ESA sets clock by distant spinning stars
esa.int
esa.int
Atomic "clocks" are more like CPU "clock speed". Atomic clocks give a very precise measure of a time interval.
But they don't tell you what time it is. The time of day needs to express both the idea of the rate of time, and also the position of the Sun and stars, relative to the position of the Earth.
Like, we use "number of seconds since midnight, 1 January 1970" and expect that number to map to a time like "2018-12-25 20:37:44 UTC", and we expect that value to map onto a time about four days after the Northern Hemisphere winter solstice.
Pulsar surveys make sure that those two concepts line up. Most of the time.
[0]: https://nrao.edu
I hope ESA documents and open sources the work. If the required antenna/receiver sensitivity is not too ridiculous, this might make a cool project.
https://www.rtl-sdr.com/detecting-pulsars-rotating-neutron-s...
I think some of the newer SDRs with 12-16 bits per sample and 20+ MHz bandwidth might be substantiated more suited to the task.
I'm thinking phased array. It's a more scalable method to getting large apertures and it can constructed to target multiple pulsars at once.
My thinking on the better hardware was that getting 10Mhz bandwidth allowed them to reduce the dish size to 3.5m. Better dynamic range and even more bandwidth might get you to <3m, which could possibly be in old C-band dish antenna range.
Edit: More recent exercise - http://hawkrao.joataman.net/pulsar/results/index.html
GPS system need to reconstruct the time of the satellites because we know they tick in sync, but those star tick independently it’s really about observing the blinking.
If you were curious how much this clock drifts. I think we might have more accurate atomic clocks, though, so this still isn’t practical for actual precise timekeeping at that level.
Their radio telescopes are located in Europe. How would you have constant time signals available? I would guess the errors in synchronizing / matching the signals across telescopes in the ground would be by far the larger error compared to the signal itself.
But who knows, I'm just an outside observer.
> “A timescale based on pulsar measurements is typically less stable than one using atomic or optical clocks in the short term but it could be competitive in the very long term, over several decades or more, beyond the working life of any individual atomic clock.
For people who rush to down vote: this is just a joke. Obviously ESA should decide how we measure time.