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[INSIGHT OUT 2011] B16 analysis of oracle asm failability(alex)
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[INSIGHT OUT 2011] B16 analysis of oracle asm failability(alex)
1.
Under the Hood
of Oracle ASM: Fault Tolerance Alex Gorbachev Oracle OpenWorld San Francisco, 2011
2.
Alex Gorbachev
• CTO, The Pythian Group • Blogger • OakTable Network member • Oracle ACE Director • BattleAgainstAnyGuess.com • President, Oracle RAC SIG 2 © 2009/2010 Pythian
3.
Why Companies Trust
Pythian • Recognized Leader: • Global industry-leader in remote database administration services and consulting for Oracle, Oracle Applications, MySQL and SQL Server • Work with over 150 multinational companies such as Western Union, Fox Interactive Media, and MDS Inc. to help manage their complex IT deployments • Expertise: • One of the world’s largest concentrations of dedicated, full-time DBA expertise. • Global Reach & Scalability: • 24/7/365 global remote support for DBA and consulting, systems administration, special projects or emergency response 3 8 © 2011 Pythian
4.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
5.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
6.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
7.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
8.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
9.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping 4 © 2009/2010 Pythian
10.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping file1 4 © 2009/2010 Pythian
11.
ASM Striping
• Extents and Allocation Units • Coarse striping & Fine striping • Random striping -> equal distribution • You cannot disable ASM striping file1 file2 4 © 2009/2010 Pythian
12.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
13.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
14.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
15.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
16.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
17.
ASM Rebalancing
• asm_power_limit - rebalancing speed • Async rebalancing in 11.2.0.2 • No auto-magic re-layout based on performance • You can force rebalancing for a DG 5 © 2009/2010 Pythian
18.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
19.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
20.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
21.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
22.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
23.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
24.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
25.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
26.
ASM Mirroring
• Primary extent & secondary extent (mirrored copy) • Write is done to all extent copies • Read is done always from primary extent by default 6 © 2009/2010 Pythian
27.
ASM Failure Groups
• Group of disks can fail at once • Mirror extents between failure groups • Beware of space provisioning SAN 1 SAN 2 7 © 2009/2010 Pythian
28.
ASM Failure Groups
• Group of disks can fail at once • Mirror extents between failure groups • Beware of space provisioning SAN 1 7 © 2009/2010 Pythian
29.
ASM Failure Groups
• Group of disks can fail at once • Mirror extents between failure groups • Beware of space provisioning SAN 1 7 © 2009/2010 Pythian
30.
ASM Redundancy Levels
• Perdiskgroup or per file • DG type external • per file - unprotected only • DG type normal redundancy • per file - unprotected, two-way or three-way • DG type high redundancy • per file - three way only 8 © 2009/2010 Pythian
31.
Read IO Failures
• Can re-read mirror block since 7.3 (initially done for Veritas) • Same happens with ASM - attempt to re-read from another mirror • If successful, repair is done for all mirrors • H/w RAID mirroring doesn’t give that flexibility • Re-read is done by database blindly hopping for the best • Read failures in the database are handled depending on context • ASM can recover not only from media failure errors but from corruptions (bad checksum or wrong SCN) 9 © 2009/2010 Pythian
32.
Read IO Failure
Remapping • Read from secondary extent is performed • Write back to the *same* place is attempted • Disk might do its own block reallocation • If the write to the same location fails then extent relocated and original AU marked as unusable • If the second write fails, then disk set OFFLINE like on any other write failure • Fix occurs only if a reading process can lock that extent • REMAP command - doesn’t detect block corruption but only read media failure 10 © 2009/2010 Pythian
33.
Silent Corruptions of
Secondary Extents • Reads are first attempted from primary extent • Secondary extent is accessed if primary read fails • preferred_read_failure_groups can cause the same issue when some mirror extents are rarely read • Automatic remap is done when failure is detected • ASMCMD REMAP command forces read of an extent so if read media error is produced, remapping happens • REMAP is used best alongside of disk scrubbing features • REMAP doesn’t detect mirrors inconsistencies or logical block corruptions! • AMDU utility - Google for “Luca Canali AMDU” 11 © 2009/2010 Pythian
34.
Partial Writes
• ASM doesn’t use DRL (Dirty Region Logging) • So what happens if one mirror is done and second mirror write didn’t complete during a crash? • Oracle database has an ability to recover corrupted blocks • Oracle database reads both mirrors if corruption is detected and if one of the mirrors is good, repair happens 12 © 2009/2010 Pythian
35.
Disk Failure
• Diskis taken offline on write error - not on read error • On disk failure, ASM reads headers of disks in FG • Whole FG is dismounted rather then individual disks • Multiple FG failures -> dismount DG • ASM also probes partners when disk fails trying to identify failure group pathology • If disks is lost while one of its partners is offline, DG is dismounted • Read failure from disk header -> ASM takes disk offline 13 © 2009/2010 Pythian
36.
What is MTBF?
• Mean Time Before Failure (practically MTTF) • MTBF is inverse of the failure rate during useful life • Thus MTBF is indicator of failure rate but does not predict useful lifetime • Assuming failures have exponential distribution • λ = 1-exp(-t/MTBF) • Annualized Failure Rate (AFR) is λ calculated for time t = 1 year • MTBF of 1,600,000 hours is 182+ years • Doesn’t mean the drive will likely work 182 years! • AFR = 1 - exp(24 * 365 / 1,600,000) = 0.546% 14 © 2009/2010 Pythian
37.
“Bathtub” Failure Rate
Curve 15 © 2009/2010 Pythian
38.
Real AFR &
Utilization (ref Google study) 3 months infant mortality: 10% AFR Assuming exponential distribution, hourly failure rate = 0.001% Poisson process: - exponential distribution - no failure correlation 16 © 2009/2010 Pythian
39.
Hardware Mirroring RAID
and 2nd Disk Failure • Data loss happens only if 2nd failed disk is the mirror of the 1st failed disk. • Window of vulnerability = 5 hours • Time to replace a failed disk • The chance that 2nd mirror fails in the next 5 hours is 0.005% resulting in data loss (based on Google’s data of 10% AFR) 17 © 2009/2010 Pythian
40.
Hardware Mirroring RAID
and 2nd Disk Failure • Data loss happens only if 2nd failed disk is the mirror of the 1st failed disk. • Window of vulnerability = 5 hours • Time to replace a failed disk • The chance that 2nd mirror fails in the next 5 hours is 0.005% resulting in data loss (based on Google’s data of 10% AFR) 17 © 2009/2010 Pythian
41.
Hardware Mirroring RAID
and 2nd Disk Failure • Data loss happens only if 2nd failed disk is the mirror of the 1st failed disk. • Window of vulnerability = 5 hours • Time to replace a failed disk • The chance that 2nd mirror fails in the next 5 hours is 0.005% resulting in data loss (based on Google’s data of 10% AFR) 17 © 2009/2010 Pythian
42.
ASM Mirroring and
2nd Disk Failure 18 © 2009/2010 Pythian
43.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? 18 © 2009/2010 Pythian
44.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? ... any 2nd disk failure would result in data loss 18 © 2009/2010 Pythian
45.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? ... any 2nd disk failure would result in data loss Think Exadata - 168 disks and one fails... then 2nd failure of any of 156 disks will result in data loss 18 © 2009/2010 Pythian
46.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? ... any 2nd disk failure would result in data loss Think Exadata - 168 disks and one fails... then 2nd failure of any of 156 disks will result in data loss 5h window of vulnerability 18 © 2009/2010 Pythian
47.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? ... any 2nd disk failure would result in data loss Think Exadata - 168 disks and one fails... then 2nd failure of any of 156 disks will result in data loss 5h window of vulnerability Chance of data loss = 0.777% 18 © 2009/2010 Pythian
48.
ASM Mirroring and
2nd Disk Failure What if mirrored extent is placed randomly on other disks? ... any 2nd disk failure would result in data loss Think Exadata - 168 disks and one fails... then 2nd failure of any of 156 disks will result in data loss 5h window of vulnerability Chance of data loss = 0.777% 18 © 2009/2010 Pythian
49.
ASM Partnering 19
© 2009/2010 Pythian
50.
ASM Partnering
Each disk is assigned several partner disks (8 partners in 11.2.0.1+ ) _asm_partner_target_disk_part 19 © 2009/2010 Pythian
51.
ASM Partnering
Each disk is assigned several partner disks (8 partners in 11.2.0.1+ ) _asm_partner_target_disk_part Now only one of 8 partner disk failures would cause data loss - i.e. only 0.04% chance of data loss during 5 hours windows of vulnerability after the first disk failure 19 © 2009/2010 Pythian
52.
ASM Partnering
Each disk is assigned several partner disks (8 partners in 11.2.0.1+ ) _asm_partner_target_disk_part Now only one of 8 partner disk failures would cause data loss - i.e. only 0.04% chance of data loss during 5 hours windows of vulnerability after the first disk failure Above is for Google’s 10% AFR. 19 © 2009/2010 Pythian
53.
ASM Partnering
Each disk is assigned several partner disks For manufacturer’s MTBF 1,600,000 hours (large partners in (8 diskgroups): 11.2.0.1+ •AFR = 0.546% _asm_partner_target_disk_part) •data loss chance is 0.002% after first failure, during 5 hours recovery time Now only one of 8 partner disk failures would cause data loss Assumption: disk failures follow Poisson process! - i.e. only 0.04% chance of data loss during 5 hours windows of vulnerability after the first disk failure Above is for Google’s 10% AFR. 19 © 2009/2010 Pythian
54.
Disk Failures in
Real Life - a non-Poisson Process • Failures are correlated in time • Manufacturing defects affecting a batch • Environmental (temperature) • Operational (power surge) • Software bugs • Non-exponential distribution in time 20 © 2009/2010 Pythian
55.
Consider a group
of n disks all coming from the same production batch. We will consider two distinct failure processes: 1. Each disk will be subject to independent failures that will be exponentially distributed with rate λ; these independent failures are the ones that are normally considered in reliability studies. 2. The whole batch will be subject to the unpredictable manifestation of a common defect. This event will be exponentially distributed with rate λ' << λ. It will not result in the immediate failure of any disk but will accelerate disk failures and make them happen at a rate λ'' >> λ. 21 © 2009/2010 Pythian
56.
Probability of Surviving
a Data Loss After a Failure P surv = exp(–nλTR) n - # of partners for a failed ASM disk (8) λ - rate of failure TR - window of vulnerability (5 hours) (normal redundancy) 22 © 2009/2010 Pythian
57.
Random Failure
(No Global Batch Defect Manifestations) P surv = exp(–nλTR) λ - “normal” rate of failure (or 1/MTBF) MTBF = 1000000 hours: P surv = 99.996% Google’s AFR of 10%: P surv = 99.954% (normal redundancy) 23 © 2009/2010 Pythian
58.
Random Failure
(No Global Batch Defect Manifestations) P surv = exp(–nλTR) λ - “normal” rate of failure (or 1/MTBF) MTBF = 1000000 hours: P surv = 99.996% Google’s AFR of 10%: P surv = 99.954% (normal redundancy) 23 © 2009/2010 Pythian
59.
After a Failure
Caused by a Global Defect P surv = exp(–nλ’’TR) λ’’ - accelerated rate of failure λ’’ is one failure per week: P surv = 78.813% λ’’ is one failure per month: P surv = 94.596% (normal redundancy) 24 © 2009/2010 Pythian
60.
After a Failure
Caused by a Global Defect P surv = (1+nλ’’TR)exp(–nλ’’TR) λ’’ - accelerated rate of failure n - 5 hours λ’’ is one failure per week: P surv = 97.58% λ’’ is one failure per month: P surv = 99.85% (high redundancy) 25 © 2009/2010 Pythian
61.
After a Failure
Caused by a Global Defect P surv = (1+nλ’’TR)exp(–nλ’’TR) λ’’ - accelerated rate of failure n - 1 hour λ’’ is one failure per week: P surv = 99.89% λ’’ is one failure per month: P surv = 99.99% (high redundancy) 26 © 2009/2010 Pythian
62.
DEMO
-- target # of partners select ksppstvl from sys.x$ksppi p, sys.x$ksppcv v where p.indx=v.indx and ksppinm='_asm_partner_target_disk_part'; -- disk partners select d.path, p.number_kfdpartner from x$kfdpartner p, v$asm_disk_stat d where p.disk=&disk_no and p.grp=group_number and p.number_kfdpartner=d.disk_number; 27 © 2009/2010 Pythian
63.
Disk Failure Recovery
- ASM vs RAID mirroring • Ask the audience! 28 © 2009/2010 Pythian
64.
Q&A
Email me - gorbachev@pythian.com Read my blog - http://www.pythian.com Follow me on Twitter - @AlexGorbachev Join Pythian fan club on Facebook & LinkedIn 29 © 2009/2010 Pythian