Figure 7.1: Results of Markwardt’s analysis [194] show Doppler residuals as a function of time of
the best fit model. The top panel shows the residuals after setting , and demonstrates the
linear increase with time. The top panel shows all of the data, including segments that were filtered
out because of interference due to the solar corona (designated by a horizontal bar with “C”) or due
to general noise (designated “N”). The bottom panel shows the filtered residuals, including the best
fit value of the anomalous acceleration. The equivalent spacecraft velocity is also shown.
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