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Ranging and Pioneer
Oh No wrote:
Thus spake " Oh No wrote: The signal from Pioneer uses an effective Doppler frequency of 1MHz, equivalent to a distance scale of 300m. ... the MDA is capable of measuring phase to 1/256 of a cycle or about 0.5mm in range. ... 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. Surely the quantum effects are only affected by the equipment, not assumptions, but no matter, this was just FYI. Cycle slips were sufficiently infrequent that many were corrected by hand by the analysts going over the data. I believe Anderson et al may have excluded any measurement with a cycle slip from subsequent processing but I'm not sure on that without rechecking the paper. 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. They are saying their checks showed the integrated Doppler velocity was consitent with the ranging result to within 4m over one day. The anomaly is comparable or smaller so needs longer timescales to show up. 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. Perhaps in percentage terms, ranging using the corner refectors on the Moon achieves cm accuracy. .... 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. You can think of Doppler giving a plot of speed over time while the ranging system intergrated hence gives something like an average ignoring acceleration. It is just a practical difficulty. ... 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. Take the Hubble constant H as 71km/s per MPc. A parsec is 3.09e16 m and an AU is 1.5e11 m so changing units H = 3.44e-7 m/s per AU. In Jan 1987 the craft was at 40 AU so the signal had to travel 80 AU giving a redshift due to the Hubble constant equivalent to a speed of 2.75e-5 m/s. Similarly in Dec 1994 at the end of the period analysed for Pioneer 10, the range was 60 AU and the round trip 120 AU which gives an apparent speed from the Hubble Law of 4.13e-5 m/s. That's a change of 1.38e-5 m/s in a time of 2921 days or 2.51e8 s giving an apparent acceleration of 5.50e-14 m/s^2. Compare that with the anomaly of 8.74e-10 m/s^2. The equation that summarises that is a = 2 H v where H is the Hubble constant, v is the radial speed of the craft, a is the resulting apparent acceleration and the factor of 2 is due to the double trip. I have it that quantum coordinates introduce an acceleration in time which can be shown by a coordinate transformation equivalent to an acceleration Hc. If it is an effect in time, that could be quite different to the ranging analysis and might explain why the numbers differ so much. Of the phenomenological time models considered by Anderson et al, do any of their equations (60) through (65) match? See page 46 of gr-qc/0104064 for details. George |
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