From nobody Fri Nov 13 10:57:04 1998 Newsgroups: sci.astro Path: newsfeed.cv.nrao.edu!newsgate.duke.edu!nntp-out.monmouth.com!newspeer.monmouth.com!sunqbc.risq.qc.ca!newsflash.concordia.ca!utnut!utgpu!utinfo!nova.astro.utoronto.ca!ayee From: Andrew Yee Subject: Radar-processing algorithm produces high-resolution lunar images (Forwarded) X-Nntp-Posting-Host: nova.astro.utoronto.ca Content-Type: TEXT/PLAIN; charset=US-ASCII Message-ID: Sender: nntp@campus-news-reading.utoronto.ca (News) Organization: UTCC Campus Access Mime-Version: 1.0 Date: Sat, 31 Oct 1998 04:14:38 GMT Lines: 72 Xref: newsfeed.cv.nrao.edu sci.astro:70015 News Bureau University of Illinois at Urbana-Champaign 807 S. Wright St., Suite 520 East Champaign, IL 61820-6219 (217) 333-1085 fax (217) 244-0161 e-mail: uinews@uiuc.edu CONTACT: James E. Kloeppel, Physical Sciences Editor (217) 244-1073 E-mail: kloeppel@uiuc.edu November 1998 Radar-processing algorithm produces high-resolution lunar images CHAMPAIGN, Ill. -- Superior radar images of the moon, inner planets and asteroids are possible with a "polar-format" radar-processing algorithm developed at the University of Illinois. The algorithm, from spotlight-mode synthetic aperture radar, provides improved image quality over conventional processing, without an excessive increase in computational requirements or complexity. "In astronomy, radar reflectivity data are sometimes used to supplement other types of observations," said David Munson, a U. of I. professor of electrical and computer engineering. "Radar measurements, for example, have proven particularly useful for imaging Venus, where a thick layer of clouds perpetually obscures the planet's surface. Oftentimes, however, the radar images produced from Earth-based measurements are of poor quality." Conventional radar-imaging systems are based on range-Doppler techniques, Munson said. "But in the time it takes to collect astronomical data -- typically 10 to 20 minutes -- the object's rotation causes both the range and the radial velocity of reflectors to change with time. Because conventional range-Doppler processing makes no allowance for this relative motion, the resulting image is blurred." The polar-format, spotlight-mode synthetic aperture radar approach avoids this problem by affixing a spatial-domain coordinate system to the target. As the object rotates with respect to the radar, the coordinate system rotates with it, thus avoiding smearing in the image. Munson, former graduate student Jennifer Webb (now a researcher at Texas Instruments) and Nick Stacy, a researcher with the Microwave Radar Division of the Defense Science and Technology Organization in Australia, recently applied the polar-format radar-processing algorithm to lunar reflectivity data collected at Arecibo Observatory in Puerto Rico. "Although the moon constantly presents the same face toward Earth, we get to see it from different angles as it moves," Munson said. "And in our mathematical model, that's all that's required. The principle employed is nearly identical to that used in computer tomography in medical imaging." The high-resolution lunar images produced by the researchers were far superior to what had been obtained in the past with conventional radar-processing techniques. "The amount of computational work was only three times what was formerly required," Munson said. "So, with a small increase in computational effort, we can get vastly improved imaging." As an additional benchmark, the researchers compared their images with those obtained with another approach developed by Stacy, called focused range-Doppler processing. This latter technique "produces the best known results, but is much more expensive, computationally," Munson said. "Our polar-format processing algorithm performed nearly as well, with considerably less effort." The researchers describe their algorithm and present their results in the November issue of IEEE Transactions on Image Processing. --- Andrew Yee ayee@nova.astro.utoronto.ca