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In this study, we use the GPS scintillation data to measure the maximum latitudinal extension of the plasma bubble.
In this study, to investigate the effects of PRE on the maximum latitudinal extension of plasma bubbles, we have used two datasets.
As shown in Figs. 3c and 4c, however, there is no correlation between the duration of PRE and the maximum latitudinal extension of scintillations.
We have also found that the maximum latitudinal extension of plasma bubble is well positively correlated with the peak h'F, maximum V u and the integral of V u, but that it is not correlated with the duration of PRE.
The longitudinal difference between the PRE and observed plasma bubble may be responsible for the scatter of the relation between the PRE and maximum latitudinal extension of plasma bubbles.
On the basis of the above results for groups 1 and 2, we find that the peak h'F, maximum V u and integral of V u at the equatorial region are well positively correlated with the maximum latitudinal extension of plasma bubble.
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According to their result, we calculate the upward E × B drift (hereafter denoted as V u) from dh'F/dt when h'F exceeds about 300 km and use the obtained value as a proxy for the eastward E. In this study, we consider that the maximum V u is one of the important parameters for latitudinal extension of plasma bubble.
In addition to the peak h'F and maximum V u, we also consider the duration of PRE as a parameter affecting the latitudinal extension of plasma bubble.
These results indicate that the altitude of the F layer, the maximum V u and the integral of V u at the initial phase of plasma bubble generation strongly control the altitudinal and latitudinal extension of plasma bubble.
Therefore, by the GPS scintillation measurement, latitudinal extension of the plasma bubbles can be observed.
By detecting weak scintillation, we can investigate latitudinal extension of plasma bubble.
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