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Henri Wilson replied to Leonard Kellogg:
Henri Wilson said to George Dishman: I have agreed that the extinction distance appears to depend on star period and star proximity. And I have said that the light speed unification distance is inversely proportional to rate of bunching. The more rapidly the light bunches, the shorter the unification distance. That applies to all light sources. It applies to pulsars, white dwarfs, red giants, cepheids, and main sequence stars. It applies to light sources bouncing back and forth on springs. It applies to infrared LIDAR and radio-frequency RADAR emitted by police speed measurement devices and reflected from moving vehicles. It applies to light and radio signals sent from or received on aircraft in flight. It applies to radio signals from satellites in Earth orbit, rovers on the surface of Mars, and Cassini orbiting Saturn. The more rapidly the light bunches, the shorter the unification distance. Always. The rate of bunching is proportional to the radial acceleration at the section of the orbit where the pulses/photon were emitted. Yes, we already know that. I was pointing out something that you appear not to have picked up on yet. For orbits with the same eccentricity, that is also proportional to the peripheral velocity at the same phase. (for instance at periastron) Again, we already know that. I was pointing out something about the unification distance that you apparently still haven't noticed. It's a simple average of all the points at that phase Henry, stop whining. Well it all sounds pretty suspect to me. It is an elementary school level problem. It is like measuring your height once an hour during the day for a week, then averaging the measurements together. You measure your height immediately after arising, again an hour later, and so on. After a week you sum all the measurements made just after arising and divide the result by seven, then you sum all the measurements made an hour after arising and divide the result by seven, and so on. When you graph the results you have a chart showing how your height changes during the day. Another way of achieving exactly the same result is to plot all of the individual measurements and then draw a smooth curve which most closely matches the data points. What has this to do with extinction? Nothing. I commented on two different things in my post. The first was the dependence of extinction distance on the rate of bunching, while the second was your concern that averaging of measurements taken over a number of cycles sounds pretty suspect to you. Leonard |
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