On the Nocturnal Downward and Westward Equatorial Ionospheric Plasma Drifts During the 17 March 2015 Geomagnetic Storm

2018 ◽  
Vol 123 (2) ◽  
pp. 1618-1626 ◽  
Author(s):  
Mala S. Bagiya ◽  
Geeta Vichare ◽  
A. K. Sinha ◽  
S. Sripathi
1971 ◽  
Vol 19 (3) ◽  
pp. 345-355 ◽  
Author(s):  
K. Knott ◽  
G. Brommundt ◽  
G. Schumann

2021 ◽  
Vol 14 (1) ◽  
pp. 38
Author(s):  
Juan Carlos Valdés-Abreu ◽  
Marcos A. Díaz ◽  
Juan Carlos Báez ◽  
Yohadne Stable-Sánchez

In this work, we present the positioning error analysis of the 12 May 2021 moderate geomagnetic storm. The storm happened during spring in the northern hemisphere (fall in the south). We selected 868 GNSS stations around the globe to study the ionospheric and the apparent position variations. We compared the day of the storm with the three previous days. The analysis shows the global impact of the storm. In the quiet days, 93% of the stations had 3D errors less than 10 cm, while during the storm, only 41% kept this level of accuracy. The higher impact was over the Up component. Although the stations have algorithms to correct ionospheric disturbances, the inaccuracies lasted for nine hours. The most severe effects on the positioning errors were noticed in the South American sector. More than 60% of the perturbed stations were located in this region. We also studied the effects produced by two other similar geomagnetic storms that occurred on 27 March 2017 and on 5 August 2019. The comparison of the storms shows that the effects on position inaccuracies are not directly deductible neither from the characteristics of geomagnetic storms nor from enhancement and/or variations of the ionospheric plasma.


1974 ◽  
Vol 22 (7) ◽  
pp. 1131-1138 ◽  
Author(s):  
K. Gueth ◽  
H.V. Hoerner ◽  
G. Brommundt

2009 ◽  
Vol 16 (1) ◽  
pp. 123-130 ◽  
Author(s):  
G. S. Tsolis ◽  
T. D. Xenos

Abstract. Ionospheric variability as a result of earthquake events is a confirmed phenomenon as published in various seismo-ionospheric coupling studies. Generally, ionospheric variations resulting from earthquake activity are much weaker than disturbances generated by different sources, e.g. geomagnetic storms. However, geomagnetic storm disturbances exhibit more global behaviour, whereas seismo-ionospheric variations occur only locally in an area that is specified by the magnitude of the earthquake. Cross-correlation coefficient analysis is a technique proposed some years ago, and ensures cancelation of geomagnetic storm variations of the ionospheric plasma, provided that the measurements are taken from stations with similar behaviour in these phenomena. In this paper we will use the aforementioned technique for analyzing data from ionospheric stations in Rome and Athens, and apply it to a series of earthquakes in Greece. Considering the local behaviour of the seismo-ionospheric variations, we expect that the Athens station, which happens to be inside the area affected by the earthquake, will accurately capture the disturbances. Due to its distance from the activity, we also do not expect the Rome station measurements to be affected by the seismic events in Greece. In addition, due to the fact that ionospheric plasma parameters exhibit non-stationary and nonlinear behaviour, we propose a novel signal processing technique known as the Hilbert-Huang transform in order to denoise the data before we calculate the cross-correlation coefficient of the two signals. Results from our analysis are in accordance with previously-conducted studies covering the same topic, clearly demonstrating that there are ionospheric precursors 1 to 7 days prior to strong seismic events as well as 1 to 2 days following such events.


BIBECHANA ◽  
2016 ◽  
Vol 14 ◽  
pp. 1-8 ◽  
Author(s):  
Narayan P Chapagain

This study presents the experimental results of the equatorial ionospheric plasma drift zonal velocity obtained from Incoherent Scatter Radar (ISR) observations for 6 selective days in 2011 from Jicamarca, Peru. Our results indicate that the daytime drifts are westward with peak values mostly below ~50 m/s, while the night time drifts velocities are eastward, with a maximum value up to 120 m/s at around local midnight hours. The drift velocity decreases during post-midnight hours and starts to reverse westward in early morning hours. Our plasma drifts results are in good agreement with results from previous radar studies and other measurement techniques.  BIBECHANA 14 (2017)1-8  


2019 ◽  
Vol 124 (8) ◽  
pp. 7123-7139 ◽  
Author(s):  
Chigomezyo M. Ngwira ◽  
John‐Bosco Habarulema ◽  
Elvira Astafyeva ◽  
Endawoke Yizengaw ◽  
Olusegun F. Jonah ◽  
...  

2016 ◽  
Vol 121 (8) ◽  
pp. 7961-7973 ◽  
Author(s):  
Chao‐Song Huang ◽  
Gordon R. Wilson ◽  
Marc R. Hairston ◽  
Yongliang Zhang ◽  
Wenbin Wang ◽  
...  

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