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In this case, the longitude of the observed h'F and V u is different from the longitude where the plasma bubble occurs.
To estimate the observed wave velocity, we took zonal and meridional cross sections (keograms) of the 630-nm airglow images at a fixed latitude and longitude where the wave was clearly seen.
In addition to GPS, there are other empirical models that are very important for estimating ionospheric characteristics of a specific region at a specific time, latitude, and longitude, where measured values are not available.
The scattered crosses show the location of the ICAS cloud top at the respective longitude, where black crosses represent cloud top of the first layer and red crosses represent cloud top of the second layer.
To see the characteristics of the amplitude more quantitatively, Figure 6 shows the latitudinal and the local time dependence of the amplitude of the zonal component around −130° of the dipole longitude, where the dipole latitude at the dip equator is near 0°.
Besides a dependence on PSSR strength, other possible factors include (1) a possible D2D variability in seeding, and (2) a variability in whether an upwelling has been imprinted onto the bottomside of the equatorial F layer by the time of SS F. An EPB would likely be launched at a longitude where SS F intercepts an upwelling.
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He found that EPBs developed in the post-sunset sector, at longitudes where upwellings were observed during the previous orbit, in the pre-sunset sector.
Following the prompt penetration electric field (PPE) at ∼0605 UT, equatorial electrojet (EEJ) enhances by ∼55 nT over 75±± 3oE longitudes where main phase step-I is coincided with local noon.
From this plot we can see that TEC reductions (marked by blue) were detected at latitudes higher than ~ 12 13° N, around the longitudes where the daytime F-region irregularities were observed.
The coupling hypothesis is supported by the larger bumps in the non-winter ({varPsi }_{N}) curves at UT between 0 and 15, corresponding to longitudes where the dip equator is in the Northern hemisphere and to seasons when the Sq current system is largest and most prone to interact with the EEJ.
And it didn't have to do with the latitude and the longitude of where I was.
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