Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.3 4.3bsd-beta 6/6/85; site ucbvax.berkeley.edu.BERKELEY.EDU Path: utzoo!watmath!clyde!burl!ulysses!mhuxr!mhuxn!ihnp4!ucbvax.berkeley.edu!space From: dietz@SLB-DOLL.CSNET (Paul Dietz) Newsgroups: net.space Subject: Re: Phase conjugation Message-ID: <8601241437.AA04546@s1-b.arpa> Date: Fri, 24-Jan-86 08:12:16 EST Article-I.D.: s1-b.8601241437.AA04546 Posted: Fri Jan 24 08:12:16 1986 Date-Received: Sat, 25-Jan-86 09:31:28 EST Sender: daemon@ucbvax.berkeley.edu.BERKELEY.EDU Organization: The ARPA Internet Lines: 22 n >Why won't the phase conjugation technique work in reverse to build a >large earth based telescope that removes the effects of atmospheric >turbulence? One would need a laser in the field of view (on a >satellite, say) to determine the distortion during the trip down through >the atmosphere, then apply the correction for that distortion to all >incoming light to produce an undistorted image. If it works, it sounds >like it could make the Space Telescope obsolete. I'm not sure if phase conjugation is what you want, but it doesn't seem impossible to use a laser beam to determine what the atmosphere is doing, then correct the image by computer. You might have some problems if the atmosphere causes different wavelength light to travel along different paths. There's already a technique, called speckle interferometry, that stacks short snapshots of a star into one image with resolution better than normally allowed by atmospheric distortion. I don't think it would make the space telescope obsolete; the ST can also be used to see infrared and ultraviolet light in wavelengths where atmospheric absorption and interference is important.