CERN Accelerating science

This website is no longer maintained. Its content may be obsolete. Please visit http://home.cern/ for current CERN information.

CERN home pageCERN home pageDocument Access by ReferenceDocument Access by ReferenceComputer News LetterComputer News LetterCNL issues in year 2000CNL issues in year 2000CNL-2000-002CNL-2000-002CNL-2000-002CNL Help pages

Contents

Editorial Information
Editorial
If you need help
Announcements Physics Computing Desktop Computing Internet Services and Network Scientific Applications and Software Engineering Desktop Publishing The Learning Zone User Documentation Just For Fun ...
Previous:CMS Completes Large Scale Objectivity Production
Next:Desktop Computing
 (See printing version)



AFS File Service, Status and Plans

Bernard Antoine, David Asbury, Olivier Le Moigne, Harry Renshall, Tim Whibley , IT/PDP and IT/TS


During the last twelve months we have been executing a plan to modernise and homogenise the AFS service both at the hardware and software level. By the end of May we had replaced some dozen old file-servers, a mixture of IBM and Sun having disk spaces ranging from 50 to 150GB and not all on secure RAID, by 5 Sun E220 servers each with 300 GB of RAID disk. In June we replaced the three old volume location data base servers by new Sun Netra servers (which no longer have to function also as file servers) and in July the addition of a sixth Sun E220 allowed us to shut down 14 old PCs running a non-standard version of AFS. We also added a large Sun E450 machine to function as a central backup server using an STK DLT 7000 robot and replacing a number of directly attached DLT stackers. All the new machines have fast networking.

All the remaining or new servers are capable of running the same latest level of the AFS server software namely 3.6 patch level 1. This level is multi threaded, so more efficient, and supports backup and restore of volumes up to 8GB in size (the previous limit was 2GB). We successfully migrated to this level on 31 July. When this has proved stable AFS client machines can be brought to the same level.

The final changes planned for this year will be to replace the last two IBM file servers, which use our deprecated FDDI networking, by two more of our standard new configuration. This should happen during August or early September and should be transparent to end users.

We appreciate the patience of our end users during this evolution which has already led to improved reliability and performance. Changes next year should be much more transparent. There are two older Suns that should be replaced then new capacity to be added according to the COCOTIME evaluations currently underway.

The changes have meant that all end user home directory and backed up project directory files are on secure RAID disks. Two disks out of six can fail without losing access (there is a hot spare mechanism). The non-backed up project directory files are also on modern disks but a single disk failure will lose data. It is very important that groups only use the non-backed up space for genuine scratch data.

You can recognise which type of disk a directory is on by the command

fs lq your-directory-name
This will return, under the heading Volume Name, a name beginning:
user.     this is a backed up user home directory
u.        this is a backed up user workspace directory
p.        this is a backed up project directory
q.        this is a non-backed up project directory - SCRATCH ONLY
We also take this opportunity to announce the departure from CERN of Olivier Le Moigne who is returning to French industry. He has made major contributions to the AFS service during his 3 years at CERN not least in training those of us who formed the new AFS team last year. We thank him sincerely for his hard work and dedication and wish him well in his future career.


For matters related to this article please contact the author.
Cnl.Editor@cern.ch


CERN-CNL-2000-002
Vol. XXXV, issue no 2


Last Updated on Fri Aug 18 19:49:20 GMT+04:30 2000.
Copyright © CERN 2000 -- European Organization for Nuclear Research