• Sorted by Date • Sorted by Last Name of First Author •
Zhang, Ruilong, Liu, Libo, Li, Wenbo, Du, Rongjin, Wang, Yuzhou, Chen, Yiding, and Le, Huijun, 2026. The Drag of Ionosphere Plasma Drifts on Thermospheric Zonal Winds During the 10–12 May 2024 Superstorm. Geophysical Research Letters, 53(11):e2025GL118472, doi:10.1029/2025GL118472.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2026GeoRL..5318472Z,
author = {{Zhang}, Ruilong and {Liu}, Libo and {Li}, Wenbo and {Du}, Rongjin and {Wang}, Yuzhou and {Chen}, Yiding and {Le}, Huijun},
title = "{The Drag of Ionosphere Plasma Drifts on Thermospheric Zonal Winds During the 10--12 May 2024 Superstorm}",
journal = {\grl},
keywords = {ionosphere plasma drift, thermosphere wind, penetration electric field, ionosphere storm},
year = 2026,
month = jun,
volume = {53},
number = {11},
eid = {e2025GL118472},
pages = {e2025GL118472},
abstract = "{The observations from GRACE-FO and DMSP satellites are utilized to
analyze the ion-neutral interaction near dusk during the 10--12
May 2024 super-storm. The horizontal plasma convection dragged
the anti-sunward wind in the polar cap and sunward winds around
the auroral and subauroral regions during whole storm times. The
strong westward winds were observed below subauroral latitudes
({\ensuremath{\sim}}35{\textdegree}S--45{\textdegree}N Mlat)
after storm onset, and these westward winds disappeared after 23
UT on 10 May. Meanwhile, the penetration of auroral and
subauroral electric fields could induce the westward plasma
drifts in lower latitudes before 23 UT on 10 May. We suggested
that the ion-drag force of the westward penetration plasma drift
is the possible source for the westward disturbance winds below
the subauroral latitudes at 17--23 UT on 10 May. Thus, the
horizontal plasma drifts drag horizontal winds from polar cap to
equator in the main phase, which has been never observed.}",
doi = {10.1029/2025GL118472},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026GeoRL..5318472Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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