Package: wnpp Severity: normal The current maintainer of cassbeam, Brian R Furry <bfurry@nac.net>, is not active anymore. Therefore, I orphan this package now. If you want to be the new maintainer, please take it -- see http://www.debian.org/devel/wnpp/index.html#howto-o for detailed instructions how to adopt a package properly. Some information about this package: Package: cassbeam Binary: cassbeam Version: 1.0-6 Priority: optional Section: science Maintainer: Brian R Furry <bfurry@nac.net> Build-Depends: fftw-dev, docbook-to-man, tetex-extra, libglib1.2-dev, jade, debhelper ( >= 4) Architecture: any Standards-Version: 3.6.1 Format: 1.0 Directory: pool/main/c/cassbeam Files: 437ba8dc10312cee43556a2edbf79801 615 cassbeam_1.0-6.dsc 8166c1cb0a4c7cc5445a242544e83ae3 142866 cassbeam_1.0.orig.tar.gz 75b47f7cf9ba6785a5b77347434be709 42213 cassbeam_1.0-6.diff.gz Package: cassbeam Priority: optional Section: science Installed-Size: 448 Maintainer: Brian R Furry <bfurry@nac.net> Architecture: i386 Version: 1.0-6 Depends: fftw2 | fftw2-double, libc6 (>= 2.3.2.ds1-21), libglib1.2 (>= 1.2.0) Filename: pool/main/c/cassbeam/cassbeam_1.0-6_i386.deb Size: 291126 MD5sum: 560e611341dc89cb6e4e3cf31501bb33 SHA1: bf883d09063287d9a5564c88b34b36e69f0c3fb6 SHA256: a4ca773a349f9f35c35554c2620f783a5da9c41d6e4bb2e805b228ad4dd3125c Description: A program for Cassegrain antenna modelling Cassbeam is a Cassegrain antenna ray tracer. A Cassegrain antenna is a double reflector system which works on the principle of cassegrain optical telescope. A high gain cassegrain reflector antenna in Ku-band has been successfully developed for command transmit application for the missile programme. It can also be used for monopulse radar, satellite communication. . Based on an input text file, it computes several properties of the antenna including gain, zenith system temperature, and the beam, in full polarization. All calculations are done in the transmit sense and use reciprocity to relate to the equivalent receiving system. . Additionally, cassbeam allows deformations, or pathologies of the optics to be modelled. Currently this is limited to rotations and translations of the feed and secondary. In the future, large scale deviations in the primary (such as a misplaced panel) will likely be supported. Christoph -- cb@df7cb.de | http://www.df7cb.de/
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