Substantive points only ...
DeiRenDopa said:
And if they don't (fall down)? Which they won't, if we're in deep space.
Then we measure the speed of light in any direction.
That's what I expected you to say.
Why didn't you just say so the first time? (that's a rhetorical question)
Also, this doesn't help if we choose to conduct our experiments in free fall; how do you propose to determine horizontal if we're in a stable, circular orbit around the Earth (to take but one example)?
Look out of the window.
Sorry, that doesn't answer the question.
Would you care to try again?
Not good, Farsight, not good.
You might like to look in a mirror, and tell your reflected self to go do some research.
I've done the research. That's why I can give references to back up my case.
Please do so.
For other readers: there are, already, known limits on the stability of any particular pulsar, and the optical clock Farsight mentioned is far more accurate/stable than any pulsar.
Other observers will verify that the pulsar rate doesn't change when
you descend into a gravitational well. They will also verify that the clock rate of the clock you carry with you,
does.
I think, in your internet posting, you'll have come across the phrase "move the goalposts", right?
Well, here's a particularly spectacular example of just that.
To see why, we need to go back to how we got started on this. Here's the set of exchanges (if anyone really wants them, I can add links):
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This began with me proposing some experiments, all of which have to do with measuring things locally, like depth, pressure, g, altitude/elevation, and time.
me: Oh, one more thing we need to agree on: how to measure the speed of light.
Can you please describe how we can do this, using devices/equipment/techniques/etc which incorporate - at whatever critical point necessary - the definitions of the second and the meter?
Farsight: We measure the speed of light with light and mirrors, like Fizeau did. We already know something about relativity, so we constrain our measurements to horizontal measurements to avoid radial length contraction and keep our experiment simple. However we are not so stupid as to use our parallel-mirror light clock to time the back-and-forth travel time. Or our atomic clock, because that employs the electromagnetic hyperfine transition and microwaves. Or the optical clock which employs UV light. Or the quartz wristwatch, because that's electromagnetic like light. Or the mechanical clock, because that's made of electrons and protons etc, which have an electromagnetic nature. We time it using the distant pulsar.
me: As far as I know, Fizeau used several different experimental setups, each with light and mirrors.
And we need to be pretty specific, I think, so would you mind spelling out the actual setup you recommend, in more detail?
OK, but as we will be doing our experiments in many different environments, including in deep space, we need a way to establish what "horizontal" is; how do you recommend we do that?
We may have a problem here Houston.
Or not; can you explain how we "time it [the back-and-forth travel time, in some Fizeau-like set-up] using the distant pulsar"?
Farsight: Yes I would, stop wasting my time. Everybody knows the setup, see English Wikipedia.
You note which way things fall down, then you take an orthogonal direction.
Are you for real? Go do some research.
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So, the whole point of my question was to try to find a way - that Farsight and I could agree - to measure the
local speed of light.
The entire research program I've outlined, so far, is aimed at local measurements, and at understanding how they can be modeled.
What Farsight has done, with this last post, is move the goalposts, to examine things beyond the scope of the clearly stated program. For sure, those things are quite interesting, and well worth examining. But let's not get ahead of ourselves, shall we?
Further, Farsight has been rather sloppy here; he said exactly this (bold added): "However we are not so stupid as to use our parallel-mirror light clock to time the back-and-forth travel time. Or [...] We time it using the distant pulsar."
I haven't been at all sloppy. Let me spell out the point. I don't use bold often, but I think this time it's warranted:
if you use your parallel-mirror light clock to measure the speed of light, then if light moves slower where you are as opposed to where you were, the light in your parallel-mirror light clock will move slower too. So your measurement of the speed of light will yield the same value at both locations. Give it up Dopa, you cannot conceal this simple point.
Right. It will.
So, back to my question: how do you use a distant pulsar to measure the
local speed of light?
Got it now?
He didn't say which distant pulsar he intended/proposed to use, and if he meant to say something like 'a set, or array, of distant pulsars', he omitted to say how he'd use such an array as a clock. If you have a few hours to spare, you can peruse the (astrophysics) literature on this topic, and discover that it is very far from trivial how to set up such a thing. Curiously, the Wikipedia link Farsight gives as his source has, itself, two papers as sources, dated 1997 and 1984. This particular area in astrophysics (and physics, no doubt) is very active, and 1984 is like the distant past. Oh, and the current SI definition of the second dates to 1997. Perhaps Farsight is simply not conversant with the relevant literature?
He is. Just as readers of this thread are now conversant with your attempt to obscure the issue at hand.
Let's see, shall we?
Dear readers of this thread, are you "
now conversant with [my]
attempt to obscure the issue at hand"?