Impact of two severe geomagnetic storms on the ionosphere over Indian longitude sector during March-April 2023

被引:8
|
作者
Rajana, Siva Sai Kumar [1 ,2 ]
Panda, Sampad Kumar [1 ]
Jade, Sridevi [2 ]
Vivek, Chiranjeevi G. [2 ]
Upadhayaya, A. K. [3 ]
Bhardwaj, Arti [3 ,4 ]
Jorphail, Sonam [5 ]
Seemala, Gopi Krishna [6 ]
机构
[1] Koneru Lakshmaiah Educ Fdn KLEF, Ctr Atmospher Sci, Dept Elect & Commun Engn, Vaddeswaram 522302, Andhra Pradesh, India
[2] CSIR Fourth Paradigm Inst CSIR 4PI, Bangalore 560037, India
[3] CSIR Natl Phys Lab CSIR NPL, Environm Sci & Biomed Metrol Div, New Delhi 110012, India
[4] Acad Sci & Innovat Res AcSIR, CSIR Natl Phys Lab Campus, New Delhi 110012, India
[5] Indian Inst Astrophys IIA, Indian Astron Observ, Leh 194101, India
[6] Indian Inst Geomagnetism IIG, Navi Mumbai 410218, India
关键词
Geomagnetic storm; Ionosphere; Global navigation satellite system; Space weather; Total electron content; Rate of TEC index; MIDDLE LATITUDES; ZONAL DRIFT; EQUATORIAL; PLASMA; IRREGULARITIES; AFRICAN;
D O I
10.1007/s10509-024-04268-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigated the ionosphere response to the two severe geomagnetic storms in the ascending phase of solar cycle 25 which occurred during the 23-24 March 2023 (SYM-Hmin = -169 nT) and 23-24 April 2023 (SYM-Hmin = -233 nT) using a latitudinally aligned dense network of Global Navigation Satellite System (GNSS) receivers, magnetometers, and digisonde along the Indian longitude sector. The significant variations in TEC during the storm's main and recovery phases are mainly linked to the influence of westward Disturbance Dynamo Electric Fields (DDEFs). During the initial phase of the March 23-24 geomagnetic storm, no changes in daytime TEC were observed, despite the storm occurring at noon time with a southward IMF Bz due to the influence of electron density in the top side ionosphere. Furthermore, both pre-reversal enhancement (PRE) and ionosphere irregularities are suppressed within two hours of their onset during the main phase of the March 23-24 storm, owing to the westward transition of zonal electric fields from an eastward direction. During the recovery phase of both storms, a daytime positive storm effect is observed over the dip equatorial region, while the beyond equatorial ionization anomaly (EIA) and mid-latitude regions perceived a negative ionospheric storm effect. This phenomenon is attributed to the influence of the dominant westward DDEFs during the period. Moreover, these DDEFs effectively inhibited the equinoctial manifestation of PRE effects and post-sunset ionospheric irregularities during the recovery phase of both storms. These findings are further confirmed with supporting information from TEC recorded by Swarm satellites, model-derived ionospheric electric fields, and thermospheric O/N2. The results from this study may advance the understanding of ionospheric response to severe geomagnetic storms under the prevailing westward DDEFs during the dayside recovery phase, complementing the global efforts for more reliable space weather modeling and prediction services.
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页数:20
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