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|    rec.arts.sf.science    |    Real and speculative aspects of SF scien    |    45,986 messages    |
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|    Message 44,704 of 45,986    |
|    Mikkel Haaheim to All    |
|    Re: James S.A. Corey's answer to There A    |
|    10 Dec 16 14:51:19    |
      From: mikkelhaaheim@gmail.com              Le jeudi 27 octobre 2016 04:06:49 UTC+2, Rick Pikul/Chakat Firepaw a écrit :              > You are trading detection over a given time in exchange for a longer time        > to be spotted. It's going to be a wash.              I think you really don't understand how probabilities work. IFF both the scan       rates and fire rates are fixed, then, yes, eventually, you are going to be       detected (unless your fire rate is the same as the scan rate, but out of phase       with the scan... in        which case you are never going to be detected by your burns). However, even       here, the amount of time before detection can be considerable, and it may take       an extensive amount of time before detection can be verified. If either of the       cycles are varied,        you are running a roullette table favouring the ship.              >               > I take it you have never seen a photo of a VASIMR drive in operation        > then. Even the little 5N testbed has a visible plume several metres long.              Actually, I HAVE seen both the stills and videos of VASIMR. However, it is       true that my laptop monitor does not handle low light levels very well. When I       reviewed the videos on another monitor, you are correct that the plume become       more apparent.       That said, I think you might be having some problem understanding the actual       scale of the images. ALL of those images were produced either by mounting a       camera directly onto one of the viewing ports, or by setting up a camera       within the chanmber itself.        This chamber has a diameter of 4m. The entire test field is only 5m in length       (so, no, there is no actual visual support for your assertion that the visible       plume is "several meters" long). Most of the photos and videos are taken with       an FOV of slightly        over 4m^ (2m x 2m), AT MOST... although there was at least one video shot from       behind that apparently covers the full 5m length of the plume test region, as       well as a meter or so of the mounting region.       So, yes, you can see the plume from a distance of 2m or so away from its       highest concentration zone, using a light sensitive camera (assuming the       monitor is capable of showing low light images), with a plume distance of       perhaps 5m or more.       I have, however, found some information that provides a best case range of       detectability. I will try to lay that out once I have a little more time.                     >        > WISE was also looking for extremely hard to spot things, many of which        > would have no bearing on interplanetary combat. It was also in the        > business of detecting and observing interstellar and intergalactic        > objects.              WISE/NEOWISE was in the business of detecting and cataloguing things that were       very difficult to detect. It had excellent capabilities (much better when       cryogenically cooled). However, its abilities were limited by the laws of       physics, as well as other        factors. For instance, it is not possible for an IR platform to detect       emissions from objects colder than the platform itself, because the platform       will flood the detectors with the same wavelength emissions that the detectors       are looking for (which is        why two of the IR bands were rendered inoperable once the cryostasis ran out).              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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