Chapter 12. Advanced Administration

This chapter revisits some aspects we already described, with a different perspective: instead of installing one single computer, we will study mass-deployment systems; instead of creating RAID or LVM volumes at install time, we'll learn to do it by hand so we can later revise our initial choices. Finally, we will discuss monitoring tools and virtualization techniques. As a consequence, this chapter is more particularly targeting professional administrators, and focuses somewhat less on individuals responsible for their home network.

12.1. RAID and LVM

Chapter 4, Installation presented these technologies from the point of view of the installer, and how it integrated them to make their deployment easy from the start. After the initial installation, an administrator must be able to handle evolving storage space needs without having to resort to an expensive reinstallation. They must therefore master the required tools for manipulating RAID and LVM volumes.

RAID and LVM are both techniques to abstract the mounted volumes from their physical counterparts (actual hard-disk drives or partitions thereof); the former secures the data by introducing redundancy, the latter makes data management more flexible and independent of the actual size of the underlying disks. In both cases, the system ends up with new block devices, which can be used to create filesystems or swap space, without necessarily having them mapped to one physical disk. RAID and LVM come from quite different backgrounds, but their functionality can overlap somewhat, which is why they are ofter mentioned together.

PERSPECTIVE Btrfs combines LVM and RAID

While LVM and RAID are two distinct kernel subsystems that come between the disk block devices and their filesystems, btrfs is a new filesystem, initially developed at Oracle, that purports to combine the featuresets of LVM and RAID and much more. It is mostly functional, although still tagged “experimental” because its development is incomplete (some features aren't implemented yet).

→ http://btrfs.wiki.kernel.org/

Among the noteworthy features are the ability to take a snapshot of a filesystem tree at any point in time. This snapshot copy doesn't initially use any disk space, the data only being duplicated when one of the copies is modified. The filesystem also handles transparent compression of files, and checksums ensure the integrity of all stored data.

In both the RAID and LVM cases, the kernel provides a block device file, similar to the ones corresponding to a hard disk drive or a partition. When an application, or another part of the kernel, requires access to a block of such a device, the appropriate subsystem routes the block to the relevant physical layer. Depending on the configuration, this block can be stored on one or several physical disks, and its physical location may not be directly correlated to the location of the block in the logical device.

12.1.1. Software RAID

RAID means Redundant Array of Independent Disks. The goal of this system is to prevent data loss in case of hard disk failure. The general principle is quite simple: data are stored on several physical disks instead of only one, with a configurable level of redundancy. Depending on this amount of redundancy, and even in the event of an unexpected disk failure, data can be losslessly reconstructed from the remaining disks.

RAID can be implemented either by dedicated hardware (RAID modules integrated into SCSI or SATA controller cards) or by software abstraction (the kernel). Whether hardware or software, a RAID system with enough redundancy can transparently stay operational when a disk fails; the upper layers of the stack (applications) can even keep accessing the data in spite of the failure. Of course, this “degraded mode” can have an impact on performance, and redundancy is reduced, so a further disk failure can lead to data loss. In practice, therefore, one will strive to only stay in this degraded mode for as long as it takes to replace the failed disk. Once the new disk is in place, the RAID system can reconstruct the required data so as to return to a safe mode. The applications won't notice anything, apart from potentially reduced access speed, while the array is in degraded mode or during the reconstruction phase.

12.1.1.1. Different RAID Levels

RAID has actually several levels, differenciated by their layout and the amount of redundancy they provide. The more redundant, the more failure-proof, since the system will be able to keep working with more failed disks. The counterpart is that the usable space shrinks; seen the other way, more disks will be needed to store the same amount of data.

Linear RAID: Even though the kernel's RAID subsystem allows creating “linear RAID”, this is not proper RAID, since this setup doesn't involve any redundancy. The kernel merely aggregates several disks end-to-end and provides the resulting aggregated volume as one virtual disk (one block device). That's about its only function. This setup is rarely used by itself (see later for the exceptions), especially since the lack of redundancy means that one disk failing makes the whole aggregate, and therefore all the data, unavailable.
RAID-0: This level doesn't provide any redundancy either, but disks aren't simply stuck on end one after another: they are divided in stripes, and the blocks on the virtual device are stored on stripes on alternating physical disks. In a two-disk RAID-0 setup, for instance, even-numbered blocks of the virtual device will be stored on the first physical disk, while odd-numbered blocks will end up on the second physical disk.
This system doesn't aim at increasing reliability, since (as in the linear case) the availability of all the data is jeopardized as soon as one disk fails, but at increasing performance: during sequential access to large amounts of contiguous data, the kernel will be able to read from both disks (or write to them) in parallel, which increases the data transfer rate. However, RAID-0 use is shrinking, its niche being filled by LVM (see later).
RAID-1: This level, also known as “RAID mirroring”, is both the simplest and the most widely used setup. In its standard form, it uses two physical disks of the same size, and provides a logical volume of the same size again. Data are stored identically on both disks, hence the “mirror” nickname. When one disk fails, the data is still available on the other. For really critical data, RAID-1 can of course be set up on more than two disks, with a direct impact on the ratio of hardware cost versus available payload space.
NOTE Disks and cluster sizes
If two disks of different sizes are set up in a mirror, the bigger one will not be fully used, since it will contain the same data as the smallest one and nothing more. The useful available space provided by a RAID-1 volume therefore matches the size of the smallest disk in the array. This still holds for RAID volumes with a higher RAID level, even though redundancy is stored differently.
It is therefore important, when setting up RAID arrays (except for RAID-0 and “linear RAID”), to only assemble disks of identical, or very close, sizes, to avoid wasting resources.
NOTE Spare disks
RAID levels that include redundancy allow assigning more disks than required to an array. The extra disks are used as spares when one of the main disks fails. For instance, in a mirror of two disks plus one spare, if one of the first two disks fails, the kernel will automatically (and immediately) reconstruct the mirror using the spare disk, so that redundancy stays assured after the reconstruction time. This can be used as another kind of safeguard for critical data.
One would be forgiven for wondering how this is better than simply mirroring on three disks to start with. The advantage of the “spare disk” configuration is that the spare disk can be shared across several RAID volumes. For instance, one can have three mirrored volumes, with redundancy assured even in the event of one disk failure, with only seven disks (three pairs, plus one shared spare), instead of the nine disks that would be required by three triplets.
This RAID level, although expensive (since only half of the physical storage space, at best, is useful), is widely used in practice. It is simple to understand, and it allows very simple backups: since both disks have identical contents, one of them can be temporarily extracted with no impact on the working system. Read performance is often increased since the kernel can read half of the data on each disk in parallel, while write performance isn't too severely degraded. In case of a RAID-1 array of N disks, the data stays available even with N-1 disk failures.
RAID-4: This RAID level, not widely used, uses N disks to store useful data, and an extra disk to store redundancy information. If that disk fails, the system can reconstruct its contents from the other N. If one of the N data disks fails, the remaining N-1 combined with the “parity” disk contain enough information to reconstruct the required data.
RAID-4 isn't too expensive since it only involves a one-in-N increase in costs and has no noticeable impact on read performance, but writes are slowed down. Furthermore, since a write to any of the N disks also involves a write to the parity disk, the latter sees many more writes than the former, and its lifespan can shorten dramatically as a consequence. Data on a RAID-4 array is safe only up to one failed disk (of the N+1).
RAID-5: RAID-5 addresses the asymmetry issue of RAID-4: parity blocks are spread over all of the N+1 disks, with no single disk having a particular role.
Read and write performance are identical to RAID-4. Here again, the system stays functional with up to one failed disk (of the N+1), but no more.
RAID-6: RAID-6 can be considered an extension of RAID-5, where each series of N blocks involves two redundancy blocks, and each such series of N+2 blocks is spread over N+2 disks.
This RAID level is slightly more expensive than the previous two, but it brings some extra safety since up to two drives (of the N+2) can fail without compromising data availability. The counterpart is that write operations now involve writing one data block and two redundancy blocks, which makes them even slower.
RAID-1+0: This isn't stricly speaking, a RAID level, but a stacking of two RAID groupings. Starting from 2×N disks, one first sets them up by pairs into N RAID-1 volumes; these N volumes are then aggregated into one, either by “linear RAID” or (increasingly) by LVM. This last case goes farther than pure RAID, but there's no problem with that.
RAID-1+0 can survive multiple disk failures: up to N in the 2×N array described above, provided that at least one disk keeps working in each of the RAID-1 pairs.
GOING FURTHER RAID-10
RAID-10 is generally considered a synonym of RAID-1+0, but a Linux specificity makes it actually a generalization. This setup allows a system where each block is stored on two different disks, even with an odd number of disks, the copies being spread out along a configurable model.
Performances will vary depending on the chosen repartition model and redundancy level, and of the workload of the logical volume.

Obviously, the RAID level will be chosen according to the constraints and requirements of each application. Note that a single computer can have several distinct RAID arrays with different configurations.

12.1.1.2. Setting up RAID

Setting up RAID volumes requires the mdadm package; it provides the mdadm command, which allows creating and manipulating RAID arrays, as well as scripts and tools integrating it to the rest of the system, including the monitoring system.

Our example will be a server with a number of disks, some of which are already used, the rest being available to setup RAID. We initially have the following disks and partitions:

the sda disk, 4 GB, is entirely available;
the sde disk, 4 GB, is also entirely available;
on the sdg disk, only partition sdg2 (about 4 GB) is available;
finally, a sdh disk, still 4 GB, entirely available.

We're going to use these physical elements to build two volumes, one RAID-0 and one mirror (RAID-1). Let's start with the RAID-0 volume:

# mdadm --create /dev/md0 --level=0 --raid-devices=2 /dev/sda /dev/sde
mdadm: Defaulting to version 1.2 metadata
mdadm: array /dev/md0 started.
# mdadm --query /dev/md0
/dev/md0: 8.00GiB raid0 2 devices, 0 spares. Use mdadm --detail for more detail.
# mdadm --detail /dev/md0
/dev/md0:
        Version : 1.2
  Creation Time : Thu Sep 30 15:21:15 2010
     Raid Level : raid0
     Array Size : 8388480 (8.00 GiB 8.59 GB)
   Raid Devices : 2
  Total Devices : 2
    Persistence : Superblock is persistent

    Update Time : Thu Sep 30 15:21:15 2010
          State : active
 Active Devices : 2
Working Devices : 2
 Failed Devices : 0
  Spare Devices : 0

     Chunk Size : 512K

           Name : squeeze:0  (local to host squeeze)
           UUID : 0012a273:cbdb8b83:0ee15f7f:aec5e3c3
         Events : 0

    Number   Major   Minor   RaidDevice State
       0       8        0        0      active sync   /dev/sda
       1       8       64        1      active sync   /dev/sde
# mkfs.ext4 /dev/md0

mke2fs 1.41.12 (17-May-2010)
Filesystem label=
OS type: Linux
Block size=4096 (log=2)
Fragment size=4096 (log=2)
Stride=0 blocks, Stripe width=0 blocks
524288 inodes, 2097152 blocks
104857 blocks (5.00%) reserved for the super user
First data block=0
Maximum filesystem blocks=2147483648
55 block groups
32768 blocks per group, 32768 fragments per group
8160 inodes per group
Superblock backups stored on blocks: 
        32768, 98304, 163840, 229376, 294912, 819200, 884736, 1605632

Writing inode tables: done
Creating journal (32768 blocks): done
Writing superblocks and filesystem accounting information: done

This filesystem will be automatically checked every 26 mounts or
180 days, whichever comes first.  Use tune2fs -c or -i to override.
# mkdir /srv/raid-0
# mount /dev/md0 /srv/raid-0
# df -h /srv/raid-0
Filesystem            Size  Used Avail Use% Mounted on
/dev/md0              8.0G  249M  7.4G   4% /srv/raid-0

The mdadm --create command requires several parameters: the name of the volume to create (/dev/md*, with MD standing for Multiple Device), the RAID level, the number of disks (which is compulsory despite being mostly meaningful only with RAID-1 and above), and the physical drives to use. Once the device is created, we can use it like we'd use a normal partition, create a filesystem on it, mount that filesystem, and so on. Note that our creation of a RAID-0 volume on md0 is nothing but coincidence, and the numbering of the array doesn't need to be correlated to the chosen amount of redundancy.

Creation of a RAID-1 follows a similar fashion, the differences only being noticeable after the creation:

# mdadm --create /dev/md1 --level=1 --raid-devices=2 /dev/sdg2 /dev/sdh
mdadm: largest drive (/dev/sdg2) exceed size (4194240K) by more than 1%
Continue creating array? y
mdadm: array /dev/md1 started.
# mdadm --query /dev/md1
/dev/md1: 4.00GiB raid1 2 devices, 0 spares. Use mdadm --detail for more detail.
# mdadm --detail /dev/md1
/dev/md1:
        Version : 1.2
  Creation Time : Thu Sep 30 15:39:13 2010
     Raid Level : raid1
     Array Size : 4194240 (4.00 GiB 4.29 GB)
  Used Dev Size : 4194240 (4.00 GiB 4.29 GB)
   Raid Devices : 2
  Total Devices : 2
    Persistence : Superblock is persistent

    Update Time : Thu Sep 30 15:39:26 2010
          State : active, resyncing
 Active Devices : 2
Working Devices : 2
 Failed Devices : 0
  Spare Devices : 0

 Rebuild Status : 10% complete

           Name : squeeze:1  (local to host squeeze)
           UUID : 20a8419b:41612750:b9171cfe:00d9a432
         Events : 27

    Number   Major   Minor   RaidDevice State
       0       8       98        0      active sync   /dev/sdg2
       1       8      112        1      active sync   /dev/sdh
# mdadm --detail /dev/md1
/dev/md1:
[...]
          State : active
[...]

A few remarks are in order. First, mdadm notices that the physical elements have different sizes; since this implies that some space will be lost on the bigger element, a confirmation is required.

More importantly, note the state of the mirror. The normal state of a RAID mirror is that both disks have exactly the same contents. However, nothing guarantees this is the case when the volume is first created. The RAID subsystem will therefore provide that guarantee itself, and there will be a synchronisation phase as soon as the RAID device is created. After some time (the exact amount will depend on the actual size of the disks…), the RAID array switches to the “active” state. Note that during this reconstruction phase, the mirror is in a degraded mode, and redundancy isn't assured. A disk failing during that risk window could lead to losing all the data. Large amounts of critical data, however, are rarely stored on a freshly created RAID array before its initial synchronisation. Note that even in degraded mode, the /dev/md1 is usable, and a filesystem can be created on it, as well as some data copied on it.

TIP Starting a mirror in degraded mode

Sometimes two disks are not immediately available when one wants to start a RAID-1 mirror, for instance because one of the disks one plans to include is already used to store the data one wants to move to the array. In such circumstances, it is possible to deliberately create a degraded RAID-1 array by passing missing instead of a device file as one of the arguments to mdadm. Once the data have been copied to the “mirror”, the old disk can be added to the array. A synchronisation will then take place, giving us the redundancy that was wanted in the first place.

TIP Setting up a mirror without synchronisation

RAID-1 volumes are often created to be used as a new disk, often considered blank. The actual initial contents of the disk is therefore not very relevant, since one only needs to know that the data written after the creation of the volume, in particular the filesystem, can be accessed later.

One might therefore wonder about the point of synchronising both disks at creation time. Why care whether the contents are identical on zones of the volume that we know will only be read after we have written to them?

Fortunately, this synchronisation phase can be avoided by passing the --assume-clean option to mdadm. However, this option can lead to surprises in cases where the initial data will be read (for instance if a filesystem is already present on the physical disks), which is why it isn't enabled by default.

Now let's see what happens when one of the elements of the RAID-1 array fails. mdadm, in particular its --fail option, allows simulating such a disk failure:

# mdadm /dev/md1 --fail /dev/sdh
mdadm: set /dev/sdh faulty in /dev/md1
# mdadm --detail /dev/md1
/dev/md1:
[...]
    Update Time : Thu Sep 30 15:45:50 2010
          State : active, degraded
 Active Devices : 1
Working Devices : 1
 Failed Devices : 1
  Spare Devices : 0

           Name : squeeze:1  (local to host squeeze)
           UUID : 20a8419b:41612750:b9171cfe:00d9a432
         Events : 35

    Number   Major   Minor   RaidDevice State
       0       8       98        0      active sync   /dev/sdg2
       1       0        0        1      removed

       2       8      112        -      faulty spare  /dev/sdh

The contents of the volume are still accessible (and, if it's mounted, the applications don't notice a thing), but the data safety isn't assured anymore: should the sdg disk fail in turn, the data would be lost. We want to avoid that risk, so we'll replace the failed disk with a new one, sdi:

# mdadm /dev/md1 --add /dev/sdi
mdadm: added /dev/sdi
# mdadm --detail /dev/md1
/dev/md1:
[...]
   Raid Devices : 2
  Total Devices : 3
    Persistence : Superblock is persistent

    Update Time : Thu Sep 30 15:52:29 2010
          State : active, degraded, recovering
 Active Devices : 1
Working Devices : 2
 Failed Devices : 1
  Spare Devices : 1

 Rebuild Status : 45% complete

           Name : squeeze:1  (local to host squeeze)
           UUID : 20a8419b:41612750:b9171cfe:00d9a432
         Events : 53

    Number   Major   Minor   RaidDevice State
       0       8       98        0      active sync   /dev/sdg2
       3       8      128        1      spare rebuilding   /dev/sdi

       2       8      112        -      faulty spare   /dev/sdh
# [...]
[...]
# mdadm --detail /dev/md1
/dev/md1:
[...]
    Update Time : Thu Sep 30 15:52:35 2010
          State : active
 Active Devices : 2
Working Devices : 2
 Failed Devices : 1
  Spare Devices : 0

           Name : squeeze:1  (local to host squeeze)
           UUID : 20a8419b:41612750:b9171cfe:00d9a432
         Events : 71

    Number   Major   Minor   RaidDevice State
       0       8       98        0      active sync   /dev/sdg2
       1       8      128        1      active sync   /dev/sdi

       2       8      112        -      faulty spare   /dev/sdh

Here again, the kernel automatically triggers a reconstruction phase during which the volume, although still accessible, is in a degraded mode. Once the reconstruction is over, the RAID array is back to a normal state. One can then tell the system that the sdh disk is about to be removed from the array, so as to end up with a classical RAID mirror on two disks:

# mdadm /dev/md1 --remove /dev/sdh
mdadm: hot removed /dev/sdh from /dev/md1
# mdadm --detail /dev/md1
/dev/md1:
[...]
    Number   Major   Minor   RaidDevice State
       0       8       98        0      active sync   /dev/sdg2
       1       8      128        1      active sync   /dev/sdi

From then on, the drive can be physically removed when the server is next switched off, or even hot-removed when the hardware configuration allows hot-swap. Such configurations include some SCSI controllers, most SATA disks, and external drives operating on USB or Firewire.

12.1.1.3. Backing up the Configuration

Most of the meta-data concerning RAID volumes are saved directly on the disks that make up these arrays, so that the kernel can detect the arrays and their components and assemble them automatically when the system starts up. However, backing up this configuration is encouraged, because this detection isn't fail-proof, and it's only expected that it will fail precisely in sensitive circumstances. In our example, if the sdh disk failure had been real (instead of simulated) and the system had been restarted without removing this sdh disk, this disk could start working again due to having been probed during the reboot. The kernel would then have three physical elements, each claiming to contain half of the same RAID volume. Another source of confusion can come when RAID volumes from two servers are consolidated onto one server only. If these arrays were running normally before the disks were moved, the kernel would be able to detect and reassemble the pairs properly; but if the moved disks had been aggregated into an md1 on the old server, and the new server already has an md1, one of the mirrors would be renamed.

Backing up the configuration is therefore important, if only for reference. The standard way to do it is by editing the /etc/mdadm/mdadm.conf file, an example of which is listed here:

Example 12.1. `mdadm` configuration file

# mdadm.conf
#
# Please refer to mdadm.conf(5) for information about this file.
#

# by default, scan all partitions (/proc/partitions) for MD superblocks.
# alternatively, specify devices to scan, using wildcards if desired.
DEVICE /dev/sd*

# auto-create devices with Debian standard permissions
CREATE owner=root group=disk mode=0660 auto=yes

# automatically tag new arrays as belonging to the local system
HOMEHOST <system>

# instruct the monitoring daemon where to send mail alerts
MAILADDR root

ARRAY /dev/md0 metadata=1.2 name=squeeze:0 UUID=6194b63f:69a40eb5:a79b7ad3:c91f20ee
ARRAY /dev/md1 metadata=1.2 name=squeeze:1 UUID=20a8419b:41612750:b9171cfe:00d9a432

One of the most useful details is the DEVICE option, which lists the devices where the system will automatically look for components of RAID volumes at start-up time. In our example, we replaced the default value, partitions, with an explicit list of device files, since we chose to use entire disks and not only partitions, for some volumes.

The last two lines in our example are those allowing the kernel to safely pick which volume number to assign to which array. The metadata stored on the disks themselves are enough to re-assemble the volumes, but not to determine the volume number (and the matching /dev/md* device name).

Fortunately, these lines can be generated automatically:

# mdadm --misc --detail --brief /dev/md?
ARRAY /dev/md0 metadata=1.2 name=squeeze:0 UUID=6194b63f:69a40eb5:a79b7ad3:c91f20ee
ARRAY /dev/md1 metadata=1.2 name=squeeze:1 UUID=20a8419b:41612750:b9171cfe:00d9a432

The contents of these last two lines doesn't depend on the list of disks included in the volume. It is therefore not necessary to regenerate these lines when replacing a failed disk with a new one. On the other hand, care must be taken to update the file when creating or deleting a RAID array.

12.1.2. LVM

LVM, the Logical Volume Manager, is another approach to abstracting logical volumes from their physical supports, which focuses on increasing flexibility rather than increasing reliability. LVM allows changing a logical volume transparently as far as the applications are concerned; for instance, it is possible to add new disks, migrate the data to them, and remove the old disks, without unmounting the volume.

12.1.2.1. LVM Concepts

This flexibility is attained by a level of abstraction involving three concepts.

First, the PV (Physical Volume) is the entity closest to the hardware: it can be partitions on a disk, or a full disk, or even any other block device. Note that when a physical element is set up to be a PV for LVM, it should only be accessed via LVM, otherwise the system will get confused.

A number of PVs can be clustered in a VG (Volume Group), which can be compared to disks both virtual and extensible. VGs are abstract, and don't appear in a device file in the /dev hierarchy, so there's no risk of using them directly.

The third kind of object is the LV (Logical Volume), which is a chunk of a VG; if we keep the VG-as-disk analogy, the LV compares to a partition. The LV appear as block device with an entry in /dev, and it can be used as any other physical partition can be (most commonly, to host a filesystem or swap space).

The important thing is that the splitting of a VG into LVs is entirely independent of its physical components (the PVs). A VG with only a single physical component (a disk for instance) can be split into a dozen logical volumes; similarly, a VG can use several physical disks and appear as a single large logical volume. The only constraint is that obviously the total size allocated to LVs can't be bigger than the total capacity of the PVs in the volume group.

It often makes sense, however, to have some kind of homogeneity among the physical components of a VG, and to split the VG into logical volumes that will have similar usage patterns. For instance, if the available hardware includes fast disks and slower disks, the fast ones could be clustered into one VG and the slower ones into another; chunks of the first one can then be assigned to applications requiring fast data access, while the second one will be kept for less demanding tasks.

In any case, keep in mind that an LV isn't particularly attached to any one PV. It is possible to influence where the data from an LV are physically stored, but this possibility isn't required for day-to-day use. On the contrary: when the set of physical components of a VG evolves, the physical storage locations corresponding to a particular LV can be migrated across disks (while staying within the PVs assigned to the VG, of course).

12.1.2.2. Setting up LVM

Let us now follow, step by step, the process of setting up LVM for a typical use case: we want to simplify a complex storage situation. Such a situation usually happens after some long and convoluted history of accumulated temporary measures. For the purposes of illustration, we'll consider a server where the storage needs have changed over time, ending up in a maze of available partitions split over several partially used disks. In more concrete terms, the following partitions are available:

on the sdb disk, a sdb2 partition, 4 GB;
on the sdc disk, a sdc3 partition, 3 GB;
the sdd disk, 4 GB, in fully available;
on the sdf disk, a sdf1 partition, 4 GB; and a sdf2 partition, 5 GB.

In addition, let's assume that disks sdb and sdf are faster than the other two.

Our goal is to set up three logical volumes for three different applications: a file server requiring 5 GB of storage space, a database (1 GB) and some space for back-ups (12 GB). The first two need good performance, but back-ups are less critical in terms of access speed. All these constraints prevent the use of partitions on their own; using LVM can abstract the physical size of the devices, so the only limit is the total available space.

The required tools are in the lvm2 package and its dependencies. When they're installed, setting up LVM takes three steps, matching the three levels of concepts.

First, we prepare the physical volumes using pvcreate:

# pvdisplay
# pvcreate /dev/sdb2
  Physical volume "/dev/sdb2" successfully created
# pvdisplay

  "/dev/sdb2" is a new physical volume of "4,00 GiB"
  --- NEW Physical volume ---
  PV Name               /dev/sdb2
  VG Name
  PV Size               4.00 GiB
  Allocatable           NO
  PE Size (KByte)       0
  Total PE              0
  Free PE               0
  Allocated PE          0
  PV UUID               9JuaGR-W7jc-pNgj-NU4l-2IX1-kUJ7-m8cRim

# for i in sdc3 sdd sdf1 sdf2 ; do pvcreate /dev/$i ; done
  Physical volume "/dev/sdc3" successfully created
  Physical volume "/dev/sdd" successfully created
  Physical volume "/dev/sdf1" successfully created
  Physical volume "/dev/sdf2" successfully created
# pvdisplay -C
  PV         VG   Fmt  Attr PSize PFree
  /dev/sdb2       lvm2 a-   4.00g 4.00g
  /dev/sdc3       lvm2 a-   3.09g 3.09g
  /dev/sdd        lvm2 a-   4.00g 4.00g
  /dev/sdf1       lvm2 a-   4.10g 4.10g
  /dev/sdf2       lvm2 a-   5.22g 5.22g

So far, so good; note that a PV can be set up on a full disk as well as on individual partitions of it. As shown above, the pvdisplay command lists the existing PVs, with two possible output formats.

Now let's assemble these physical elements into VGs using vgcreate. We'll gather only PVs from the fast disks into a vg_critical VG; the other VG, vg_normal, will also include slower elements.

# vgdisplay
# vgcreate vg_critical /dev/sdb2 /dev/sdf1
  Volume group "vg_critical" successfully created
# vgdisplay
  --- Volume group ---
  VG Name               vg_critical
  System ID
  Format                lvm2
  Metadata Areas        2
  Metadata Sequence No  1
  VG Access             read/write
  VG Status             resizable
  MAX LV                0
  Cur LV                0
  Open LV               0
  Max PV                0
  Cur PV                2
  Act PV                2
  VG Size               8.14 GB
  PE Size               4.00 MB
  Total PE              2084
  Alloc PE / Size       0 / 0
  Free  PE / Size       2084 / 8.14 GB
  VG UUID               6eG6BW-MmJE-KB0J-dsB2-52iL-N6eD-1paeo8

# vgcreate vg_normal /dev/sdc3 /dev/sdd /dev/sdf2
  Volume group "vg_normal" successfully created
# vgdisplay -C
  VG          #PV #LV #SN Attr   VSize  VFree
  vg_critical   2   0   0 wz--n-  8.14g  8.14g
  vg_normal     3   0   0 wz--n- 12.30g 12.30g

Here again, commands are rather straightforward (and vgdisplay proposes two output formats). Note that it's quite possible to use two partitions of the same physical disk into two different VGs. Note also that we used a vg_ prefix to name our VGs, but it's nothing more than a convention.

We now have two “virtual disks”, sized about 8 GB and 12 GB, respectively. Let's now carve them up into “virtual partitions” (LVs). This involves the lvcreate command, and a slightly more complex syntax:

# lvdisplay
# lvcreate -n lv_files -L 5G vg_critical
  Logical volume "lv_files" created
# lvdisplay
  --- Logical volume ---
  LV Name                /dev/vg_critical/lv_files
  VG Name                vg_critical
  LV UUID                4QLhl3-2cON-jRgQ-X4eT-93J4-6Ox9-GyRx3M
  LV Write Access        read/write
  LV Status              available
  # open                 0
  LV Size                5.00 GB
  Current LE             1280
  Segments               2
  Allocation             inherit
  Read ahead sectors     auto
  - currently set to     256
  Block device           253:0

# lvcreate -n lv_base -L 1G vg_critical
  Logical volume "lv_base" created
# lvcreate -n lv_backups -L 12G vg_normal
  Logical volume "lv_backups" created
# lvdisplay -C
  LV         VG          Attr   LSize  Origin Snap%  Move Log Copy%  Convert
  lv_base    vg_critical -wi-a-  1.00G
  lv_files   vg_critical -wi-a-  5.00G
  lv_backups vg_normal   -wi-a- 12.00G

Two parameters are required when creating logical volumes; they must be passed to the lvcreate as options. The name of the LV to be created is specified with the -n option, and its size is generally given using the -L option. We also need to tell the command what VG to operate on, of course, hence the last parameter on the command line.

GOING FURTHER `lvcreate` options

The lvcreate command has several options to allow tweaking how the LV is created.

Let's first describe the -l option, with which the LV's size can be given as a number of blocks (as opposed to the “human” units we used above). These blocks (called PEs, physical extents, in LVM terms) are contiguous units of storage space in PVs, and they can't be split across LVs. When one wants to define storage space for an LV with some precision, for instance to use the full available space, the -l option will probably be preferred over -L.

It's also possible to hint at the physical location of an LV, so that its extents are stored on a particular PV (while staying within the ones assigned to the VG, of course). Since we know that sdb is faster than sdf, we may want to store the lv_base there if we want to give an advantage to the database server compared to the file server. The command line becomes: lvcreate -n lv_base -L 1G vg_critical /dev/sdb2. Note that this command can fail if the PV doesn't have enough free extents. In our example, we would probably have to create lv_base before lv_files to avoid this situation – or free up some space on sdb2 with the pvmove command.

Logical volumes, once created, end up as block device files in /dev/mapper/:

# ls -l /dev/mapper
total 0
crw-rw---- 1 root root  10, 59  5 oct.  17:40 control
lrwxrwxrwx 1 root root       7  5 oct.  18:14 vg_critical-lv_base -> ../dm-1
lrwxrwxrwx 1 root root       7  5 oct.  18:14 vg_critical-lv_files -> ../dm-0
lrwxrwxrwx 1 root root       7  5 oct.  18:14 vg_normal-lv_backups -> ../dm-2
# ls -l /dev/dm-*
brw-rw---- 1 root disk 253,  0  5 oct.  18:14 /dev/dm-0
brw-rw---- 1 root disk 253,  1  5 oct.  18:14 /dev/dm-1
brw-rw---- 1 root disk 253,  2  5 oct.  18:14 /dev/dm-2

NOTE Autodetecting LVM volumes

When the computer boots, the /etc/init.d/lvm script scans the available devices; those that have been initialised as physical volumes for LVM are registered into the LVM subsystem, those that belong to volume groups are assembled, and the relevant logical volumes are started and made available. There is therefore no need to edit configuration files when creating or modifying LVM volumes.

Note, however, that the layout of the LVM elements (physical and logical volumes, and volume groups) is backed up in /etc/lvm/backup, which can be useful in case of a problem (or just to sneak a peek under the hood).

To make things easier, convenience symbolic links are also created in directories matching the VGs:

# ls -l /dev/vg_critical
total 0
lrwxrwxrwx 1 root root 7  5 oct.  18:14 lv_base -> ../dm-1
lrwxrwxrwx 1 root root 7  5 oct.  18:14 lv_files -> ../dm-0
# ls -l /dev/vg_normal
total 0
lrwxrwxrwx 1 root root 7  5 oct.  18:14 lv_backups -> ../dm-2

The LVs can then be used exactly like standard partitions:

# mkfs.ext4 /dev/vg_normal/lv_backups
mke2fs 1.41.12 (17-May-2010)
Filesystem label=
OS type: Linux
Block size=4096 (log=2)
[...]
This filesystem will be automatically checked every 34 mounts or
180 days, whichever comes first.  Use tune2fs -c or -i to override.
# mkdir /srv/backups
# mount /dev/vg_normal/lv_backups /srv/backups
# df -h /srv/backups
Filesystem            Size  Used Avail Use% Mounted on
/dev/mapper/vg_normal-lv_backups
                       12G  159M   12G   2% /srv/backups
# [...]
[...]
# cat /etc/fstab
[...]
/dev/vg_critical/lv_base    /srv/base       ext4
/dev/vg_critical/lv_files   /srv/files      ext4
/dev/vg_normal/lv_backups   /srv/backups    ext4

From the applications' point of view, the myriad small partitions have now been abstracted into one large 12 GB volume, with a friendlier name.

12.1.2.3. LVM Over Time

Even though the ability to aggregate partitions or physical disks is convenient, this is not the main advantage brought by LVM. The flexibility it brings is especially noticed as time passes, when needs evolve. In our example, let's assume that new large files must be stored, and that the LV dedicated to the file server is too small to contain them. Since we haven't used the whole space available in vg_critical, we can grow lv_files. For that purpose, we'll use the lvresize command, then resize2fs to adapt the filesystem accordingly:

# df -h /srv/files/
Filesystem            Size  Used Avail Use% Mounted on/dev/mapper/vg_critical-lv_files                      5.0G  4.6G  142M  98% /srv/files
# lvdisplay -C vg_critical/lv_files
  LV       VG          Attr   LSize Origin Snap%  Move Log Copy%  Convert
  lv_files vg_critical -wi-ao 5.00g
# vgdisplay -C vg_critical
  VG          #PV #LV #SN Attr   VSize VFree
  vg_critical   2   2   0 wz--n- 8.14g 2.14g
# lvresize -L 7G vg_critical/lv_files
  Extending logical volume lv_files to 7.00 GB
  Logical volume lv_files successfully resized
# lvdisplay -C vg_critical/lv_files
  LV       VG          Attr   LSize Origin Snap%  Move Log Copy%  Convert
  lv_files vg_critique -wi-ao 7.00g
# resize2fs /dev/vg_critical/lv_files
resize2fs 1.41.12 (17-May-2010)
Filesystem at /dev/vg_critical/lv_files is mounted on /srv/files; on-line resizing required
old desc_blocks = 1, new_desc_blocks = 1
Performing an on-line resize of /dev/vg_critical/lv_files to 1835008 (4k) blocks.
The filesystem on /dev/vg_critical/lv_files is now 1835008 blocks long.

# df -h /srv/files/
Filesystem            Size  Used Avail Use% Mounted on
/dev/mapper/vg_critical-lv_files
                      6.9G  4.6G  2.1G  70% /srv/files

CAUTION Resizing filesystems

Not all filesystems can be resized online; resizing a volume can therefore require unmounting the filesystem first and remounting it afterwards. Of course, if one wants to shrink the space allocated to an LV, the filesystem must be shrunk first; the order is reversed when the resizing goes in the other direction: the logical volume must be grown before the filesystem on it. It's rather straightforward, since at no time must the filesystem size be larger than the block device where it resides (whether that device is a physical partition or a logical volume).

The ext3, ext4 and xfs filesystems can be grown online, without unmounting; shrinking requires an unmount. The reiserfs filesystem allows online resizing in both directions. The venerable ext2 allows neither, and always requires unmounting.

We could proceed in a similar fashion to extend the volume hosting the database, only we've reached the VG's available space limit:

# df -h /srv/base/
Filesystem            Size  Used Avail Use% Mounted on
/dev/mapper/vg_critical-lv_base
                     1008M  835M  123M  88% /srv/base
# vgdisplay -C vg_critical
  VG          #PV #LV #SN Attr   VSize VFree
  vg_critical   2   2   0 wz--n- 8.14g 144.00m

No matter, since LVM allows adding physical volumes to existing volume groups. For instance, maybe we've noticed that the sdb1 partition, which was so far used outside of LVM, only contained archives that could be moved to lv_backups. We can now recycle it and integrate it to the volume group, and thereby reclaim some available space. This is the purpose of the vgextend command. Of course, the partition must be prepared as a physical volume beforehand. Once the VG has been extended, we can use similar commands as previously to grow the logical volume then the filesystem:

# pvcreate /dev/sdb1
  Physical volume "/dev/sdb1" successfully created
# vgextend vg_critical /dev/sdb1
  Volume group "vg_critical" successfully extended
# vgdisplay -C vg_critical
  VG          #PV #LV #SN Attr   VSize VFree
  vg_critical   3   2   0 wz--n- 9.09g 1.09g
# [...]
[...]
# df -h /srv/base/
Filesystem            Size  Used Avail Use% Mounted on
/dev/mapper/vg_critical-lv_base
                      2.0G  835M  1.1G  44% /srv/base

GOING FURTHER Advanced LVM

LVM also caters for more advanced uses, where many details can be specified by hand. For instance, an administrator can tweak the size of the blocks that make up physical and logical volumes, as well as their physical layout. It is also possible to move blocks across PVs, for instance to fine-tune performance or, in a more mundane way, to free a PV when one needs to extract the corresponding physical disk from the VG (whether to affect it to another VG or to remove it from LVM altogether). The manual pages describing the commands are generally clear and detailed. A good entry point is the lvm(8) manual page.

12.1.3. RAID or LVM?

RAID and LVM both bring undisputable advantages as soon as one leaves the simple case of a desktop computer with a single hard disk where the usage pattern doesn't change over time. However, RAID and LVM go in two different directions, with diverging goals, and it is legitimate to wonder which one should be adopted. The most appropriate answer will of course depend on current and foreseeable requirements.

There are a few simple cases where the question doesn't really arise. If the requirement is to safeguard data against hardware failures, then obviously RAID will be set up on a redundant array of disks, since LVM doesn't really address this problem. If, on the other hand, the need is for a flexible storage scheme where the volumes are made independent of the physical layout of the disks, RAID doesn't help much and LVM will be the natural choice.

The third notable use case is when one just wants to aggregate two disks into one volume, either for performance reasons or to have a single filesystem that is larger than any of the available disks. This case can be addressed both by a RAID-0 (or even linear-RAID) and by an LVM volume. When in this situation, and barring extra constraints (keeping in line with the rest of the computers if they only use RAID), the configuration of choice will often be LVM. The initial set up is slightly more complex, but that slight increase in complexity more than makes up for the extra flexibility that LVM brings if the requirements change or if new disks need to be added.

Then of course, there is the really interesting use case, where the storage system needs to be made both resistant to hardware failure and flexible when it comes to volume allocation. Neither RAID nor LVM can address both requirements on their own; no matter, this is where we use both at the same time — or rather, one on top of the other. The scheme that has all but become a standard since RAID and LVM have reached maturity is to ensure data redundancy first by grouping disks in a small number of large RAID arrays, and to use these RAID arrays as LVM physical volumes; logical partitions will then be carved from these LVs for filesystems. The selling point of this setup is that when a disk fails, only a small number of RAID arrays will need to be reconstructed, thereby limiting the time spent by the administrator for recovery.

Let's take a concrete example: the public relations department at Falcot Corp needs a workstation for video editing, but the department's budget doesn't allow investing in high-end hardware from the bottom up. A decision is made to favour the hardware that is specific to the graphic nature of the work (monitor and video card), and to stay with generic hardware for storage. However, as is widely known, digital video does have some particular requirements for its storage: the amount of data to store is large, and the throughput rate for reading and writing this data is important for the overall system performance (more than typical access time, for instance). These constraints need to be fulfilled with generic hardware, in this case two 300 GB SATA hard disk drives; the system data must also be made resistant to hardware failure, as well as some of the user data. Edited videoclips must indeed be safe, but video rushes pending editing are less critical, since they're still on the videotapes.

RAID-1 and LVM are combined to satisfy these constraints. The disks are attached to two different SATA controllers to optimize parallel access and reduce the risk of a simultaneous failure, and they therefore appear as sda and sdc. They are partitioned identically along the following scheme:

# fdisk -l /dev/sda

Disk /dev/hda: 300.0 GB, 300090728448 bytes
255 heads, 63 sectors/track, 36483 cylinders
Units = cylinders of 16065 * 512 = 8225280 bytes
Sector size (logical/physical): 512 bytes / 512 bytes
I/O size (minimum/optimal): 512 bytes / 512 bytes
Disk identifier: 0x00039a9f

   Device Boot      Start      End      Blocks   Id  System
/dev/sda1   *           1      124      995998+  fd  Linux raid autodetect
/dev/sda2             125      248      996030   82  Linux swap / Solaris
/dev/sda3             249    36483   291057637+   5  Extended
/dev/sda5             249    12697    99996561   fd  Linux raid autodetect
/dev/sda6           12698    25146    99996561   fd  Linux raid autodetect
/dev/sda7           25147    36483    91064421   8e  Linux LVM

The first partitions of both disks (about 1 GB) are assembled into a RAID-1 volume, md0. This mirror is directly used to store the root filesystem.
The sda2 and sdc2 partitions are used as swap partitions, providing a total 2 GB of swap space. With 1 GB of RAM, the workstation has a comfortable amount of available memory.
The sda5 and sdc5 partitions, as well as sda6 and sdc6, are assembled into two new RAID-1 volumes of about 100 GB each, md1 and md2. Both these mirrors are initialized as physical volumes for LVM, and assigned to the vg_raid volume group. This VG thus contains about 200 GB of safe space.
The remaining partitions, sda7 and sdc7, are directly used as physical volumes, and assigned to another VG called vg_bulk, which therefore ends up with roughly 200 GB of space.

Once the VGs are created, they can be partitioned in a very flexible way. One must keep in mind that LVs created in vg_raid will be preserved even if one of the disks fails, which will not be the case for LVs created in vg_bulk; on the other hand, the latter will be allocated in parallel on both disks, which allows higher read or write speeds for large files.

We'll therefore create the lv_usr, lv_var and lv_home LVs on vg_raid, to host the matching filesystems; another large LV, lv_movies, will be used to host the definitive versions of movies after editing. The other VG will be split into a large lv_rushes, for data straight out of the digital video cameras, and a lv_tmp for temporary files. The location of the work area is a less straightforward choice to make: while good performance is needed for that volume, is it worth risking losing work if a disk fails during an editing session? Depending on the answer to that question, the relevant LV will be created on one VG or the other.

We now have both some redundancy for important data and much flexibility in how the available space is split across the applications. Should new software be installed later on (for editing audio clips, for instance), the LV hosting /usr/ can be grown painlessly.

NOTE Why three RAID-1 volumes?

We could have set up one RAID-1 volume only, to serve as a physical volume for vg_raid. Why create three of them, then?

The rationale for the first split (md0 vs. the others) is about data safety: data written to both elements of a RAID-1 mirror are exactly the same, and it is therefore possible to bypass the RAID layer and mount one of the disks directly. In case of a kernel bug, for instance, or if the LVM metadata become corrupted, it is still possible to boot a minimal system to access critical data such as the layout of disks in the RAID and LVM volumes; the metadata can then be reconstructed and the files can be accessed again, so that the system can be brought back to its nominal state.

The rationale for the second split (md1 vs. md2) is less clear-cut, and more related to acknowledging that the future is uncertain. When the workstation is first assembled, the exact storage requirements are not necessarily known with perfect precision; they can also evolve over time. In our case, we can't know in advance the actual storage space requirements for video rushes and complete video clips. If one particular clip needs a very large amount of rushes, and the VG dedicated to redundant data is less than halfway full, we can re-use some of its unneeded space. We can remove one of the physical volumes, say md2 from vg_raid and either assign it to vg_bulk directly (if the expected duration of the operation is short enough that we can live with the temporary drop in performance), or undo the RAID setup on md2 and integrate its components sda6 and sdc6 into the bulk VG (which grows by 200 GB instead of 100 GB); the lv_rushes logical volume can then be grown according to requirements.