For the two global solutions we find that as expected,
the horizontal components are less noisy for white and
flicker noise magnitudes than the vertical components by a
factor of 2–3. The east components, also as expected, are
somewhat noisier than the north components because of no
(SOPAC) or incomplete (JPL) integer-cycle phase ambiguity
resolution in the global solutions. The white noise amplitudes
are about 2 times larger in the JPL global solutions
compared to the SOPAC global solutions, in all three
components, while the flicker noise amplitudes are only
marginally larger. The white noise amplitude differences are
probably due to processing strategies (what these may be are
beyond the scope of this paper), while the comparable flicker
noise amplitudes may reflect a common physical basis, such
as seasonal atmospheric mass distributions [e.g
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