• Sorted by Date • Sorted by Last Name of First Author •
Ye, Hailun, Xue, Xianghui, Sun, Yang-Yi, Yu, Tao, Yi, Wen, Wu, Jianfei, Yu, Bingkun, Wang, Jianyuan, Long, Chi, Zhou, Baozhu, Li, Zezhong, Wang, Chong, Chen, Tingdi, and Dou, Xiankang, 2025. Observations of Unusual Postsunrise Interhemispheric Geomagnetic Conjugate Super Plasma Depletions at Midlatitudes During the Recovery Phase of the November 2003 Superstorm. Space Weather, 23(2):2024SW004240, doi:10.1029/2024SW004240.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025SpWea..2304240Y,
author = {{Ye}, Hailun and {Xue}, Xianghui and {Sun}, Yang-Yi and {Yu}, Tao and {Yi}, Wen and {Wu}, Jianfei and {Yu}, Bingkun and {Wang}, Jianyuan and {Long}, Chi and {Zhou}, Baozhu and {Li}, Zezhong and {Wang}, Chong and {Chen}, Tingdi and {Dou}, Xiankang},
title = "{Observations of Unusual Postsunrise Interhemispheric Geomagnetic Conjugate Super Plasma Depletions at Midlatitudes During the Recovery Phase of the November 2003 Superstorm}",
journal = {Space Weather},
keywords = {midlatitude plasma depletions, geomagnetic conjugate, geomagnetic storm recovery phase, eastward electric field, early morning},
year = 2025,
month = feb,
volume = {23},
number = {2},
pages = {2024SW004240},
abstract = "{This study reports an extreme ionospheric plasma depletion event over
the Eastern Pacific from postmidnight to early morning during
the superstorm's recovery phase on 21 November 2003 observed by
the DMSP F13, ROCSAT-1, GRACE, and CHAMP satellites, and two
ground-based GPS receivers. The depletion and its
interhemispheric geomagnetic conjugate effect occurred between
{\ensuremath{\sim}}40{\textdegree}S and 40{\textdegree}N
geomagnetic latitudes. This suggests a possible extremely long-
range flux tube connection with an apex altitude exceeding 6,000
km over the geomagnetic equator. Notably, the observed altitude
for midlatitude depletions of equatorial origin in the morning
is the highest ever reported. Previous studies have primarily
observed the extension of equatorial plasma bubbles to middle
latitudes in the post-sunset hours. The continuous upward
vertical plasma drift, supported by ROCSAT-1 and TIE-GCM
simulations, may drive the unprecedentedly strong latitudinal
extension of these midlatitude plasma depletions in the
midnight-to-morning sector.}",
doi = {10.1029/2024SW004240},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025SpWea..2304240Y},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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