Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456798/198
Title: An experimental investigation into the possible connections between the zonal neutral wind speeds and equatorial plasma bubble drift velocities over the African equatorial region
Authors: Okoh, D.I.
Rabiu, A.B.
Shiokawa, K.
Otsuka, Y.
Wu, Q.
Seemala, G.K.
Katamzi-Joseph, Z. T.
Keywords: Neutral wind, Plasma bubble, Zonal speed, Airglow, FPI All-sky imager
Issue Date: 2021
Citation: Journal of Atmospheric and Solar-Terrestrial Physics, Volume 220, 1 September 2021, 105663,https://doi.org/10.1016/j.jastp.2021.105663
Abstract: There is increasing interest to understand thermospheric neutral wind and ionized plasma coupling, especially by using empirical observations. This is the first study that reports simultaneous measurements of thermospheric neutral wind and equatorial plasma bubble (EPB) speeds over the African equatorial region. Neutral wind speeds were obtained using a Fabry-Perot interferometer (FPI), while EPB speeds were obtained using an all-sky optical imager. Both instruments are co-located in Abuja (Geographic: 8.99◦N, 7.38◦E; Geomagnetic: 1.60◦S). Data for 11 nights of coincident neutral wind and EPB speed observations were used. The neutral wind speeds were in the range of about �� 30 to 300 m/s, while EPB speeds were in the range of about 15–400 m/s. The speeds of both neutral winds and EPBs were generally observed to be faster during the early night hours and to slow down towards midnight. In some instances, the neutral wind and EPB speeds were comparable, an observation that is in agreement with full development of the F region dynamo. There were also instances in which the EPBs were faster or slower than the neutral winds. In one of the nights, a southward turning of the IMF-Bz was observed to cause a sudden increase in the EPB speed. For some nights, the neutral winds were faster than the EPBs during earlier hours of the nights, and the disparity reduced during the later hours of the nights. This was attributed to the possibility that the F region dynamo was yet to be fully developed during the earlier hours.
URI: http://library.iigm.res.in:8080/xmlui/handle/123456798/198
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