnetic storm over the East Asian. J Geophys Res Space Phys 129: e2024JA033170. https://doi.org/10.1029/2024JA033170. [Google Scholar]
- Hajra, R, Echer E, Tsurutani BT, Gonzalez WD. 2014. Solar wind-magnetosphere energy coupling efficiency and partitioning: HILDCAAs and preceding CIR storms during solar cycle 23. J Geophys Res Space Phys 119: 2675–2690. https://doi.org/10.1002/2013JA019646. [Google Scholar]
- Hajra, R, Tsurutani BT, Lakhina GS, Lu Q, Du A. 2024a. Interplanetary causes and impacts of the 2024 May superstorm on the geosphere: An overview. Astrophys J 974: 264. https://doi.org/10.3847/1538-4357/ad7462. [Google Scholar]
- Hajra, R, Tsurutani BT. 2018. Interplanetary shocks inducing magnetospheric supersubstorms (SML < −2500 nT): Unusual auroral morphologies and energy flow. Astrophys J 858: 123. https://doi.org/10.3847/1538-4357/aabaed. [Google Scholar]
- Hajra, R, Tsurutani BT, Echer E, Gonzalez WD, Gjerloev JW. 2016. Supersubstorms (SML < −2500): Magnetic storm and solar cycle dependences. J Geophys Res Space Phys 121: 7805–7816. https://doi.org/10.1002/2015JA021835. [Google Scholar]
- Hajra, R, Echer E, Franco AMDS, Bolzan MJA. 2023. Earth’s magnetotail variability during supersubstorms (SSSs): A study on solar wind–magnetosphere–ionosphere coupling. Adv Space Res 72: 1208–1223. https://doi.org/10.1016/j.asr.2023.04.013. [Google Scholar]
- Hajra, R, Tsurutani BT, Lu Q, Horne RB, Lakhina GS, et al. 2024b. The April 2023 SYM-H = −233 nT geomagnetic storm: A classical event. J Geophys Res Space Phys 129: e2024JA032986. https://doi.org/10.1029/2024JA032986. [Google Scholar]
- Hayakawa, H, Ebihara Y, Mishev A, Koldobskiy S, Kusano K, et al. 2025. The solar and geomagnetic storms in 2024 May: A flash data report. Astrophys J 979: 49. https://doi.org/10.3847/1538-4357/ad9335. [Google Scholar]
- Hsu, TS, McPherron RL. 2003. Occurrence frequencies of IMF triggered and nontriggered substorms. J Geophys Res 108: 1307. https://doi.org/10.1029/2002JA009442. [Google Scholar]
- Hugoniot, H. 1887. Mémoire sur la propagation des mouvements dans les corps et spécialement dans les gaz parfaits (première partie). J École Polytech 57: 3–97. [Google Scholar]
- Hugoniot, H. 1889. Mémoire sur la propagation des mouvements dans les corps et spécialement dans les gaz parfaits (deuxième partie). J École Polytech 58: 1–125. [Google Scholar]
- Iyemori, T. 1990. Storm-time magnetospheric currents inferred from mid-latitude geomagnetic field variations. J Geomag Geoelectr 42: 1249–1265. https://doi.org/10.5636/jgg.42.1249. [Google Scholar]
- Kennel, CF, Edmiston JP, Hada T. 1985. A quarter century of collisionless shock research. In: Geophysical Monograph Series, RG, Stone, Tsurutani BT (Eds.). American Geophysical Union, Washington, D.C., pp. 1–36. https://doi.org/10.1029/GM034p0001. [Google Scholar]
- Knipp, DJ, Tobiska WK, Emery BA. 2004. Direct and indirect thermospheric heating sources for solar cycles 21–23. Solar Phys 224: 495–505. https://doi.org/10.1007/s11207-005-6393-4. [CrossRef] [Google Scholar]
- Laitinen, J, Holappa L, Vanhamäki H. 2024. The polarity of IMF By strongly modulates particle precipitation during high-speed streams. Geophys Res Lett 51: e2024GL110877. https://doi.org/10.1029/2024GL110877. [Google Scholar]
- Lakhina, GS, Tsurutani BT, Kojima H, Matsumoto H. 2000. “Broadband” plasma waves in the boundary layers. J Geophys Res Space Phys 105: 27791–27831. https://doi.org/10.1029/2000JA900054. [Google Scholar]
- Lakhina, GS, Tsurutani BT. 2016. Geomagnetic storms: Historical perspective to modern view. Geosci Lett 3: 5. https://doi.org/10.1186/s40562-016-0037-4. [Google Scholar]
- Lee, W, Liu G, Wu DL, Rowland DE. 2025. Ionospheric response to the 10 May 2024 geomagnetic storm as observed in GNSS radio occultation electron density. J Geophys Res Space Phys , 130: e2024JA033489. https://doi.org/10.1029/2024JA033489. [Google Scholar]
- Liou, K, Sotirelis T, Mitchell E. 2020.Control of the East–West component of the interplanetary magnetic field on the occurrence of magnetic substorms. Geophys Res Lett 47: e2020GL087406. https://doi.org/10.1029/2020GL087406. [Google Scholar]
- Lockwood, M, Owens MJ, Brown W, Vázquez M. 2025. The 2024 May event in the context of auroral activity over the past 375 yr. Mon Not Royal Astron Soc 540: 3596–3624. https://doi.org/10.1093/mnras/staf827. [Google Scholar]
- Lu, Q, Fu H, Wang R, Lu S. 2022. Collisionless magnetic reconnection in the magnetosphere. Chin Phys B 31: 089401. https://doi.org/10.1088/1674-1056/ac76ab. [Google Scholar]
- Lu, S, Guo J, Lu Q, Shu Y, Ren J, Wang R, Hajra R. 2025. Three-dimensional global hybrid simulations of plasma transport and energy conversion during solar wind-magnetosphere interactions. Geophys Res Lett 52: e2025GL117084. https://doi.org/10.1029/2025GL117084. [Google Scholar]
- Marubashi, K, Lepping RP. 2007. Long-duration magnetic clouds: a comparison of analyses using torus- and cylinder-shaped flux rope models. Ann Geophys 25: 2453–2477. https://doi.org/10.5194/angeo-25-2453-2007. [CrossRef] [Google Scholar]
- Nanjo, S, Shiokawa K. 2024. Spatial structures of blue low-latitude aurora observed from Japan during the extreme geomagnetic storm of May 2024. Earth Planets Space 76: 156. https://doi.org/10.1186/s40623-024-02090-9. [CrossRef] [Google Scholar]
- Newell, PT, Gjerloev JW. 2011. Substorm and magnetosphere characteristic scales inferred from the SuperMAG auroral electrojet indices. J Geophys Res 116: A12232. https://doi.org/10.1029/2011JA016936. [Google Scholar]
- Ohma, A, Reistad JP, Hatch SM. 2021. Modulation of magnetospheric substorm frequency: Dipole tilt and IMF By effects. J Geophys Res Space Phys 126: e2020JA028856. https://doi.org/10.1029/2020JA028856. [Google Scholar]
- Ohtani, S. 2021. Revisiting the partial ring current model: Longitudinal asymmetry of ground magnetic depression during geomagnetic storms. J Geophys Res Space Phys 126: e2021JA029643. https://doi.org/10.1029/2021JA029643. [Google Scholar]
- Paul, KS, Moses M, Haralambous H, Oikonomou C. 2025. Effects of the Mother’s Day superstorm (10–11 May 2024) over the global ionosphere. Remote Sens 17: 859. https://doi.org/10.3390/rs17050859. [Google Scholar]
- Perreault, P, Akasofu SI. 1978. A study of geomagnetic storms. Geophys J Int 54: 547–573. https://doi.org/10.1111/j.1365-246X.1978.tb05494.x. [Google Scholar]
- Piersanti, M, Oliveira DM, D’Angelo G, Diego P, Napoletano G, et al. 2025. On the geoelectric field response to the SSC of the May 2024 super storm over Europe. Space Weather 23: e2024SW004191. [Google Scholar]
- Rankine, WJM. 1870. XV. On the thermodynamic theory of waves of finite longitudinal disturbance. Phil Trans Royal Soc 160: 277–288. https://doi.org/10.1098/rstl.1870.0015. [Google Scholar]
- Sckopke, N. 1966. A general relation between the energy of trapped particles and the disturbance field near the Earth. J Geophys Res 71: 3125–3130. https://doi.org/10.1029/JZ071i013p03125. [CrossRef] [Google Scholar]
- Spogli, L, Alberti T, Bagiacchi P, Cafarella L, Cesaroni C, et al. 2024. The effects of the May 2024 Mother’s Day superstorm over the Mediterranean sector: From data to public communication. Ann Geophys 67: PA218. https://doi.org/10.4401/ag-9117. [Google Scholar]
- Sun, W, Li G, Zhang S, Zhao B, Li Y, et al. 2024. Complex ionospheric fluctuations over East and Southeast Asia during the May 2024 super geomagnetic storm. J Geophys Res Space Phys 129: e2024JA033096. https://doi.org/10.1029/2024JA033096. [Google Scholar]
- Themens, DR, Elvidge S, McCaffrey A, Jayachandran PT, Coster A, et al. 2024. The high latitude ionospheric response to the major May 2024 geomagnetic storm: A synoptic view. Geophys Res Lett 51: e2024GL111677. https://doi.org/10.1029/2024GL111677. [Google Scholar]
- Tsurutani, BT, Mannucci AJ, Iijima B, Abdu MA, Sobral JHA, et al. 2004. Global dayside ionospheric uplift and enhancement associated with interplanetary electric fields. J Geophys Res Space Phys 109: 2003JA010342. https://doi.org/10.1029/2003JA010342. [Google Scholar]
- Tsurutani, BT, Hajra R, Echer E, Gjerloev JW. 2015. Extremely intense (SML ≤–2500 nT) substorms: isolated events that are externally triggered? Ann Geophys 33: 519–524. https://doi.org/10.5194/angeo-33-519-2015. [Google Scholar]
- Tsurutani, BT, Hajra R, Tanimori T, Takada A, Remya B, et al. 2016. Heliospheric plasma sheet (HPS) impingement onto the magnetosphere as a cause of relativistic electron dropouts (REDs) via coherent EMIC wave scattering with possible consequences for climate change mechanisms. J Geophys Res Space Phys 121: 10130–10156. https://doi.org/10.1002/2016JA022499. [Google Scholar]
- Tsurutani, BT. 2024. A long and winding path through space weather research. Persp Earth Space Sci 5: e2024CN000259. https://doi.org/10.1029/2024CN000259. [Google Scholar]
- Tsurutani, BT, Gonzalez WD. 2007. A new perspective on the relationship between substorms and magnetic storms. In: Advances in geosciences, Vol. 8: Solar Terrestrial (ST), World Scientific Publishing Co. Pte. Ltd., Singapore, pp. 25–45. https://doi.org/10.1142/9789812708939_0002. [Google Scholar]
- Tsurutani, BT, Hajra R. 2023. Energetics of shock-triggered supersubstorms (SML < −2500 nT). Astrophys J 946: 17. https://doi.org/10.3847/1538-4357/acb143. [Google Scholar]
- Tsurutani, BT, Lin RP. 1985. Acceleration of >47 keV Ions and >2 keV electrons by interplanetary shocks at 1 AU. J Geophys Res 90: 1–11. https://doi.org/10.1029/JA090iA01p00001. [Google Scholar]
- Tsurutani, BT, Gonzalez WD, Tang F, Akasofu SI, Smith EJ. 1988. Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978–1979). J Geophys Res 93: 8519–8531. https://doi.org/10.1029/JA093iA08p08519. [Google Scholar]
- Tsurutani, BT, Sen A, Hajra R, Lakhina GS, Horne RB, et al. 2024. Review of the August 1972 and March 1989 (Allen) space weather events: Can we learn anything new from them? J Geophys Res Space Phys 129: e2024JA032622. https://doi.org/10.1029/2024JA032622. [Google Scholar]
- Tsurutani, BT, Lakhina GS, Verkhoglyadova OP, Gonzalez WD, Echer E, et al. 2011. A review of interplanetary discontinuities and their geomagnetic effects. J Atmos Solar-Terr Phys 73: 5–19. https://doi.org/10.1016/j.jastp.2010.04.001. [Google Scholar]
- Turner, NE, Mitchell EJ, Knipp DJ, Emery BA. 2006. Energetics of magnetic storms driven by corotating interaction regions: A study of geoeffectiveness. In: Geophysical Monograph Series, Vol. 167, BT, Tsurutani, McPherron R, Gonzalez W, Lu G, Sobral JHA, Gopalswamy N (Eds.). American Geophysical Union, Washington, D.C., pp. 113–124. https://doi.org/10.1029/167GM11. [Google Scholar]
- Wang, H, Cheng Q, Lühr H, Zhong Y, Zhang K, et al. 2024. Local time and hemispheric asymmetries of field-aligned currents and polar electrojet during May 2024 superstorm periods. J Geophys Res Space Phys 129: e2024JA033020. https://doi.org/10.1029/2024JA033020. [Google Scholar]
- West, HI, Buck RM, Walton JR. 1972. Shadowing of electron azimuthal-drift motions near the noon magnetopause. Nature Phys Sci 240: 6–7. https://doi.org/10.1038/physci240006a0. [Google Scholar]
- West, HI, Buck RM, Davidson GT. 1981.The dynamics of energetic electrons in the Earth’s outer radiation belt during 1968 as observed by the Lawrence livermore National Laboratory’s spectrometer on Ogo 5. J Geophys Res Space Phys 86: 2111–2142. https://doi.org/10.1029/JA086iA04p02111. [Google Scholar]
- Yokoyama, N, Kamide Y. 1997. Statistical nature of geomagnetic storms. J Geophys Res Space Phys 102: 14215–14222. https://doi.org/10.1029/97JA00903. [Google Scholar]
- Zhou, X, Tsurutani BT. 1999. Rapid intensification and propagation of the dayside aurora: Large scale interplanetary pressure pulses (fast shocks). Geophys Res Lett 26: 1097–1100. https://doi.org/10.1029/1999GL900173. [Google Scholar]
- Zhou, X, Tsurutani BT. 2001. Interplanetary shock triggering of nightside geomagnetic activity: Substorms, pseudobreakups, and quiescent events. J Geophys Res Space Phys 106: 18957–18967. https://doi.org/10.1029/2000JA003028. [Google Scholar]
- Zou, Y, Shin O, Gjerloev JW, Anderson BJ, Waters CL, et al. 2025. Are supersubstorms substorms? Extreme nightside auroral electrojet activities during the May 2024 geomagnetic storm. J Geophys Res Space Phys 130: e2024JA033303. https://doi.org/10.1029/2024JA033303. [Google Scholar]
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