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where:
ξ 4 =
f L 1 /
f L 2 ≈−
1
0
.
647 factor (GPS) for relating the ionospheric refraction
on L 4 to L 1 ,
B 4 = λ L 1 B
(
f L 1 ) λ L 2 B
(
f L 2 )
ambiguity parameter with undefined wavelength,
thus defined in length units,
b S
b S , 1
b S , 2
Δ
=
differential inter-frequency hardware delay of the
satellite S in time units,
Δ
b R =
b R , 1
b R , 2 differential inter-frequency hardware delay of the
receiver R in time units.
The ionospheric refraction I in Eqs. 87 and 88 can be related to the VTEC as a
function of the geomagnetic latitude and the sun-fixed longitude in the following
way:
I
= ξ E STEC
(β,
s
) = ξ E F
(
z
)
VTEC
(β,
s
),
(89)
with:
F
(
z
)
mapping function evaluated at zenith distance z ,
β
geomagnetic latitude,
s sun-fixed longitude,
C x
2
f 2
1
ξ E =
0
.
162 m/TECU (GPS).
By substituting Eq. 89 in Eqs. 87 and 88 the ionospheric observable for code and
phase measurements reads
c
b R
b S
P 4 ≈+ ξ 4 ξ E F
(
z
)
VTEC
(β,
s
) +
Δ
Δ
,
(90)
and
L 4 ≈− ξ 4 ξ E F
(
z
)
VTEC
(β,
s
) +
B 4 .
(91)
In Eqs. 90 and 91 , the equation sign '
=
' has been replaced by the approximate equa-
tion sign '
' because of including the simplified single layer assumption. Depending
on the study and whether we want to estimate VTEC on a local, regional or global
basis, VTEC
is represented with an appropriate base-function. As an example
Taylor series expansion can be used for local representation of TEC; B-splines are
very suitable for studying TEC in regional applications, and for global representa-
tion of TEC, spherical harmonics expansion is most commonly used. Here we briefly
discuss the spherical harmonics expansion approach:
(β,
s
)
Global TEC Representation Using Spherical Harmonics Expansion
In order to develop a global ionosphere model, the vertical TEC has to be represented
as a function of longitude, latitude and time, or according to the definition of the
adopted coordinate system given in Sect. 4.3 —as a function of the geomagnetic
latitude
β
and sun-fixed longitude s (Schaer 1999 ):
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