Equatorial and low-latitude ionospheric response to the 17–18 March 2015 great storm over Southeast Asia longitude sector

Equatorial and low-latitude ionospheric response to the 17–18 March 2015 great storm over Southeast Asia longitude sector

©2017. American Geophysical Union. All Rights Reserved. This study mainly investigates equatorial and low-latitude ionospheric response to a great geomagnetic storm that occurred on 17 March 2015. We found that there were some interesting ionospheric phenomena, e.g., short-term ionospheric positive...

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Bibliographic Details
Main Authors: Chunhua Jiang, Guobin Yang, Jing Liu, Tatsuhiro Yokoyama, Tongxin Liu, Ting Lan, Chen Zhou, Yuannong Zhang, Zhengyu Zhao, Tharadol Komolmis, Pornchai Supnithi, Clara Y. Yatini
Format: Journal
Published: 2018
Subjects:
Agricultural and Biological Sciences
Earth and Planetary Sciences
Environmental Science
Online Access:https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85019950142&origin=inward
http://cmuir.cmu.ac.th/jspui/handle/6653943832/56525
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Institution: Chiang Mai University
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Summary:©2017. American Geophysical Union. All Rights Reserved. This study mainly investigates equatorial and low-latitude ionospheric response to a great geomagnetic storm that occurred on 17 March 2015. We found that there were some interesting ionospheric phenomena, e.g., short-term ionospheric positive effect, daytime spread F, and morning Equatorial Ionization Anomaly (EIA) in the topside ionosphere, emerged at equatorial and low-latitude region along the longitude of about 100°E. Ground-based ionosondes and in situ satellite (Swarm) were utilized to study the possible mechanisms for these ionospheric phenomena. We found that vertical downward transport of plasma or neutral induced by traveling ionospheric disturbances (TIDs) or traveling atmospheric disturbances (TADs) might make a contribution to the short-term ionospheric positive effect at the main stage of this great storm. Additionally, results suggested that the occurrence of daytime spread F at low latitudes might be due to the diffusion of equatorial ionospheric irregularities in the topside ionosphere along geomagnetic field lines. Moreover, observational evidence shows that TIDs also might be the main driver for morning EIA-like feature recorded by Swarm B satellite in the topside ionosphere. These ionospheric phenomena mentioned above could make us gain a better understanding of ionospheric storm effects at equatorial and low-latitude region.

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