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#199 | ||
6809 > 6502
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Aug 2003
101ร103 Posts
2A8B16 Posts |
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#200 |
"TF79LL86GIMPS96gpu17"
Mar 2017
US midwest
1CC616 Posts |
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C-130s go back to the 1950s; LC-130s to 1956. https://en.wikipedia.org/wiki/Lockheed_LC-130
When failure is not an option, as in the last resupply flight of the season to the South Pole Station, it's an LC-130 that doesn't QUITE touch down. They kick cargo out the back at a few feet of altitude above the runway and let the crates slide to a stop on the snow. It's called "drifting". If they were to land and be unable to take off, the air crew would be staying until another could come get them, possibly for months, and there might not be enough provisions on site for that added demand. Last fiddled with by kriesel on 2022-09-27 at 13:57 |
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#201 |
Bamboozled!
"๐บ๐๐ท๐ท๐ญ"
May 2003
Down not across
2·5,827 Posts |
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#202 | |
Bamboozled!
"๐บ๐๐ท๐ท๐ญ"
May 2003
Down not across
2·5,827 Posts |
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#203 |
"TF79LL86GIMPS96gpu17"
Mar 2017
US midwest
736610 Posts |
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That's putting it mildly. The first particle type to exit a star going supernova is neutrinos. Xrays take a long time to get out, but very large quantities of matter are essentially transparent to neutrinos, including planets and stars. The Ice Cube Neutrino Observatory uses the bulk of the earth as a shield against other particles, and deduces which neutrino events arrived through the earth rather than through the ice, by relative timing of detection among the several adjacent modules, rejecting northward-bound detections in favor of southward. It's only what I call the unluckiest neutrinos that get detected; made it ALMOST through the earth, but interacted with the last kilometers of ice before escaping into space again.
https://en.wikipedia.org/wiki/IceCub...no_Observatory was a ~$330 million US construction project (without the dense core). Fermilab (Batavia Illinois) will be used to drive pulsed neutrino beams aimed at an underground neutrino detector DUNE 1300 km away at Lead South Dakota. Current projections are $2.6 billion US. Much of the excavation & infrastructure was preexisting due to repurposing a long-operating deep gold mine. How to make a neutrino beam: https://www.symmetrymagazine.org/art...-neutrino-beam Last fiddled with by kriesel on 2022-09-27 at 17:51 |
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#204 | |
Bamboozled!
"๐บ๐๐ท๐ท๐ญ"
May 2003
Down not across
2×5,827 Posts |
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#205 | |
If I May
"Chris Halsall"
Sep 2002
Barbados
2×72×113 Posts |
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I remember that. But the team figured out their issue. Damn those BNC connectors! |
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#206 | |
"TF79LL86GIMPS96gpu17"
Mar 2017
US midwest
163068 Posts |
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The largest submarines known are Russia's Typhoon class, with 48,000 ton displacement. https://en.wikipedia.org/wiki/Typhoon-class_submarine Allocating ~2% of its displacement to a neutrino detector's active volume would allow 1 kiloton detector (receiver) size. (Containment structure, shielding/veto of reactor & cosmic backgrounds, cabling, data acquisition etc. would be additional and could exceed 5% in total.) Table IV of https://www.aps.org/policy/reports/m...king_Group.pdf shows muon neutrino interaction rates of 14. to 180,000 per kiloton-YEAR, depending on energy and distance. That's not much signal on which to impose modulation no matter how cleverly done. The Daya Bay neutrino experiment (8 times 20 tons detector size) achieved 5.5 million interactions over 9 years in close proximity to a 6-pack of nuclear reactors used as particle source. http://dayawane.ihep.ac.cn/twiki/bin...blic/DYB_Final That's 5.5E6 interactions/9 years / (8 * .020 kilotons) = 3.8E6. interactions/kiloton-year. Reactors used as transmitters by frequent modulation of fission rate and power output would require excellent encryption since their neutrino output would likely be nearly isotropic, and could also present problems of grid stabilization. Their output power modulation might be easily inexpensively detectable by a well placed monitoring of grid voltage. The power modulation of a nuclear core can be risky (Chernobyl!) US power slew rates are of order 6-10 MW/sec or less, which would limit signaling rate. If we suppose modulation was limited to 10% of fission output and signal falls off as inverse square of distance, 3.8E6 /kiloton-year *0.1 * (1.9 km / 1000 km ) ^2 = 1.38 interactions/receiver-year at 1000 km. At 100 km, it's 138., still less than one half interaction per day. Last fiddled with by kriesel on 2022-09-27 at 22:34 |
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#207 |
If I May
"Chris Halsall"
Sep 2002
Barbados
2×72×113 Posts |
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#208 | |
Feb 2017
Nowhere
5·11·113 Posts |
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EDIT: It occurred to me that, however unlikely, it is possible that the launch code transmission could continue despite a general nuclear war. If that happened, what would follow? It would lead to a barrage of nuclear missiles after the initial exchange by however long it takes to transmit the signal - six months, a year, whatever. Last fiddled with by Dr Sardonicus on 2022-09-27 at 23:35 |
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#209 |
"Rich"
Aug 2002
Benicia, California
5×17×19 Posts |
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This US Navy communications station, shut down in 1993, is about a 20 minute drive from my home and was used to communicate with ballistic missile submarines:
https://en.wikipedia.org/wiki/Skaggs...cation_Station |
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