- 35,014
- 21,723
And a much more omnidirectional antenna.Filip Larsen said:And that is just using RF technology
I am amused that a giant planet sized iris shutter is sensible, but a radio? Now that's just crazy talk!
And a much more omnidirectional antenna.Filip Larsen said:And that is just using RF technology
The cold light of reality. It would involve crude amplitude modulation of a very dirty signal.Baluncore said:A planet sized mirror or metallic reflector, will not work near a pulsar because the eddy currents induced in the mirror by the pulsar rotation, will distort the mirror.
A back-lighted LC (liquid crystal) shutter does not need to remain accurately aligned, but it does need a sandwich of five layers made up of two polarizers, two transparent sheet electrodes, and a liquid crystal filling. The transparent sheet electrodes cannot be superconducting because then they would become mirrors.Devin-M said:"Each eye's glass contains a liquid crystal layer which has the property of becoming opaque when voltage is applied, being otherwise transparent."
https://en.wikipedia.org/wiki/Active_shutter_3D_system
Were you referring to my post about timing the feeds to parts of the reflector / mask?Vanadium 50 said:This is the principle behind a Yagi antenna.
You seems to have missed my point here. The planned project would need to modulate the light from the star. The star light hitting the screen is uniform and continuous and the requirement would be to alter the level of the light output (reflected or in the shadow; it doesn't matter) from elements all over the disc. That means it's necessary to get a synchronised modulating signal to every part of the disc to drive any 'shutter'. Mis-timing of the modulating signal to any of the elements will blur the received pulse shape.Vanadium 50 said:Sure, but it accomplishes the same thing, just with reflections rather than active delays on the feeds.
It's amusing that a planetary-sized mechanical iris is perfectly fine, but a planetary sized antenna? More crazy talk.
Ballpark, a 10 km antenna would have enough gain to make the signal as bright as the Pioneer missions with no more power, and if you could go to kilowatt-level power, you need only 1 km. Make it out of aluminized mylar and it weighs 100 tons.
This may be rocket science, but it's not Ringworld.
Can we launch repeater stations along the way? There is a particular advantage in having a relay station well away from Earth, as it means that the space probe is not looking at the warm, and hence noisy, Earth.sophiecentaur said:You seems to have missed my point here. The planned project would need to modulate the light from the star. The star light hitting the screen is uniform and continuous and the requirement would be to alter the level of the light output (reflected or in the shadow; it doesn't matter) from elements all over the disc. That means it's necessary to get a synchronised modulating signal to every part of the disc to drive any 'shutter'. Mis-timing of the modulating signal to any of the elements will blur the received pulse shape.
I'd suggest that a data rate would need to be at least tens of MB/s and the delays over hundreds of thousands of km would make this problematic. (It's not just a matter of 'detecting' the presence of the light modulator.)
BTW, a Yagi antenna is not a good example of a super directive antenna as there is only one driven element. There are synthesised arrays with multiple feeds and even multiple transmitters but, again, the transmitters need to have synchronised modulation as well mutually coherent RF carrier waves.
I don't know how effective relay links would be as there is nothing 'in the way' which is why relays are used for Earth systems.tech99 said:Can we launch repeater stations along the way? There is a particular advantage in having a relay station well away from Earth, as it means that the space probe is not looking at the warm, and hence noisy, Earth.
Repeater/relay links are also used for signal amplification. As long as there is a local source of energy, using a receiver/transmitter device at the relay location boosts the overall signal/noise ratio. Think about the undersea phone cables or other long communication links where powered repeaters are used...sophiecentaur said:I don't know how effective relay links would be as there is nothing 'in the way' which is why relays are used for Earth systems.
The first trans-Pacific telephone cable was laid from Hawaii to Japan in 1964, with an extension from Guam to The Philippines.[21] Also in 1964, the Commonwealth Pacific Cable System (COMPAC), with 80 telephone channel capacity, opened for traffic from Sydney to Vancouver, and in 1967, the South East Asia Commonwealth (SEACOM) system, with 160 telephone channel capacity, opened for traffic. This system used microwave radio from Sydney to Cairns (Queensland), cable running from Cairns to Madang (Papua New Guinea), Guam, Hong Kong, Kota Kinabalu (capital of Sabah, Malaysia), Singapore, then overland by microwave radio to Kuala Lumpur. In 1991, the North Pacific Cable system was the first regenerative system (i.e., with repeaters) to completely cross the Pacific from the US mainland to Japan.
Of course that's correct but there is always something 'in the way' with existing comms routes to make things worse than inverse square law. Cable loss is 'per metre' and all terrestrial routes involve obstacles (the horizon for example). I don't know what the 'absorption coefficient' of empty space is. I guess a signal passing through a nebula could be attenuated right across the band - there a certainly absorption lines.berkeman said:Repeater/relay links are also used for signal amplification.
As the number of links in a repeater chain increases, the reliability of communication falls very rapidly.tech99 said:Can we launch repeater stations along the way?
Yes I agree. This reminds me of a couple more of the AI Art renderings I made using DALLE 2 with the following prompt:collinsmark said:There are bigger problems than the modulation scheme. The iris would need to be gigantic, perhaps between planet sized and solar system sized. That's the real challenge.
Destructive interference will destroy the advantage of an aperture. If it takes 1 second for the modulation clock to spread across the elements of a flat iris, then the data rate will be less than 1 bit per second.collinsmark said:I don't think the problem is necessarily phase synchronization in this situation.
Baluncore said:Destructive interference will destroy the advantage of an aperture. If it takes 1 second for the modulation clock to spread across the elements of a flat iris, then the data rate will be less than 1 bit per second.
The data rate could be greatly increased by employing a parabolic iris, and distributing the modulation clock to each element from the focus. The modulation bandwidth would then be limited by the phase error of the parabolic iris surface, with receiver noise and bandwidth being a separate problem.
A large aperture is always necessary to make any array very directive and Tx RF power will always be limited. Information rate will be directly affected by the level of signal arriving at Earth so the array would need to be as big as possible in order to maximise data rate.collinsmark said:high-gain RF transmitters don't need to be big.
Fair enough. What you say is correct. Chalk it up to poor wording on my part.sophiecentaur said:A large aperture is always necessary to make any array very directive and Tx RF power will always be limited. Information rate will be directly affected by the level of signal arriving at Earth so the array would need to be as big as possible in order to maximise data rate.
The same sums apply for Tx and Rx; SNR is affected by both.
I think we are not disagreeing. An Rx system can use fancy signal processing with multiple sub antennae. For Tx, the problem of getting powerful signals to be coherent would be much harder so there would be a real limit to the Tx gain available.collinsmark said:What I should have said is that for a given link budget, and for practical reasons, it would be a lot easier to have a bigger Rx antenna on (or near) Earth and have a comparatively smaller Tx antenna on the probe that has to travel to a whole 'nother star system.
I wonder how you deal with that big bright thing right next to the image of your 1W laser... I didn't see that addressed in the short popular article -- is it addressed in the more detailed articles about this technique?Devin-M said:“a solar-lens telescope would be able to detect a 1 Watt laser coming from Proxima Centauri b, about 4 light-years away”
— by placing a telescope around 600AU from the sun & using the sun itself as a gravitational lens.
Detecting is one thing; detecting modulation is an entirely different matter. There is really no point in discussing this without addressing the rate of information carried.Devin-M said:“a solar-lens telescope would be able to detect a 1 Watt laser coming from Proxima Centauri b, about 4 light-years away”
Yet again, SNR is not mentioned.berkeman said:I wonder how you deal with that big bright thing right next to the image of your 1W laser... I didn't see that addressed in the short popular article -- is it addressed in the more detailed articles about this technique?