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"WIDE-LANE" COMBINATION |
This is also sometimes referred to as the "L5" combination.
Instead of subtracting the L2 observation from the L1 observation in metric
units, the phase equations can be differenced ((6.4-3a)
& (6.4-3b)):
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(6.4-16) |
This is known as the "wide-lane" combination because the effective
wavelength of the resultant observable is
0.86 metres. The n5
ambiguity is:
| n5[cycles] = n1 n2 |
Hence n5 is an integer, however each cycle
has a 0.86m wavelength. Eqn (6.4-16) can be converted to metric units through
multiplication with the wavelength
5:
| (6.4-17a) |
or in terms of the L1 ionospheric delay (using eqn (6.4-2)):
| (6.4-17b) |
Hence the L5 ionospheric effect is approximately 1.28 times that affecting
L1 observations (1.28
f1 / f2). However, the noise on
L5 observables is approximately six times (Table
in section 6.4.6) that on L1 observables!
It can be shown that eqn (6.4-17) is the same expression for the L5 observable if constructed from the P1 and P2 pseudo-range observations except that there is no ambiguity term, and the sign of the ionospheric delay is reversed :
| (6.4-17c) |
(Hint: convert eqns (6.4-10) to cycles, difference the
expressions and then scale them back to metric units using
5).
The wide-lane pseudo-range is therefore advanced by the ionosphere
(range too short), while the wide-lane phase is delayed by the
ionosphere (phase-range too long).
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© Chris Rizos, SNAP-UNSW, 1999