Features of the F3 layer in the low-latitude ionosphere at sunset
The Fâ layer is a common feature within ±10° of the magnetic equatorial ionosphere in the daytime. According to Balan et al. (1998) the Fâ layer occurs mainly during the morning-noon period due to the combined effect of the upward E à B drift and the neutral wind that provides upward plasma drifts at and above the Fâ layer. The Fâ layer occurrence rate is higher in summer and decreases with increasing solar activity. In this study, the characteristic of the sunset Fâ layer is first investigated using a solar cycle of ionosonde data (1995 - 2010) from the magnetic equatorial station at Jicamarca, and compared with the features derived from the four subtropical stations at Sao Luis, Fortaleza, Kwajalein, and Vanimo. Evidence shows that the local time distribution of the occurrence of the Fâ layer can extend to the postsunset time (1800 - 2100 local time). The sunset Fâ layer has a strong seasonal dependence occurring mainly during the summertime. Unlike the daytime Fâ layer, the occurrence of the sunset Fâ layer clearly increases and the virtual height of the bottom side of the Fâ layer statistically increases from 620 to 1000 km with increasing solar activity. In addition, the occurrence of the sunset Fâ layer at the other stations is much less than that at Jicamarca. These features of the dependence on the season, solar activity, and latitude are clearly related to the geomagnetic control of the evening prereversal enhancement of the equatorial zonal electric field and geomagnetic configuration.
document
https://n2t.org/ark:/85065/d7pc33pg
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2011-01-25T00:00:00Z
An edited version of this paper was published by AGU. Copyright 2011 American Geophysical Union.
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