Path: utzoo!utgpu!news-server.csri.toronto.edu!mailrus!uwm.edu!zaphod.mps.ohio-state.edu!mips!winchester!mash From: mash@mips.COM (John Mashey) Newsgroups: comp.sys.super Subject: Re: I/O subsystems Message-ID: <39320@mips.mips.COM> Date: 12 Jun 90 03:44:12 GMT References: <201@csinc.UUCP> <253@garth.UUCP> <202@csinc.UUCP> <292@garth.UUCP> <10280@batcomputer.tn.cornell.edu> <359@garth.UUCP> <6374@amelia.nas.nasa.gov> <424@garth.UUCP> <6583@amelia.nas.nasa.gov> <39284@mips.mips.COM> <6662@amelia.nas.nasa.gov> Sender: news@mips.COM Reply-To: mash@mips.COM (John Mashey) Distribution: na Organization: Your Organization Goes Here Lines: 20 In article <6662@amelia.nas.nasa.gov> eugene@wilbur.nas.nasa.gov (Eugene N. Miya) writes: >In article <39284@mips.mips.COM> mash@mips.COM (John Mashey) writes: > >>1) I/O will always be a problem, for all of the usual design reasons, > > "When you can give me disks which rotate significantly > faster than 3600 RPM, then we can start talking." > --Don Senzig > >Time to round up all the "usual" suspects. ;) Seems like the RPM is only suspect #2. I'd observe that N cheap disks running in parallel-transfer designs may have N times the "logical" rotation speed & N times the data xfer rate.... but don't seek in 1/N of the time of one.... so I'd say that disk seek is suspect #1. -- -john mashey DISCLAIMER: UUCP: mash@mips.com OR {ames,decwrl,prls,pyramid}!mips!mash DDD: 408-524-7015, 524-8253 or (main number) 408-720-1700 USPS: MIPS Computer Systems, 930 E. Arques, Sunnyvale, CA 94086