Specifically, how are the solar wind plasma, cosmic ray interaction with the interplanetary magnetic field, the termination shock, the heliopause, the heliosheath, and Oort cloud objects interfering with radio astronomy done from the vicinity of Earth? What radio bands are affected, why, and to what extent? Do you have any technical references for your proposal?I don’t know if I’ve posted this musing before…but to get radio telescopes out past the heliopause if not the Oort might be revealing…get out of our big solar radar’s ground clutter, as it were.
The solar wind plasma has an effect on radio signals - much like the ionosphere does - but then so does the ionised interstellar medium. It's an interesting question. It was the examination of fluctuations of the radio signals from quasars due to the solar wind plasma that led to the discovery of pulsars.Perhaps very weak ET signals can’t make it in…just the buzz of the cosmos at large. It would be nice to start hearing signals.
[...] interplanetary scintillation can be used as a probe of the density of the solar wind. Interplanetary scintillation measurements may also be used to infer the velocity of the solar wind.
[...] it was an investigation of interplanetary scintillation that led to the discovery of pulsars, even though the discovery was a by-product rather than the purpose of the investigation.
Yeah, our TV and radio broadcast signals likely get lost in the noise beyond a couple of light years. Radar pulses from Arecibo (when it was operating) and from military radars probably get somewhat farther. Aliens might use lasers, masers, gravitational waves, or even neutrinos to communicate over light years. Unfortunately, it appears that quantum entanglement doesn't offer any way of transmitting and receiving information even at light speed. If the aliens want to be found, either they or we need to try harder. I suspect many alien civilisations would find it easier to simulate universes to explore rather than actually do it. It's less expensive and also far less risky. When their (presumably roughly solar mass or less massive) suns eventually leave the main sequence, things get tricky during the red giant phase but the eventual white dwarfs emit exploitable energy for a long time - perhaps a hundred billion years.That’s a more satisfying answer to Fermi than us being alone.
Our local neighborhood is REALLY big. Even just the Local Bubble alone. I don't doubt there's alien civilizations out there. But if radio signals decay at 2 ly, and even directed signals have a low chance of being recieved, we have to rely on telescopes and sub-relativistic laser-communication probes, and those might not get back results until the higher end of this century, if we even launch any this century: this might be a very Mars and Venus and Titan and Callisto focused century, which is fine - but it does mean we're not looking far out, and most of our scopes and missions might go to Centauri, Bernard's, maybe Wolf or something of that nature.
The Local Bubble is a low-density cavity, thought to be a supernova remnant, about 300ly across in the Orion Arm of our galaxy.What do you consider "our local bubble", would that be just our galaxy?
The Local Bubble is a low-density cavity, thought to be a supernova remnant, about 300ly across in the Orion Arm of our galaxy.
Local Bubble - Wikipedia
Nope, it's a specific thing. That's why it's capitalised.Ah OK. I thought he meant he thought our local neighbourhood, our part of the galaxy being a local bubble.
I brought this up elsewhere when my suggested crowd-funded vomit-comet flight with one on Zero-G didn't go anywhere (and in retrospect, seeing how many problems Fran Blanche from FranLab had on her recent Zero-G flight trying to get her cameras ready in between arcs, i have to agree. it has to be a satellite. )I'd like to see it tested in space. It doesn't sound very expensive to construct and it might fit on a small cubesat. How much power is required to generate the claimed 200 μN of thrust and how efficient is the device? I assume waste heat needs to be radiated away. Assuming it is shown to work, how well would it scale up into something much larger? Nuclear fission would be required for power beyond a few AU presumably.
Have they tried piezoelectric polymers? The piezo-response is not as great as for ceramics but they might be more durable.I know Woodward and Fearn got some money from the NIAC grant but that probably all went into research. they've been trying to find a piezo material that doesn't fall part as quickly as what they are using now.
Have they tried piezoelectric polymers? The piezo-response is not as great as for ceramics but they might be more durable.
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