TY - JOUR
T1 - The Ionosphere at Middle and Low Latitudes Under Geomagnetic Quiet Time of December 2019
AU - Kuai, Jiawei
AU - Li, Qiaoling
AU - Zhong, Jiahao
AU - Zhou, Xu
AU - Liu, Libo
AU - Yoshikawa, Akimasa
AU - Hu, Lianhuan
AU - Xie, Haiyong
AU - Huang, Chaoyan
AU - Yu, Xumin
AU - Wan, Xin
AU - Cui, Jun
N1 - Funding Information:
This research is supported by the Strategic Priority Research Program of Chinese Academy of Sciences (XDB41000000), the National Natural Science Foundation of China (41804153, 41804150, 42030202), the Natural Science Foundation of Jiangsu Province (No. BK20180445), Guangdong Basic and Applied Basic Research Foundation (2021A1515011216, 2020A1515110242), the Joint Open Fund of Mengcheng National Geophysical Observatory (No. MENGO‐202018), China Postdoctoral Science Foundation (2020M683025), the Fundamental Research Funds for the Central Universities, the Opening Funding of Chinese Academy of Sciences dedicated for the Chinese Meridian Project, and the Open Research Project of Large Research Infrastructures of CAS—“Study on the interaction between low/mid‐latitude atmosphere and ionosphere based on the Chinese Meridian Project.” Project Supported by the Specialized Research Fund for State Key Laboratories. A. Yoshikawa was also supported by JSPS KAKENHI Grant Number JP20H01961. C. Huang was also supported by the National Key Laboratory Foundation (Contract No. 6142411193114). The authors acknowledge the use of data from the Chinese Meridian Project. We also appreciate one of the anonymous reviewers for his/her great effort in improving this work.
Publisher Copyright:
© 2021. American Geophysical Union. All Rights Reserved.
PY - 2021/6
Y1 - 2021/6
N2 - The ionospheric electron density shows remarkable day-to-day variability due to solar radiance, geomagnetic activity and lower atmosphere forcing. In this report, we investigated the ionospheric variations at middle and low latitudes during a period under geomagnetic quiet time (Kpmax = 1.7) from November 30 to December 8, 2019. During the quiescent period, the ionosphere is not undisturbed as expected in the Asian-Australian and the American sectors. Total electron content (TEC) has multiple prominent enhancements at middle and low latitudes in the two sectors, and TEC depletions also occur repeatedly in the Asian-Australian sector. The low-latitude electric fields vary significantly, which is likely to be modulated by the notably changing tides in the mesosphere and lower thermosphere region. It is worth noting that the variations of TEC and the electric fields are not consistent in the two sectors, particularly on December 4–6. Further investigation reveals that the increase in TEC depends on altitude. The TEC enhancements are mainly contributed by the altitude below 500 km in both two sectors, which indirectly reflects that the driving sources may come from the lower atmosphere. Especially, a mid-latitude band structure continuously appears at all local times in the North American sector on December 6–8, which is also mainly contributed by the altitude below 500 km.
AB - The ionospheric electron density shows remarkable day-to-day variability due to solar radiance, geomagnetic activity and lower atmosphere forcing. In this report, we investigated the ionospheric variations at middle and low latitudes during a period under geomagnetic quiet time (Kpmax = 1.7) from November 30 to December 8, 2019. During the quiescent period, the ionosphere is not undisturbed as expected in the Asian-Australian and the American sectors. Total electron content (TEC) has multiple prominent enhancements at middle and low latitudes in the two sectors, and TEC depletions also occur repeatedly in the Asian-Australian sector. The low-latitude electric fields vary significantly, which is likely to be modulated by the notably changing tides in the mesosphere and lower thermosphere region. It is worth noting that the variations of TEC and the electric fields are not consistent in the two sectors, particularly on December 4–6. Further investigation reveals that the increase in TEC depends on altitude. The TEC enhancements are mainly contributed by the altitude below 500 km in both two sectors, which indirectly reflects that the driving sources may come from the lower atmosphere. Especially, a mid-latitude band structure continuously appears at all local times in the North American sector on December 6–8, which is also mainly contributed by the altitude below 500 km.
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U2 - 10.1029/2020JA028964
DO - 10.1029/2020JA028964
M3 - Article
AN - SCOPUS:85110626599
SN - 2169-9380
VL - 126
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 6
M1 - e2020JA028964
ER -