Operating Systems: Lecture 20 - Disk Structure, Addressing, and Scheduling, Study notes of Computer Science

A lecture note from a university course on operating systems, specifically focusing on the topic of storage. The lecture covers the need for storage, the structure of disks, disk addressing, disk scheduling, and various types of secondary storage. It also discusses the history of storage and the future of technologies such as solid-state drives and holographic storage.

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Pre 2010

Uploaded on 09/24/2009

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Operating Systems
CMPSC 473
Storage
April 3, 2008 - Lecture 20
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Operating Systems

CMPSC 473

Storage April 3, 2008 - Lecture 20

Outline

  • Disk structure: physical and logical
  • Disk addressing
  • Disk scheduling
  • Management

CERN Particle Collider

Example of Mass Storage

Application

Past & Present in Storage

1956: IBM 305 RAMAC - 5 MB capacity (50 disks, each 24” in diameter) 2008: Seagate Savvio 15K - 73.4 GB capacity, 2.5” diameter

  • can read/write complete works of Shakespeare 15 times per second

Secondary Storage

  • Generally, magnetic disks provide the bulk of secondary storage in systems - future alternative: solid-state drives? - e.g. MacBook Air - MEMS and NEMS(nanotech) - holographic storage - data read from intersecting laser beams www.inphase-technologies.com

Inside a Hard Disk Aluminum (sometimes glass) platters

Disk Operation

  • Platters start moving from rest ( spinup time)
    • lots of mass to start moving
  • Heads find the right track ( seek time)
    • arm powered by actuator motor, accelerates and coasts, slows down and settles on correct track (servo-guided)
  • Disk rotates until correct sector found ( rotational latency ) - contingent on platter diameter and RPM (Savvio 15K rotates 300 times/second)
  • Have to stop the platters ( spindown time)

Addressing Disks

  • Old days: CHS (cylinder-head-sector)
    • supply physical characteristics of the disk to the operating system
    • it specifies exactly where on the physical disk to read and write data
  • Nowadays: cylinders not uniform
    • can store more data on outer tracks than inner tracks (zoned bit recording) - why? - function of constant angular velocity (CAV) vs constant linear velocity (CLV) found in CD-ROM

Disk Scheduling

  • Why does the OS need to schedule?
    • Improves access time (seek time & rotational latency)
    • even with LBA, assumption is that blocks are written in essentially contiguous order
    • maximizes bandwidth
      • transferred bytes / service + transfer time

Disk Scheduling Algorithms

  • Consider the following request queue
    • min cylinder = 0, max cylinder = 199
      • requests at the following cylinders:
      • 98, 183, 37, 122, 14, 124, 65, 67
      • drive head is at cylinder 53

Shortest Seek Time First

(SSTF)

  • Min. seek time from head position (like SJF)
  • Head movement of 236 cylinders

SCAN (Elevator) Algorithm

  • Arm moves from one end of disk to the other then reverses (like an elevator)
  • Head movement of 208 cylinders

C-LOOK Algorithm

  • Like C-SCAN but only seeks to farthest request in queue
  • Returns to lowest request (not start of disk)

Choosing a Disk Scheduling

Algorithm

  • SSTF: increased performance over FCFS
  • SCAN, C-SCAN: good for heavy loads
    • less chance of starvation
  • C-LOOK: good overall
  • File allocation plays a role
    • contiguous allocation limits head movement
  • Note: only considering seek time
    • rotational latency also important but hard for OS to know (doesn’t have physical drive characteristics) - drive controllers implement some queueing and request coalescing