3. Method of Data Processing

[10]  The standard GPS technology provides a means for calculation of slant TEC Is along line of sight (LOS) between GPS satellite and receiver based on phase measurements at each of spaced two-frequency GPS receivers. Data of phase measurements are contained in the RINEX files, available at ftp://sopac.ucsd.edu/pub/.

[11]  A method of the TEC calculating was specified and validated in a series of publications [e.g., Afraimovich, 0]. We reproduce here only the final formula for phase measurements:

eq001.gif(1)

where L1 l1 and L2 l2 are additional paths of the radio signal caused by the phase delay in the ionosphere [m]; L1 and L2 represent the number of phase rotations at the frequencies f1 and f2; l1 and l2 stand for the corresponding wavelengths [m]; const is the unknown initial phase ambiguity [m]; and nL are the errors in determining the phase path [m].

[12]  Phase measurements in the GPS can be performed with a high degree of accuracy corresponding to the error of TEC determination of at least 1013 m-2 when averaged on a 30-s time interval, with some uncertainty of the initial value of TEC, however. Filtered out in the range of periods 30-60 min, the standard deviation of TEC series is not worse than 0.2 times1013 m-2.

[13]  To normalize the response amplitude, we have converted "slant'' TEC Is to an equivalent "vertical'' value I [Klobuchar, 1986]:

eq002.gif(2)

where Rz is the Earth's radius, h max=300 km is the height of the F2 -layer maximum, and qs is the elevations of the LOS.

[14]  Then we selected continuous TEC series I(t) with a duration of about 2 hours from the obtained TEC data so that we had 22 overlapping time intervals with a 1-hour shift for the day. We used specified threshold of 30o for elevations qs to the GPS satellites. I(t) series for all GPS sites in the region under consideration and for all visible satellites were filtered in the timescale of 20-60 min and 2-10 min using running average filtering. Standard deviation s of TEC variations was calculated for each series. The s values were averaged on all series; thus we got for each 2 hours time interval the mean absolute values dI = [S si]/m, where i =1, 2, ldots, m; m is a total number of series. The dI represents an absolute value of the amplitude of TEC variations. The distribution of the number of series Im over days is shown in Table 1. The total number of analyzing series is about 106.

[15]  The relative amplitude dI/I0 is determined by normalization of the dI to the background I0 value, where I0 is the absolute vertical TEC obtained with 2-hour time resolution from the global TEC maps in the IONEX format (the so-called global ionospheric maps (GIM) [Mannucci et al., 1998]). The spatial range of GIM is 0-360o in longitude and 90oS-90oN in latitude. The spatial resolution is restricted by the dimensions of an elementary GIM cell ( 5o and 2.5o in longitude and latitude, respectively). For the normalization, the I0 values are used for the GIM cell closest to the GPS station used for determination of the dI value.

[16]  The series Im, dIm, and dI/Im were averaged over the chosen area to obtain the mean values of TEC langle Irangle, of the absolute amplitude langle dIrangle and of the relative amplitude langle dI/Irangle of TEC variations in the period ranges of MS and IS ionospheric irregularities.


AGU

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