Sentence examples for maximum latitude of from inspiring English sources

The maximum latitude of scintillation observed at Pontianak and Bandung stations is plotted as a function of the peak h'F, maximum V u, duration of PRE and integral of V u measured at Bac Lieu.

The first (group 1) is used for comparison of peak h'F, maximum V u, duration of PRE and integral of V u obtained from the Chumphon ionosonde with the maximum latitude of scintillation observed by the GPS receivers at Kototabang and Bandung between 18 00 and 22 00 LT.

Thus, we can reasonably assert that the maximum latitudes of scintillation are positively correlated with the peak h'F, maximum V u and integral of V u, and that there is no correlation between the maximum latitude of scintillation and the duration of PRE.

Statistically, our finding of good correlation of the maximum latitude of scintillation versus the peak h'F and magnitude of PRE reaffirms that the altitude of the F layer and V u at the initial growth of plasma bubble is important in deciding how far plasma bubbles will extend.

Figure 3a d shows the latitude of scintillation furthest away from the magnetic equator (the maximum latitude of scintillation) during 18 00 22 00 LT as a function of the peak h'F, maximum V u, duration of PRE and integral of V u, respectively, obtained from group 1 (ionosonde at Chumphon and GPS scintillation at Bandung and Pontianak).

Actually, Valladares et al. (2004) have reported that the maximum latitudes of scintillation are mostly located at lower latitudes than the boundary of the EIA crest at the American longitudinal sector.

From the figure, most of the maximum latitudes of the scintillation during the observation period are found to distribute from 0°S to 10°S corresponding to 10°S 20°S magnetic latitudes in the Southeast Asian longitudinal sector.

Cross-correlation coefficients for the relations of the maximum latitudes of scintillation to the peak h'F, maximum V u, duration of PRE and integral of V u for group 2 are 0.4, 0.3, 0.02 and 0.3, respectively.

The cross-correlation coefficients for the relations of the maximum latitudes of scintillation to the peak h'F, maximum V u, duration of PRE and integral of V u are 0.6, 0.5, 0.05 and 0.5, respectively.

Fig. 3 Relations between maximum latitudes of scintillation for group 1 and a peak h'F, b maximum upward E × B drift, c duration of PRE and d the integral of upward E × B drift.

Most of the maximum latitudes of scintillation occur in the range between 0°S 10°S, with the peak h'F varying with 250 450 km, maximum V u varying with 10 60 m/s and integral of V u varying with 50 250 m/s.