Articles | Volume 35, issue 3
https://doi.org/10.5194/angeo-35-763-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-35-763-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Regular paper
| 
22 Jun 2017
Regular paper |
| 22 Jun 2017
Features of 3–7-day planetary-wave-type oscillations in F-layer vertical drift and equatorial spread F observed over two low-latitude stations in China
Zhengping Zhu
CORRESPONDING AUTHOR
College of Electronics and Information Engineering, South-Central
University for Nationalities, Wuhan 430074, China
Weihua Luo
College of Electronics and Information Engineering, South-Central
University for Nationalities, Wuhan 430074, China
Jiaping Lan
College of Electronics and Information Engineering, South-Central
University for Nationalities, Wuhan 430074, China
Shanshan Chang
College of Electronics and Information Engineering, South-Central
University for Nationalities, Wuhan 430074, China
Related authors
Weihua Luo, Chao Xiong, Zhengping Zhu, Shanshan Chang, and Xiao Yu
Ann. Geophys. Discuss., https://doi.org/10.5194/angeo-2019-128, https://doi.org/10.5194/angeo-2019-128, 2019
Manuscript not accepted for further review
Short summary
Short summary
The plasma bubbles and blobs were recorded on two successive days. The interesting is that one of the event occured in a quiet day, and the other in the main phase of a storm. The latitudinal variations of electron density at low- and middle ionosphere were used to analyze the physical factors leading to the variations in the F region and the occurrence of plasma bubbles and blobs. The work would help to understand the dominant factor accounting for the day-to-day occurrence of irregularities.
Weihua Luo, Chao Xiong, Zhengping Zhu, Shanshan Chang, and Xiao Yu
Ann. Geophys. Discuss., https://doi.org/10.5194/angeo-2019-128, https://doi.org/10.5194/angeo-2019-128, 2019
Manuscript not accepted for further review
Short summary
Short summary
The plasma bubbles and blobs were recorded on two successive days. The interesting is that one of the event occured in a quiet day, and the other in the main phase of a storm. The latitudinal variations of electron density at low- and middle ionosphere were used to analyze the physical factors leading to the variations in the F region and the occurrence of plasma bubbles and blobs. The work would help to understand the dominant factor accounting for the day-to-day occurrence of irregularities.
S. S. Chang, B. B. Ni, J. Bortnik, C. Zhou, Z. Y. Zhao, J. X. Li, and X. D. Gu
Ann. Geophys., 32, 507–518, https://doi.org/10.5194/angeo-32-507-2014, https://doi.org/10.5194/angeo-32-507-2014, 2014
J. J. Zhao, C. Zhou, G. B. Yang, C. H. Jiang, S. S. Chang, P. Zhu, X. D. Gu, B. B. Ni, and Z. Y. Zhao
Ann. Geophys., 32, 465–472, https://doi.org/10.5194/angeo-32-465-2014, https://doi.org/10.5194/angeo-32-465-2014, 2014
Short summary
Features of planetary waves in Chinese low-latitude regions are investigated. Planetary waves are observed in both MLT winds and ionospheric vertical drifts. ESF occurrence is with the uplift of the F layer caused by PRE, and a delay of about 6 days is observed for planetary waves propagating from the lower atmosphere to the ionosphere. This investigation contributes to the understanding of atmosphere–ionosphere coupling processes and the effects of planetary waves on ESF.
Features of planetary waves in Chinese low-latitude regions are investigated. Planetary waves...
