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Auroral activity observed from unusual latitudes in China and its underlying significance

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    1. Spectacular auroras were spotted at unusual latitudes in China during a severe geomagnetic storm.

      CN-DARN reveals the link of auroral intensification to dawnside subauroral polarization (SAPS) streams.

      CN-DARN observed high-speed ionospheric irregularities driven by dawnside SAPS invading China’s airspace.

  • Auroras have been observed at unusual latitudes of China over the past couple of years, which may be a direct result of the north magnetic pole’s drift and intense solar activity. However, the specific impact on the Asian space environment remains unknown. Here, we present auroral activities recorded in southern Inner Mongolia (~37.2° N in magnetic latitude) and the resulting ionospheric environmental changes detected by the Chinese Dual Auroral Radar Network (CN-DARN) during a recent severe geomagnetic storm. Leveraging the wide spatial coverage and continuous high time resolution monitoring capabilities of the CN-DARN, comprehensive analysis of ground-based and space-based multi-source data reveals that CN-DARN has captured the spatiotemporal evolution characteristics of dawnside subauroral polarization streams (SAPS). The study identifies a direct link between auroral intensification and dawnside SAPS acceleration for the first time, establishing a mechanistic connection between auroral activity and ionospheric convection dynamics in subauroral region. Moreover, the observations show that the ionospheric irregularities with high velocity of 1,000 m/s induced by the dawnside SAPS have propagated to Mohe (~ 48.6° N in magnetic latitude), the northernmost region of China. The research also reveals that intense auroral particle precipitation caused severe degradation of high-frequency (HF) communications in the Asian region. This study represents the first comprehensive investigation of auroral activity observed at unusual latitudes of China, unraveling the impact of auroral activities on the ionospheric environment of Asian mid-to-high latitudes. It also showcases the critical capabilities of the Chinese Meridian Project in addressing space environmental challenges of Asia.
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  • [1] Akasofu S.I. (1966). The auroral oval, the auroral substorm, and their relations with the internal structure of the magnetosphere. Planet. Space Sci. 14:587−595. DOI:10.1016/0032-0633(66)90043-2

    View in Article CrossRef Google Scholar

    [2] Kataoka R., Reddy S.A., Nakano S., et al. (2024). Extended magenta aurora as revealed by citizen science. Sci. Rep. 14:25849. DOI:10.1038/s41598-024-75184-9

    View in Article CrossRef Google Scholar

    [3] Livermore P.W., Finlay C.C. and Bayliff M (2020). Recent north magnetic pole acceleration towards Siberia caused by flux lobe elongation. Nat. Geosci. 13:387-391. DOI: 10.1038/s41561-020-0570-9

    View in Article Google Scholar

    [4] Ross, J.C. (1834). On the position of the North Magnetic Pole. Phil. Trans. R. Soc. 124:47−52. DOI:10.1098/rspl.1830.0139

    View in Article CrossRef Google Scholar

    [5] Barraclough D.R., and Malin S.R.C. (1981). 150 years of the North Magnetic Pole. Nature 291:377−377. DOI:10.1038/291377a0

    View in Article CrossRef Google Scholar

    [6] Chulliat A., Brown W., Alken P., et al. (2020). The US/UK world magnetic model for 2020-2025 : Tech. Rep. DOI: 10.25923/ytk1-yx35

    View in Article Google Scholar

    [7] Tsyganenko N.A. (2019). Secular drift of the Auroral ovals: How fast do they actually move. Geophys. Res. Lett. 46:3017−3023. DOI:10.1029/2019GL082159

    View in Article CrossRef Google Scholar

    [8] Zhang J., Lan A., Yan J., et al. (2024). Development of the Chinese Dual Auroral Radar Network and preliminary results. Space Weather 22:e2024SW004131. DOI:10.1029/2024SW004131

    View in Article CrossRef Google Scholar

    [9] Wang C., Xu J., Chen Z., et al. (2024). China's ground-based space environment monitoring network—Chinese Meridian Project (CMP). Space Weather 22:e2024SW003972. DOI:10.1029/2024SW003972

    View in Article CrossRef Google Scholar

    [10] Chisham G., Lester M., Milan S.E., et al. (2007). A decade of the Super Dual Auroral Radar Network (SuperDARN): scientific achievements, new techniques and future directions. Surv. Geophys. 28:33−109. DOI:10.1007/s10712-007-9017-8

    View in Article CrossRef Google Scholar

    [11] Nishitani N., Ruohoniemi J.M., Lester M., et al. (2019). Review of the accomplishments of mid-latitude Super Dual Auroral Radar Network (SuperDARN) HF radars. Prog. Earth Planet. Sci. 6:27. DOI:10.1186/s40645-019-0270-5

    View in Article CrossRef Google Scholar

    [12] Greenwald R.A., Baker K.B., Hutchins R.A., et al. (1985). An HF phased-array radar for studying small-scale structure in the high-latitude ionosphere. Radio Science 20:63−79. DOI:10.1029/RS020i001p00063

    View in Article CrossRef Google Scholar

    [13] Shepherd S.G. (2014). Altitude‐adjusted corrected geomagnetic coordinates: Definition and functional approximations. J. Geophys. Res. 119:7501−7521. DOI:10.1002/2014JA020264

    View in Article CrossRef Google Scholar

    [14] Jonkers A.R.T., Jackson A., and Murray A. (2003). Four centuries of geomagnetic data from historical records. Rev. Geophys. 41. DOI: 10.1029/2002RG000115

    View in Article Google Scholar

    [15] Sotirelis T., Korth H., Hsieh S.-Y., et al. (2013). Empirical relationship between electron precipitation and far-ultraviolet auroral emissions from DMSP observations. J. Geophys. Res. 118:1203−1209. DOI:10.1002/jgra.50157

    View in Article CrossRef Google Scholar

    [16] Wang X., Zhang X., Wang J., et al. (2023). Plasma analyzer for the Chinese FY-3E satellite: In-orbit performance and ground calibration. Atmosphere 14:1665. DOI:10.3390/atmos14111665

    View in Article CrossRef Google Scholar

    [17] Ruohoniemi J., and Baker K. (1998). Large‐scale imaging of high‐latitude convection with Super Dual Auroral Radar Network HF radar observations. J. Geophys. Res. 103:20797−20811. DOI:10.1029/98JA01288

    View in Article CrossRef Google Scholar

    [18] Zhang J.J., Wang W., Wang C., et al. (2020). First observation of ionospheric convection from the Jiamusi HF radar during a strong geomagnetic storm. Earth Space Sci. 7:e2019EA000911. DOI:10.1029/2019ea000911

    View in Article CrossRef Google Scholar

    [19] Wanliss J.A., and Showalter K.M. (2006). High-resolution global storm index: Dst versus SYM-H. J. Geophys. Res. 111:A02202. DOI: 10.1029/2005ja011034

    View in Article Google Scholar

    [20] Matzka J., Stolle C., Yamazaki Y., et al. (2021). The geomagnetic Kp index and derived indices of geomagnetic activity. Space Weather 19:e2020SW002641. DOI:10.1029/2020SW002641

    View in Article CrossRef Google Scholar

    [21] Kataoka R., Miyoshi Y., Shiokawa K., et al. (2024). Magnetic storm-time red aurora as seen from Hokkaido, Japan on 1 December 2023 associated with high-density solar wind. Geophys. Res. Lett. 51:e2024GL108778. DOI:10.1029/2024GL108778

    View in Article CrossRef Google Scholar

    [22] Shiokaw K., Meng C.-I., Reeves G.D., et al. (1997). A multievent study of broadband electrons observed by the DMSP satellites and their relation to red aurora observed at midlatitude stations. J. Geophys. Res. 102:14237−14253. DOI:10.1029/97JA00741

    View in Article CrossRef Google Scholar

    [23] Foster J.C., Erickson P.J., Nishimura Y., et al. (2024). Imaging the May 2024 extreme aurora with ionospheric total electron content. Geophys. Res. Lett. 51:e2024GL111981. DOI:10.1029/2024GL111981

    View in Article CrossRef Google Scholar

    [24] Foster J.C., and Vo H.B. (2002). Average characteristics and activity dependence of the subauroral polarization stream. J. Geophys. Res. 107:1475. DOI: 10.1029/2002ja009409

    View in Article Google Scholar

    [25] Anderson P.C., Hanson W.B., Heelis R.A., et al. (1993). A proposed production model of rapid subauroral ion drifts and their relationship to substorm evolution. J. Geophys. Res. 98:6069−6078. DOI:10.1029/92JA01975

    View in Article CrossRef Google Scholar

    [26] Califf S., Li X., Wolf R.A., et al. (2016). Large-amplitude electric fields in the inner magnetosphere: Van Allen Probes observations of subauroral polarization streams. J. Geophys. Res. 121:5294−5306. DOI:10.1002/2015JA022252

    View in Article CrossRef Google Scholar

    [27] Horvath I., and Lovell B.C. (2022). Newly formed dawnside, duskside, and nightside subauroral flows developed during magnetically active times. J. Geophys. Res. 127:e2021JA030215. DOI:10.1029/2021JA030215

    View in Article CrossRef Google Scholar

    [28] Lin D., Wang W., Merkin V.G., et al. (2022). Origin of dawnside subauroral polarization streams during major geomagnetic storms. AGU Adv. 3:e2022AV000708. DOI:10.1029/2022AV000708

    View in Article CrossRef Google Scholar

    [29] Vasyliunas V.M. (1970). Mathematical models of magnetospheric convection and its coupling to the ionosphere. In B.M. McCormac (ed). Particles and Fields in the Magnetosphere. Dordrecht. DOI:10.1007/978-94-010-3284-1_6

    View in Article Google Scholar

    [30] Thomas E.G., and Shepherd S.G. (2018). Statistical patterns of ionospheric convection derived from mid-latitude, high-latitude, and polar SuperDARN HF radar observations. J. Geophys. Res. 123:3196−3216. DOI:10.1002/2018JA025280

    View in Article CrossRef Google Scholar

    [31] Nielsen E., and Axford W.I. (1977). Small scale auroral absorption events associated with substorms. Nature 267:502−504. DOI:10.1038/267502a0

    View in Article CrossRef Google Scholar

    [32] Mishin E., and Streltsov A. (2021). Mesoscale and small-scale structure of the subauroral geospace. In Ionosphere Dynamics and Applications, pp:139-158. DOI: 10.1002/9781119815617.ch8

    View in Article Google Scholar

  • Cite this article:

    Zhang J., Deng X., Xu J., et al. (2026). Auroral activity observed from unusual latitudes in China and its underlying significance. The Innovation Geoscience 4:100197. https://doi.org/10.59717/j.xinn-geo.2026.100197
    Zhang J., Deng X., Xu J., et al. (2026). Auroral activity observed from unusual latitudes in China and its underlying significance. The Innovation Geoscience 4:100197. https://doi.org/10.59717/j.xinn-geo.2026.100197

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