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Ranging and Pioneer
Thus spake "
Of critical importance is the timescale between initial state and final state when modelling the motion. This timescale is determined by the accuracy with which we can measure. Local distances can be measured with great accuracy, equivalent to a short timescale. Remote distances are intrinsically less accurate (e.g. radar distance measurements to mars are accurate to about 12m). I'm not familiar with the details of Mars ranging but I have looked at Pioneer in some detail. I will comment on that as it may be of interest to you but it doesn't seem to answer my original question. The signal from Pioneer uses an effective Doppler frequency of 1MHz, equivalent to a distance scale of 300m. Although the final digital analysis is done around 1MHz, the RF is heterodyned down to that against the reference. It means that the measurement resolution is still that of the 2.291GHz carrier. Further the MDA is capable of measuring phase to 1/256 of a cycle or about 0.5mm in range. While the ranging system itself wasn't available, the frequency measurements are still taken from that same hardware and have that resolution. This might be true if everything were perfect, but it is not. To interpolate higher frequencies than the 1MHz effective Doppler frequency one has to assume no such thing as cycle slip, for example. In fact even GPS systems are plagued with cycle slip. Note the residuals from Galileo in Figure 10 of gr-qc/0104064 and the discussion to the left that indicates consistency to about 4m over a day. The discussion seems to indicate that they cannot tell whether the acceleration was present. If they are suggesting that radar was accurate to 4m, then I would expect it not to be present. I am not sure that that is what they are saying because I had been given to believe that the measurements of Mars are the most accurate within the Solar system. The actual measurements are limited to a few metres accuracy mainly due to the group delay in the somewhat unpredictable solar plasma and the unknown angle of refraction through the atmosphere and at the boundary of the ionosphere, but the resolution of the instrument which I think is the determining aspect from the QM point of view is better than 1mm. All these things have an effect, but the reason given by Anderson on p7 "Currently, two types of Galileo navigation data are available, namely Doppler and range measurements. As mentioned before, an instantaneous comparison between the ranging signal that goes up with the ranging signal that comes down would yield an â~@~\instantaneousâ~@~] twoway range delay. Unfortunately, an instantaneous comparison was not possible in this case. The reason is that the signal-to-noise ratio on the incoming ranging signal is small and a long integration time (typically minutes) must be used (for correlation purposes). During such long integration times, the range to the spacecraft is constantly changing". The long integration times appear to me to introduce uncertainties much greater than 1mm. Certainly the uncertainties can be reduced in principle by using a stronger signal, and more accurate measurement may be possible, but if this idea is right that will merely extend the distance to a space craft at which ranging becomes impracticable and the Pioneer acceleration becomes observable. This was the gist of my original question and where I am still puzzled. The conventional linear Hubble law if applied to Pioneer 10 predicts an apparent acceleration some 15000 times smaller than the anomaly given by the equation a_H = 2 H v. I don't understand why you think your analysis produces a result four orders of magnitude larger than the normal Hubble Law under either of the regimes you explain above. Sorry if I'm being a bit slow but it is this factor of 15000 increase that I cannot fathom. I am not quite sure where the 15000 increase is, or what the equation a_H = 2 Hv refers to. I have it that quantum coordinates introduce an acceleration in time which can be shown by a coordinate transformation equivalent to an acceleration Hc. Regards -- Charles Francis substitute charles for NotI to email |
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