Figure 31

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 a = 0 P, 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.