WOULD STRONG LARGER SCALE MAGNETIC FIELDS BE OF WORTH TO MAKE A CHEAPER GIANT TELESCOPE TO RESOLVE EARTHLIKE WORLDS?
Magnetic bubbles may make a telescope with great high resolution, or at any rate a telescope with a high cash value! As I say here the large size of the field may enable us to make a telescope with the lense of the field lines of any size up to the size of the solar system or more. A beam sent through the somewhat shimmered field to a near sensor or a light on the other side would then be processed by the computer to find the image, an earthlike world, or anything else in the cosmos we would hope to resolve well.
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We read where it will be many years perhaps 50 or more in the hiatus from when the exosolar planets were seen in the 1990's to when the proof of life on some earthlike worlds will be proven. This was an underestimation (knowing me!) and the magnetic bubble method means we may see life on other worlds without the wait! This would be better than any telescope for resolution, even so there is some cost, although it would be the cheapest cost/resolution by far, the only way I can think of to build this much resolution.
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If in 100 years we actually build a sensor to sense the change in the light as it moves through the more distant magnetic fields it would be low cost. A problem with this more giant scope would be that because we can't move much relative to the more distant magnetic fields, so we have to either wait till we slowly move with the refracted line of sight till it's where we can see the more distant cosmic light show, or move our own sensors to see through the lense, and each image because of the slow motion of the giant wheel would be mostly all we got. No more resolution and no more images than what the optics would allow.
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Even so this seems like a good way to see Earthlike worlds or search with much more web zoom map power for advanced worlds by merely using a source a receiver and a sensor to make the giant telescope that might change our world, change is inevitable, other than from a giant vending machine!
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Also of use and cheaper yet than building this machine may be to use the radiation of planets like Jupiter or Saturn to refract the light with a powerful wave, a ready to go lense at no cost for the field maintenance (To make the bubble field machine in more Euclidian realms the most cheap, reflecting the waves to make standing waves, and using solitons may save a lot. Another option might be to block all the field lines with a cowl or shield ectcetra except for the lines to see just the stars we want to see while saving power.). The massive fields of planets are cost saving till we might be able to build a truly giant field telescope with more power like fusion power. Here's my site about Inertial Focus Fusion and why it seems to have advantages over other fusion machines.
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Whatever type of higher power machines we may build in the years ahead for now at any rate cost will be important. For nearer travels in non lightyears using the already powerful fields of Jupiter or Saturn seems of use (the sun's is just .5 Gauss, and Jupiter’s is about 100). From Earth to other planets like the larger cosmic fields the line of site through the fields is limited, this could be solved by moving a set of satellites to continual orbit around Jupiter. When one machine was in site of what we want to see e.g. mom's win at sewing the stars on her weave in mom's county celebration, the line of site as it changes as the ship moves through the field would tell us about via of the distant light or other field, and as it would travel out of conjunction to line of sight the job would be relayed to the next machine. This method may tell us about distant radiance like no other machine may allow because it's moving through the strong magnetic field and also at more than one frequency.
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Lensing by electric or magnetic fields is a much stronger effect than Einstein's gravitational lensing because of the much higher intrinsic strength of the field, and this is optical lensing, or at any rate may be more useful to lense the radiation in the form of electrons and of considerable use for light too, depending on the wavelength and energy.
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