After bin averaging the media corrected crossover differences (as indicated
above) we examined the 19 sets of DSCs and SSCs shown in Figure 2
(left column for the data, middle for the residuals after
the inversion, right column for the formal data precision (
sd)).
These observations are assumed to be conditioned by geopotential,
one cycle per revolution orbit error (1 cpr), altimeter time-tag,
and (for DSCs) a constant altimeter bias and a possible
geocenter shift (between the two missions applying).
