source file: mills2.txt Date: Fri, 26 Jan 1996 13:11:24 -0800 Subject: Wilson's CPS From: "John H. Chalmers" I need to correct a misapprehension that I am the co-discoverer of Wilson's CPS. This is not the case; Erv did it all by himself. I think the confusion stems from a joint paper we published in the ICMC proceedings back in 1981 (at NTSU) on our computer projects at UCSD in the late 60's, though the paper makes it clear that they were Erv's alone. Erv's discovery of the CPS came about as he pondered the best set of pitch bases for a large table of ratios I was compiling. As we were becoming limited by the great length of the table, Erv observed we could obtain extra "complexity" (more composite intervals and longer chains of 5ths, 3rds, etc.) by transposing the whole list to various pitches related by well-chosen ratios. This turned out to be a very efficient procedure as we had to print out the results on wide computer paper anyway and it cost us essentially nothing to add the extra columns when we printed the list off a tape. I didn't mean to imply that the XH12 paper was the only place where Erv Wilson's theories have been published, but it is the most complete and easily accessible source. Other issues of XH have articles by Erv or his student Kraig Grady and Paul mentioned his article on the 14-tone stellated 1.3.5.7 hexany. (BTW, Paul, Erv said he likes your setting of the Hildegarde of Bingen text very much.) The Tables of Contents of all issues of XH are available at John Pusey's WEB site whose URL is http://www.tiac.net/users/xen/xh.html --John Received: from eartha.mills.edu [144.91.3.20] by vbv40.ezh.nl with SMTP-OpenVMS via TCP/IP; Sat, 27 Jan 1996 01:40 +0100 Received: from by eartha.mills.edu via SMTP (940816.SGI.8.6.9/930416.SGI) for id QAA03976; Fri, 26 Jan 1996 16:39:59 -0800 Date: Fri, 26 Jan 1996 16:39:59 -0800 Message-Id: <960127003642_71670.2576_HHB75-1@CompuServe.COM> Errors-To: madole@ella.mills.edu Reply-To: tuning@eartha.mills.edu Originator: tuning@eartha.mills.edu Sender: tuning@eartha.mills.edu