© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Disk Drive Science
IBM Systems & Technology Group
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Data Storage through the ages…
Today we store data on computer disk drives
Previously we used writing on paper
Before that, marks on clay
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
…Grandmothers
Data capacity ~ 100MB ?
Data rate ~ 10b/s
Error rate ?
Reliability ?
Manufacturing cost ?
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Agenda
Demand for disk storage
What drives areal density?
Aerodynamics
Magnetic recording
Future storage technologies
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Disk Capacity Demand
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
CERN LHC
50 yrs, pure research, technology
(NMR, PET, X-ray imaging, WWW)
27km tunnel, 100m below FR/CH
14TeV hadron collider
Scheduled start April 2007
Storage requirements:
10
9events / sec
1PB/s raw data rate
Hardware filtering to 100MB/s
1PB/yr
By 2008, 15PB/yr
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Disk drive capacity - definitions
B
Byte
=
One letter or number
“A”
KB
Kilobyte
=
1000 B (~ few line e-mail)
MB
Megabyte
=
1000 KB (~ Bible or Qu’ran)
GB
Gigabyte
=
1000 MB (~ human genome)
TB
Terabyte
=
1000 GB (~ Books, annually)
PB
Petabyte
=
1000 TB (Large companies)
EB
Exabyte
=
1000 PB (Human knowledge)
ZB
Zettabyte
=
1000 EB
10
21
B
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Driving Areal density
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Aerodynamics
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Head / Disk interface
Disk Substrate (Aluminium or Glass)
Disk Coating (NiCrMo alloy + 3 atoms Ru)
Slider (Ferrite, Fe/Silicate glass)
Head
Tiny air gap!
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Managing flying height
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Disk Surface Preparation
Head / Slider
Full Surface Texture
Zone Texture
No Texture
Ramp or lift mechanism
Dedicated
landing zone
Smooth
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Disk Aerodynamics - summary
Slider “flies”over the disk surface
(but very close)
“Air Bearing” is formed by the airflow
Slider acts like a racing car in “Ground Effect”
“Landing” in the data zone is a
VERY BAD THING TO DO
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
IBM Systems & Technology Group
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Giant Magnetoresistive effect (GMR)
‘Pinned layer’
‘Free layer’
R
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
Giant Magnetoresistive effect (GMR)
‘Pinned layer’
‘Free layer’
R
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
AntiFerromagnetically Coupled media (“Pixie Dust”)
Demagnetisation energy ~ kT
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation
A Parting shot – How
safe
is your data?
[Even IBM]
Drives can fail – hence RAID
Density is also limited by error rates
Data is a tiny 400MHz signal with S/N ratio close to 1
Soft error rates 1 in 10
6bits
PRML data channel
Partial Response – Maximum Likelihood (look for patterns)
Hard error rates:
‘Server class’ drives (SCSI or Fibre Channel)
1 in 10
15bits
‘Desktop class’ drives (ATA or S-ATA)
1 in 10
14bits
…10% chance of a hard error in reading 1TB for Desktop drives
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
The End
© 2004 IBM Corporation
IBM Systems & Technology Group
| March 2004 |
Chemistry
IBM Systems & Technology Group
Soton.ac.uk 2004 | Disk Drive Science | © 2004 IBM Corporation