Statistics
| Branch: | Tag: | Revision:

root / man / hbal.rst @ 2c04ae0d

History | View | Annotate | Download (26.5 kB)

1 5a19bd35 Iustin Pop
HBAL(1) Ganeti | Version @GANETI_VERSION@
2 5a19bd35 Iustin Pop
=========================================
3 49148d15 Iustin Pop
4 49148d15 Iustin Pop
NAME
5 49148d15 Iustin Pop
----
6 49148d15 Iustin Pop
7 49148d15 Iustin Pop
hbal \- Cluster balancer for Ganeti
8 49148d15 Iustin Pop
9 49148d15 Iustin Pop
SYNOPSIS
10 49148d15 Iustin Pop
--------
11 49148d15 Iustin Pop
12 49148d15 Iustin Pop
**hbal** {backend options...} [algorithm options...] [reporting options...]
13 49148d15 Iustin Pop
14 f624fa95 Iustin Pop
**hbal** \--version
15 49148d15 Iustin Pop
16 49148d15 Iustin Pop
17 49148d15 Iustin Pop
Backend options:
18 49148d15 Iustin Pop
19 0547d608 René Nussbaumer
{ **-m** *cluster* | **-L[** *path* **] [-X]** | **-t** *data-file* |
20 0547d608 René Nussbaumer
**-I** *path* }
21 49148d15 Iustin Pop
22 49148d15 Iustin Pop
Algorithm options:
23 49148d15 Iustin Pop
24 f624fa95 Iustin Pop
**[ \--max-cpu *cpu-ratio* ]**
25 f624fa95 Iustin Pop
**[ \--min-disk *disk-ratio* ]**
26 49148d15 Iustin Pop
**[ -l *limit* ]**
27 49148d15 Iustin Pop
**[ -e *score* ]**
28 f624fa95 Iustin Pop
**[ -g *delta* ]** **[ \--min-gain-limit *threshold* ]**
29 49148d15 Iustin Pop
**[ -O *name...* ]**
30 f624fa95 Iustin Pop
**[ \--no-disk-moves ]**
31 f624fa95 Iustin Pop
**[ \--no-instance-moves ]**
32 49148d15 Iustin Pop
**[ -U *util-file* ]**
33 f624fa95 Iustin Pop
**[ \--evac-mode ]**
34 f624fa95 Iustin Pop
**[ \--select-instances *inst...* ]**
35 f624fa95 Iustin Pop
**[ \--exclude-instances *inst...* ]**
36 49148d15 Iustin Pop
37 49148d15 Iustin Pop
Reporting options:
38 49148d15 Iustin Pop
39 49148d15 Iustin Pop
**[ -C[ *file* ] ]**
40 49148d15 Iustin Pop
**[ -p[ *fields* ] ]**
41 f624fa95 Iustin Pop
**[ \--print-instances ]**
42 5a736782 Guido Trotter
**[ -S *file* ]**
43 49148d15 Iustin Pop
**[ -v... | -q ]**
44 49148d15 Iustin Pop
45 49148d15 Iustin Pop
46 49148d15 Iustin Pop
DESCRIPTION
47 49148d15 Iustin Pop
-----------
48 49148d15 Iustin Pop
49 49148d15 Iustin Pop
hbal is a cluster balancer that looks at the current state of the
50 49148d15 Iustin Pop
cluster (nodes with their total and free disk, memory, etc.) and
51 49148d15 Iustin Pop
instance placement and computes a series of steps designed to bring
52 49148d15 Iustin Pop
the cluster into a better state.
53 49148d15 Iustin Pop
54 49148d15 Iustin Pop
The algorithm used is designed to be stable (i.e. it will give you the
55 49148d15 Iustin Pop
same results when restarting it from the middle of the solution) and
56 f624fa95 Iustin Pop
reasonably fast. It is not, however, designed to be a perfect algorithm:
57 f624fa95 Iustin Pop
it is possible to make it go into a corner from which it can find no
58 f624fa95 Iustin Pop
improvement, because it looks only one "step" ahead.
59 49148d15 Iustin Pop
60 49148d15 Iustin Pop
By default, the program will show the solution incrementally as it is
61 49148d15 Iustin Pop
computed, in a somewhat cryptic format; for getting the actual Ganeti
62 49148d15 Iustin Pop
command list, use the **-C** option.
63 49148d15 Iustin Pop
64 49148d15 Iustin Pop
ALGORITHM
65 49148d15 Iustin Pop
~~~~~~~~~
66 49148d15 Iustin Pop
67 49148d15 Iustin Pop
The program works in independent steps; at each step, we compute the
68 49148d15 Iustin Pop
best instance move that lowers the cluster score.
69 49148d15 Iustin Pop
70 49148d15 Iustin Pop
The possible move type for an instance are combinations of
71 49148d15 Iustin Pop
failover/migrate and replace-disks such that we change one of the
72 49148d15 Iustin Pop
instance nodes, and the other one remains (but possibly with changed
73 49148d15 Iustin Pop
role, e.g. from primary it becomes secondary). The list is:
74 49148d15 Iustin Pop
75 49148d15 Iustin Pop
- failover (f)
76 49148d15 Iustin Pop
- replace secondary (r)
77 49148d15 Iustin Pop
- replace primary, a composite move (f, r, f)
78 49148d15 Iustin Pop
- failover and replace secondary, also composite (f, r)
79 49148d15 Iustin Pop
- replace secondary and failover, also composite (r, f)
80 49148d15 Iustin Pop
81 49148d15 Iustin Pop
We don't do the only remaining possibility of replacing both nodes
82 49148d15 Iustin Pop
(r,f,r,f or the equivalent f,r,f,r) since these move needs an
83 49148d15 Iustin Pop
exhaustive search over both candidate primary and secondary nodes, and
84 49148d15 Iustin Pop
is O(n*n) in the number of nodes. Furthermore, it doesn't seems to
85 49148d15 Iustin Pop
give better scores but will result in more disk replacements.
86 49148d15 Iustin Pop
87 49148d15 Iustin Pop
PLACEMENT RESTRICTIONS
88 49148d15 Iustin Pop
~~~~~~~~~~~~~~~~~~~~~~
89 49148d15 Iustin Pop
90 49148d15 Iustin Pop
At each step, we prevent an instance move if it would cause:
91 49148d15 Iustin Pop
92 49148d15 Iustin Pop
- a node to go into N+1 failure state
93 49148d15 Iustin Pop
- an instance to move onto an offline node (offline nodes are either
94 325947e7 Klaus Aehlig
  read from the cluster or declared with *-O*; drained nodes are
95 325947e7 Klaus Aehlig
  considered offline)
96 49148d15 Iustin Pop
- an exclusion-tag based conflict (exclusion tags are read from the
97 f624fa95 Iustin Pop
  cluster and/or defined via the *\--exclusion-tags* option)
98 f624fa95 Iustin Pop
- a max vcpu/pcpu ratio to be exceeded (configured via *\--max-cpu*)
99 49148d15 Iustin Pop
- min disk free percentage to go below the configured limit
100 f624fa95 Iustin Pop
  (configured via *\--min-disk*)
101 49148d15 Iustin Pop
102 49148d15 Iustin Pop
CLUSTER SCORING
103 49148d15 Iustin Pop
~~~~~~~~~~~~~~~
104 49148d15 Iustin Pop
105 49148d15 Iustin Pop
As said before, the algorithm tries to minimise the cluster score at
106 325947e7 Klaus Aehlig
each step. Currently this score is computed as a weighted sum of the
107 325947e7 Klaus Aehlig
following components:
108 49148d15 Iustin Pop
109 49148d15 Iustin Pop
- standard deviation of the percent of free memory
110 49148d15 Iustin Pop
- standard deviation of the percent of reserved memory
111 49148d15 Iustin Pop
- standard deviation of the percent of free disk
112 49148d15 Iustin Pop
- count of nodes failing N+1 check
113 49148d15 Iustin Pop
- count of instances living (either as primary or secondary) on
114 325947e7 Klaus Aehlig
  offline nodes; in the sense of hbal (and the other htools) drained
115 325947e7 Klaus Aehlig
  nodes are considered offline
116 49148d15 Iustin Pop
- count of instances living (as primary) on offline nodes; this
117 49148d15 Iustin Pop
  differs from the above metric by helping failover of such instances
118 49148d15 Iustin Pop
  in 2-node clusters
119 49148d15 Iustin Pop
- standard deviation of the ratio of virtual-to-physical cpus (for
120 49148d15 Iustin Pop
  primary instances of the node)
121 49148d15 Iustin Pop
- standard deviation of the dynamic load on the nodes, for cpus,
122 49148d15 Iustin Pop
  memory, disk and network
123 49148d15 Iustin Pop
124 49148d15 Iustin Pop
The free memory and free disk values help ensure that all nodes are
125 49148d15 Iustin Pop
somewhat balanced in their resource usage. The reserved memory helps
126 49148d15 Iustin Pop
to ensure that nodes are somewhat balanced in holding secondary
127 49148d15 Iustin Pop
instances, and that no node keeps too much memory reserved for
128 49148d15 Iustin Pop
N+1. And finally, the N+1 percentage helps guide the algorithm towards
129 49148d15 Iustin Pop
eliminating N+1 failures, if possible.
130 49148d15 Iustin Pop
131 49148d15 Iustin Pop
Except for the N+1 failures and offline instances counts, we use the
132 49148d15 Iustin Pop
standard deviation since when used with values within a fixed range
133 49148d15 Iustin Pop
(we use percents expressed as values between zero and one) it gives
134 49148d15 Iustin Pop
consistent results across all metrics (there are some small issues
135 49148d15 Iustin Pop
related to different means, but it works generally well). The 'count'
136 49148d15 Iustin Pop
type values will have higher score and thus will matter more for
137 49148d15 Iustin Pop
balancing; thus these are better for hard constraints (like evacuating
138 49148d15 Iustin Pop
nodes and fixing N+1 failures). For example, the offline instances
139 49148d15 Iustin Pop
count (i.e. the number of instances living on offline nodes) will
140 49148d15 Iustin Pop
cause the algorithm to actively move instances away from offline
141 49148d15 Iustin Pop
nodes. This, coupled with the restriction on placement given by
142 49148d15 Iustin Pop
offline nodes, will cause evacuation of such nodes.
143 49148d15 Iustin Pop
144 49148d15 Iustin Pop
The dynamic load values need to be read from an external file (Ganeti
145 49148d15 Iustin Pop
doesn't supply them), and are computed for each node as: sum of
146 49148d15 Iustin Pop
primary instance cpu load, sum of primary instance memory load, sum of
147 49148d15 Iustin Pop
primary and secondary instance disk load (as DRBD generates write load
148 49148d15 Iustin Pop
on secondary nodes too in normal case and in degraded scenarios also
149 49148d15 Iustin Pop
read load), and sum of primary instance network load. An example of
150 49148d15 Iustin Pop
how to generate these values for input to hbal would be to track ``xm
151 49148d15 Iustin Pop
list`` for instances over a day and by computing the delta of the cpu
152 49148d15 Iustin Pop
values, and feed that via the *-U* option for all instances (and keep
153 49148d15 Iustin Pop
the other metrics as one). For the algorithm to work, all that is
154 49148d15 Iustin Pop
needed is that the values are consistent for a metric across all
155 49148d15 Iustin Pop
instances (e.g. all instances use cpu% to report cpu usage, and not
156 49148d15 Iustin Pop
something related to number of CPU seconds used if the CPUs are
157 49148d15 Iustin Pop
different), and that they are normalised to between zero and one. Note
158 49148d15 Iustin Pop
that it's recommended to not have zero as the load value for any
159 49148d15 Iustin Pop
instance metric since then secondary instances are not well balanced.
160 49148d15 Iustin Pop
161 49148d15 Iustin Pop
On a perfectly balanced cluster (all nodes the same size, all
162 49148d15 Iustin Pop
instances the same size and spread across the nodes equally), the
163 49148d15 Iustin Pop
values for all metrics would be zero. This doesn't happen too often in
164 49148d15 Iustin Pop
practice :)
165 49148d15 Iustin Pop
166 49148d15 Iustin Pop
OFFLINE INSTANCES
167 49148d15 Iustin Pop
~~~~~~~~~~~~~~~~~
168 49148d15 Iustin Pop
169 49148d15 Iustin Pop
Since current Ganeti versions do not report the memory used by offline
170 49148d15 Iustin Pop
(down) instances, ignoring the run status of instances will cause
171 49148d15 Iustin Pop
wrong calculations. For this reason, the algorithm subtracts the
172 49148d15 Iustin Pop
memory size of down instances from the free node memory of their
173 49148d15 Iustin Pop
primary node, in effect simulating the startup of such instances.
174 49148d15 Iustin Pop
175 49148d15 Iustin Pop
EXCLUSION TAGS
176 49148d15 Iustin Pop
~~~~~~~~~~~~~~
177 49148d15 Iustin Pop
178 49148d15 Iustin Pop
The exclusion tags mechanism is designed to prevent instances which
179 49148d15 Iustin Pop
run the same workload (e.g. two DNS servers) to land on the same node,
180 49148d15 Iustin Pop
which would make the respective node a SPOF for the given service.
181 49148d15 Iustin Pop
182 49148d15 Iustin Pop
It works by tagging instances with certain tags and then building
183 49148d15 Iustin Pop
exclusion maps based on these. Which tags are actually used is
184 f624fa95 Iustin Pop
configured either via the command line (option *\--exclusion-tags*)
185 49148d15 Iustin Pop
or via adding them to the cluster tags:
186 49148d15 Iustin Pop
187 f624fa95 Iustin Pop
\--exclusion-tags=a,b
188 49148d15 Iustin Pop
  This will make all instance tags of the form *a:\**, *b:\** be
189 49148d15 Iustin Pop
  considered for the exclusion map
190 49148d15 Iustin Pop
191 49148d15 Iustin Pop
cluster tags *htools:iextags:a*, *htools:iextags:b*
192 49148d15 Iustin Pop
  This will make instance tags *a:\**, *b:\** be considered for the
193 49148d15 Iustin Pop
  exclusion map. More precisely, the suffix of cluster tags starting
194 49148d15 Iustin Pop
  with *htools:iextags:* will become the prefix of the exclusion tags.
195 49148d15 Iustin Pop
196 49148d15 Iustin Pop
Both the above forms mean that two instances both having (e.g.) the
197 49148d15 Iustin Pop
tag *a:foo* or *b:bar* won't end on the same node.
198 49148d15 Iustin Pop
199 49148d15 Iustin Pop
OPTIONS
200 49148d15 Iustin Pop
-------
201 49148d15 Iustin Pop
202 49148d15 Iustin Pop
The options that can be passed to the program are as follows:
203 49148d15 Iustin Pop
204 f624fa95 Iustin Pop
-C, \--print-commands
205 49148d15 Iustin Pop
  Print the command list at the end of the run. Without this, the
206 49148d15 Iustin Pop
  program will only show a shorter, but cryptic output.
207 49148d15 Iustin Pop
208 49148d15 Iustin Pop
  Note that the moves list will be split into independent steps,
209 49148d15 Iustin Pop
  called "jobsets", but only for visual inspection, not for actually
210 49148d15 Iustin Pop
  parallelisation. It is not possible to parallelise these directly
211 49148d15 Iustin Pop
  when executed via "gnt-instance" commands, since a compound command
212 49148d15 Iustin Pop
  (e.g. failover and replace-disks) must be executed
213 49148d15 Iustin Pop
  serially. Parallel execution is only possible when using the Luxi
214 49148d15 Iustin Pop
  backend and the *-L* option.
215 49148d15 Iustin Pop
216 49148d15 Iustin Pop
  The algorithm for splitting the moves into jobsets is by
217 49148d15 Iustin Pop
  accumulating moves until the next move is touching nodes already
218 49148d15 Iustin Pop
  touched by the current moves; this means we can't execute in
219 49148d15 Iustin Pop
  parallel (due to resource allocation in Ganeti) and thus we start a
220 49148d15 Iustin Pop
  new jobset.
221 49148d15 Iustin Pop
222 f624fa95 Iustin Pop
-p, \--print-nodes
223 d7731f51 Iustin Pop
  Prints the before and after node status, in a format designed to allow
224 d7731f51 Iustin Pop
  the user to understand the node's most important parameters. See the
225 354c4f62 Michael Hanselmann
  man page **htools**\(1) for more details about this option.
226 49148d15 Iustin Pop
227 f624fa95 Iustin Pop
\--print-instances
228 49148d15 Iustin Pop
  Prints the before and after instance map. This is less useful as the
229 49148d15 Iustin Pop
  node status, but it can help in understanding instance moves.
230 49148d15 Iustin Pop
231 49148d15 Iustin Pop
-O *name*
232 49148d15 Iustin Pop
  This option (which can be given multiple times) will mark nodes as
233 49148d15 Iustin Pop
  being *offline*. This means a couple of things:
234 49148d15 Iustin Pop
235 49148d15 Iustin Pop
  - instances won't be placed on these nodes, not even temporarily;
236 49148d15 Iustin Pop
    e.g. the *replace primary* move is not available if the secondary
237 49148d15 Iustin Pop
    node is offline, since this move requires a failover.
238 49148d15 Iustin Pop
  - these nodes will not be included in the score calculation (except
239 49148d15 Iustin Pop
    for the percentage of instances on offline nodes)
240 49148d15 Iustin Pop
241 49148d15 Iustin Pop
  Note that algorithm will also mark as offline any nodes which are
242 49148d15 Iustin Pop
  reported by RAPI as such, or that have "?" in file-based input in
243 49148d15 Iustin Pop
  any numeric fields.
244 49148d15 Iustin Pop
245 f624fa95 Iustin Pop
-e *score*, \--min-score=*score*
246 49148d15 Iustin Pop
  This parameter denotes the minimum score we are happy with and alters
247 49148d15 Iustin Pop
  the computation in two ways:
248 49148d15 Iustin Pop
249 49148d15 Iustin Pop
  - if the cluster has the initial score lower than this value, then we
250 49148d15 Iustin Pop
    don't enter the algorithm at all, and exit with success
251 49148d15 Iustin Pop
  - during the iterative process, if we reach a score lower than this
252 49148d15 Iustin Pop
    value, we exit the algorithm
253 49148d15 Iustin Pop
254 49148d15 Iustin Pop
  The default value of the parameter is currently ``1e-9`` (chosen
255 49148d15 Iustin Pop
  empirically).
256 49148d15 Iustin Pop
257 f624fa95 Iustin Pop
-g *delta*, \--min-gain=*delta*
258 49148d15 Iustin Pop
  Since the balancing algorithm can sometimes result in just very tiny
259 49148d15 Iustin Pop
  improvements, that bring less gain that they cost in relocation
260 49148d15 Iustin Pop
  time, this parameter (defaulting to 0.01) represents the minimum
261 49148d15 Iustin Pop
  gain we require during a step, to continue balancing.
262 49148d15 Iustin Pop
263 f624fa95 Iustin Pop
\--min-gain-limit=*threshold*
264 49148d15 Iustin Pop
  The above min-gain option will only take effect if the cluster score
265 49148d15 Iustin Pop
  is already below *threshold* (defaults to 0.1). The rationale behind
266 49148d15 Iustin Pop
  this setting is that at high cluster scores (badly balanced
267 49148d15 Iustin Pop
  clusters), we don't want to abort the rebalance too quickly, as
268 49148d15 Iustin Pop
  later gains might still be significant. However, under the
269 49148d15 Iustin Pop
  threshold, the total gain is only the threshold value, so we can
270 49148d15 Iustin Pop
  exit early.
271 49148d15 Iustin Pop
272 f624fa95 Iustin Pop
\--no-disk-moves
273 49148d15 Iustin Pop
  This parameter prevents hbal from using disk move
274 49148d15 Iustin Pop
  (i.e. "gnt-instance replace-disks") operations. This will result in
275 49148d15 Iustin Pop
  a much quicker balancing, but of course the improvements are
276 49148d15 Iustin Pop
  limited. It is up to the user to decide when to use one or another.
277 49148d15 Iustin Pop
278 f624fa95 Iustin Pop
\--no-instance-moves
279 0aa71dbd Guido Trotter
  This parameter prevents hbal from using instance moves
280 0aa71dbd Guido Trotter
  (i.e. "gnt-instance migrate/failover") operations. This will only use
281 0aa71dbd Guido Trotter
  the slow disk-replacement operations, and will also provide a worse
282 0aa71dbd Guido Trotter
  balance, but can be useful if moving instances around is deemed unsafe
283 0aa71dbd Guido Trotter
  or not preferred.
284 0aa71dbd Guido Trotter
285 f624fa95 Iustin Pop
\--evac-mode
286 49148d15 Iustin Pop
  This parameter restricts the list of instances considered for moving
287 49148d15 Iustin Pop
  to the ones living on offline/drained nodes. It can be used as a
288 49148d15 Iustin Pop
  (bulk) replacement for Ganeti's own *gnt-node evacuate*, with the
289 49148d15 Iustin Pop
  note that it doesn't guarantee full evacuation.
290 49148d15 Iustin Pop
291 f624fa95 Iustin Pop
\--select-instances=*instances*
292 bcd87e22 Guido Trotter
  This parameter marks the given instances (as a comma-separated list)
293 bcd87e22 Guido Trotter
  as the only ones being moved during the rebalance.
294 bcd87e22 Guido Trotter
295 f624fa95 Iustin Pop
\--exclude-instances=*instances*
296 49148d15 Iustin Pop
  This parameter marks the given instances (as a comma-separated list)
297 49148d15 Iustin Pop
  from being moved during the rebalance.
298 49148d15 Iustin Pop
299 49148d15 Iustin Pop
-U *util-file*
300 49148d15 Iustin Pop
  This parameter specifies a file holding instance dynamic utilisation
301 49148d15 Iustin Pop
  information that will be used to tweak the balancing algorithm to
302 49148d15 Iustin Pop
  equalise load on the nodes (as opposed to static resource
303 49148d15 Iustin Pop
  usage). The file is in the format "instance_name cpu_util mem_util
304 49148d15 Iustin Pop
  disk_util net_util" where the "_util" parameters are interpreted as
305 49148d15 Iustin Pop
  numbers and the instance name must match exactly the instance as
306 49148d15 Iustin Pop
  read from Ganeti. In case of unknown instance names, the program
307 49148d15 Iustin Pop
  will abort.
308 49148d15 Iustin Pop
309 49148d15 Iustin Pop
  If not given, the default values are one for all metrics and thus
310 49148d15 Iustin Pop
  dynamic utilisation has only one effect on the algorithm: the
311 49148d15 Iustin Pop
  equalisation of the secondary instances across nodes (this is the
312 49148d15 Iustin Pop
  only metric that is not tracked by another, dedicated value, and
313 49148d15 Iustin Pop
  thus the disk load of instances will cause secondary instance
314 49148d15 Iustin Pop
  equalisation). Note that value of one will also influence slightly
315 49148d15 Iustin Pop
  the primary instance count, but that is already tracked via other
316 49148d15 Iustin Pop
  metrics and thus the influence of the dynamic utilisation will be
317 49148d15 Iustin Pop
  practically insignificant.
318 49148d15 Iustin Pop
319 f624fa95 Iustin Pop
-S *filename*, \--save-cluster=*filename*
320 4188449c Iustin Pop
  If given, the state of the cluster before the balancing is saved to
321 4188449c Iustin Pop
  the given file plus the extension "original"
322 4188449c Iustin Pop
  (i.e. *filename*.original), and the state at the end of the
323 4188449c Iustin Pop
  balancing is saved to the given file plus the extension "balanced"
324 4188449c Iustin Pop
  (i.e. *filename*.balanced). This allows re-feeding the cluster state
325 acd9fa11 Iustin Pop
  to either hbal itself or for example hspace via the ``-t`` option.
326 acd9fa11 Iustin Pop
327 f624fa95 Iustin Pop
-t *datafile*, \--text-data=*datafile*
328 acd9fa11 Iustin Pop
  Backend specification: the name of the file holding node and instance
329 acd9fa11 Iustin Pop
  information (if not collecting via RAPI or LUXI). This or one of the
330 acd9fa11 Iustin Pop
  other backends must be selected. The option is described in the man
331 354c4f62 Michael Hanselmann
  page **htools**\(1).
332 49148d15 Iustin Pop
333 49148d15 Iustin Pop
-m *cluster*
334 acd9fa11 Iustin Pop
  Backend specification: collect data directly from the *cluster* given
335 acd9fa11 Iustin Pop
  as an argument via RAPI. The option is described in the man page
336 354c4f62 Michael Hanselmann
  **htools**\(1).
337 49148d15 Iustin Pop
338 49148d15 Iustin Pop
-L [*path*]
339 acd9fa11 Iustin Pop
  Backend specification: collect data directly from the master daemon,
340 acd9fa11 Iustin Pop
  which is to be contacted via LUXI (an internal Ganeti protocol). The
341 354c4f62 Michael Hanselmann
  option is described in the man page **htools**\(1).
342 49148d15 Iustin Pop
343 49148d15 Iustin Pop
-X
344 49148d15 Iustin Pop
  When using the Luxi backend, hbal can also execute the given
345 49148d15 Iustin Pop
  commands. The execution method is to execute the individual jobsets
346 49148d15 Iustin Pop
  (see the *-C* option for details) in separate stages, aborting if at
347 49148d15 Iustin Pop
  any time a jobset doesn't have all jobs successful. Each step in the
348 49148d15 Iustin Pop
  balancing solution will be translated into exactly one Ganeti job
349 49148d15 Iustin Pop
  (having between one and three OpCodes), and all the steps in a
350 49148d15 Iustin Pop
  jobset will be executed in parallel. The jobsets themselves are
351 49148d15 Iustin Pop
  executed serially.
352 49148d15 Iustin Pop
353 2b634302 Iustin Pop
  The execution of the job series can be interrupted, see below for
354 2b634302 Iustin Pop
  signal handling.
355 2b634302 Iustin Pop
356 f624fa95 Iustin Pop
-l *N*, \--max-length=*N*
357 49148d15 Iustin Pop
  Restrict the solution to this length. This can be used for example
358 49148d15 Iustin Pop
  to automate the execution of the balancing.
359 49148d15 Iustin Pop
360 f624fa95 Iustin Pop
\--max-cpu=*cpu-ratio*
361 f815aa89 Iustin Pop
  The maximum virtual to physical cpu ratio, as a floating point number
362 f815aa89 Iustin Pop
  greater than or equal to one. For example, specifying *cpu-ratio* as
363 f815aa89 Iustin Pop
  **2.5** means that, for a 4-cpu machine, a maximum of 10 virtual cpus
364 f815aa89 Iustin Pop
  should be allowed to be in use for primary instances. A value of
365 f815aa89 Iustin Pop
  exactly one means there will be no over-subscription of CPU (except
366 f815aa89 Iustin Pop
  for the CPU time used by the node itself), and values below one do not
367 f815aa89 Iustin Pop
  make sense, as that means other resources (e.g. disk) won't be fully
368 f815aa89 Iustin Pop
  utilised due to CPU restrictions.
369 49148d15 Iustin Pop
370 f624fa95 Iustin Pop
\--min-disk=*disk-ratio*
371 49148d15 Iustin Pop
  The minimum amount of free disk space remaining, as a floating point
372 49148d15 Iustin Pop
  number. For example, specifying *disk-ratio* as **0.25** means that
373 49148d15 Iustin Pop
  at least one quarter of disk space should be left free on nodes.
374 49148d15 Iustin Pop
375 f624fa95 Iustin Pop
-G *uuid*, \--group=*uuid*
376 646aa028 Iustin Pop
  On an multi-group cluster, select this group for
377 646aa028 Iustin Pop
  processing. Otherwise hbal will abort, since it cannot balance
378 646aa028 Iustin Pop
  multiple groups at the same time.
379 646aa028 Iustin Pop
380 f624fa95 Iustin Pop
-v, \--verbose
381 49148d15 Iustin Pop
  Increase the output verbosity. Each usage of this option will
382 49148d15 Iustin Pop
  increase the verbosity (currently more than 2 doesn't make sense)
383 49148d15 Iustin Pop
  from the default of one.
384 49148d15 Iustin Pop
385 f624fa95 Iustin Pop
-q, \--quiet
386 49148d15 Iustin Pop
  Decrease the output verbosity. Each usage of this option will
387 49148d15 Iustin Pop
  decrease the verbosity (less than zero doesn't make sense) from the
388 49148d15 Iustin Pop
  default of one.
389 49148d15 Iustin Pop
390 f624fa95 Iustin Pop
-V, \--version
391 49148d15 Iustin Pop
  Just show the program version and exit.
392 49148d15 Iustin Pop
393 2b634302 Iustin Pop
SIGNAL HANDLING
394 2b634302 Iustin Pop
---------------
395 2b634302 Iustin Pop
396 2b634302 Iustin Pop
When executing jobs via LUXI (using the ``-X`` option), normally hbal
397 2b634302 Iustin Pop
will execute all jobs until either one errors out or all the jobs finish
398 2b634302 Iustin Pop
successfully.
399 2b634302 Iustin Pop
400 2b634302 Iustin Pop
Since balancing can take a long time, it is possible to stop hbal early
401 2b634302 Iustin Pop
in two ways:
402 2b634302 Iustin Pop
403 2b634302 Iustin Pop
- by sending a ``SIGINT`` (``^C``), hbal will register the termination
404 2b634302 Iustin Pop
  request, and will wait until the currently submitted jobs finish, at
405 2d6bdcc5 Iustin Pop
  which point it will exit (with exit code 0 if all jobs finished
406 2d6bdcc5 Iustin Pop
  correctly, otherwise with exit code 1 as usual)
407 2d6bdcc5 Iustin Pop
408 2b634302 Iustin Pop
- by sending a ``SIGTERM``, hbal will immediately exit (with exit code
409 2d6bdcc5 Iustin Pop
  2\); it is the responsibility of the user to follow up with Ganeti
410 2d6bdcc5 Iustin Pop
  and check the result of the currently-executing jobs
411 2b634302 Iustin Pop
412 2b634302 Iustin Pop
Note that in any situation, it's perfectly safe to kill hbal, either via
413 2b634302 Iustin Pop
the above signals or via any other signal (e.g. ``SIGQUIT``,
414 2b634302 Iustin Pop
``SIGKILL``), since the jobs themselves are processed by Ganeti whereas
415 2b634302 Iustin Pop
hbal (after submission) only watches their progression. In this case,
416 2d6bdcc5 Iustin Pop
the user will have to query Ganeti for job results.
417 2b634302 Iustin Pop
418 49148d15 Iustin Pop
EXIT STATUS
419 49148d15 Iustin Pop
-----------
420 49148d15 Iustin Pop
421 2b634302 Iustin Pop
The exit status of the command will be zero, unless for some reason the
422 2a2e2610 Iustin Pop
algorithm failed (e.g. wrong node or instance data), invalid command
423 2a2e2610 Iustin Pop
line options, or (in case of job execution) one of the jobs has failed.
424 2a2e2610 Iustin Pop
425 2a2e2610 Iustin Pop
Once job execution via Luxi has started (``-X``), if the balancing was
426 2a2e2610 Iustin Pop
interrupted early (via *SIGINT*, or via ``--max-length``) but all jobs
427 2a2e2610 Iustin Pop
executed successfully, then the exit status is zero; a non-zero exit
428 2a2e2610 Iustin Pop
code means that the cluster state should be investigated, since a job
429 2a2e2610 Iustin Pop
failed or we couldn't compute its status and this can also point to a
430 2a2e2610 Iustin Pop
problem on the Ganeti side.
431 49148d15 Iustin Pop
432 49148d15 Iustin Pop
BUGS
433 49148d15 Iustin Pop
----
434 49148d15 Iustin Pop
435 2b634302 Iustin Pop
The program does not check all its input data for consistency, and
436 2b634302 Iustin Pop
sometime aborts with cryptic errors messages with invalid data.
437 49148d15 Iustin Pop
438 49148d15 Iustin Pop
The algorithm is not perfect.
439 49148d15 Iustin Pop
440 49148d15 Iustin Pop
EXAMPLE
441 49148d15 Iustin Pop
-------
442 49148d15 Iustin Pop
443 49148d15 Iustin Pop
Note that these examples are not for the latest version (they don't
444 49148d15 Iustin Pop
have full node data).
445 49148d15 Iustin Pop
446 49148d15 Iustin Pop
Default output
447 49148d15 Iustin Pop
~~~~~~~~~~~~~~
448 49148d15 Iustin Pop
449 49148d15 Iustin Pop
With the default options, the program shows each individual step and
450 49148d15 Iustin Pop
the improvements it brings in cluster score::
451 49148d15 Iustin Pop
452 49148d15 Iustin Pop
    $ hbal
453 49148d15 Iustin Pop
    Loaded 20 nodes, 80 instances
454 49148d15 Iustin Pop
    Cluster is not N+1 happy, continuing but no guarantee that the cluster will end N+1 happy.
455 49148d15 Iustin Pop
    Initial score: 0.52329131
456 49148d15 Iustin Pop
    Trying to minimize the CV...
457 49148d15 Iustin Pop
        1. instance14  node1:node10  => node16:node10 0.42109120 a=f r:node16 f
458 49148d15 Iustin Pop
        2. instance54  node4:node15  => node16:node15 0.31904594 a=f r:node16 f
459 49148d15 Iustin Pop
        3. instance4   node5:node2   => node2:node16  0.26611015 a=f r:node16
460 49148d15 Iustin Pop
        4. instance48  node18:node20 => node2:node18  0.21361717 a=r:node2 f
461 49148d15 Iustin Pop
        5. instance93  node19:node18 => node16:node19 0.16166425 a=r:node16 f
462 49148d15 Iustin Pop
        6. instance89  node3:node20  => node2:node3   0.11005629 a=r:node2 f
463 49148d15 Iustin Pop
        7. instance5   node6:node2   => node16:node6  0.05841589 a=r:node16 f
464 49148d15 Iustin Pop
        8. instance94  node7:node20  => node20:node16 0.00658759 a=f r:node16
465 49148d15 Iustin Pop
        9. instance44  node20:node2  => node2:node15  0.00438740 a=f r:node15
466 49148d15 Iustin Pop
       10. instance62  node14:node18 => node14:node16 0.00390087 a=r:node16
467 49148d15 Iustin Pop
       11. instance13  node11:node14 => node11:node16 0.00361787 a=r:node16
468 49148d15 Iustin Pop
       12. instance19  node10:node11 => node10:node7  0.00336636 a=r:node7
469 49148d15 Iustin Pop
       13. instance43  node12:node13 => node12:node1  0.00305681 a=r:node1
470 49148d15 Iustin Pop
       14. instance1   node1:node2   => node1:node4   0.00263124 a=r:node4
471 49148d15 Iustin Pop
       15. instance58  node19:node20 => node19:node17 0.00252594 a=r:node17
472 49148d15 Iustin Pop
    Cluster score improved from 0.52329131 to 0.00252594
473 49148d15 Iustin Pop
474 49148d15 Iustin Pop
In the above output, we can see:
475 49148d15 Iustin Pop
476 49148d15 Iustin Pop
- the input data (here from files) shows a cluster with 20 nodes and
477 49148d15 Iustin Pop
  80 instances
478 49148d15 Iustin Pop
- the cluster is not initially N+1 compliant
479 49148d15 Iustin Pop
- the initial score is 0.52329131
480 49148d15 Iustin Pop
481 49148d15 Iustin Pop
The step list follows, showing the instance, its initial
482 49148d15 Iustin Pop
primary/secondary nodes, the new primary secondary, the cluster list,
483 49148d15 Iustin Pop
and the actions taken in this step (with 'f' denoting failover/migrate
484 49148d15 Iustin Pop
and 'r' denoting replace secondary).
485 49148d15 Iustin Pop
486 49148d15 Iustin Pop
Finally, the program shows the improvement in cluster score.
487 49148d15 Iustin Pop
488 49148d15 Iustin Pop
A more detailed output is obtained via the *-C* and *-p* options::
489 49148d15 Iustin Pop
490 49148d15 Iustin Pop
    $ hbal
491 49148d15 Iustin Pop
    Loaded 20 nodes, 80 instances
492 49148d15 Iustin Pop
    Cluster is not N+1 happy, continuing but no guarantee that the cluster will end N+1 happy.
493 49148d15 Iustin Pop
    Initial cluster status:
494 49148d15 Iustin Pop
    N1 Name   t_mem f_mem r_mem t_dsk f_dsk pri sec  p_fmem  p_fdsk
495 49148d15 Iustin Pop
     * node1  32762  1280  6000  1861  1026   5   3 0.03907 0.55179
496 49148d15 Iustin Pop
       node2  32762 31280 12000  1861  1026   0   8 0.95476 0.55179
497 49148d15 Iustin Pop
     * node3  32762  1280  6000  1861  1026   5   3 0.03907 0.55179
498 49148d15 Iustin Pop
     * node4  32762  1280  6000  1861  1026   5   3 0.03907 0.55179
499 49148d15 Iustin Pop
     * node5  32762  1280  6000  1861   978   5   5 0.03907 0.52573
500 49148d15 Iustin Pop
     * node6  32762  1280  6000  1861  1026   5   3 0.03907 0.55179
501 49148d15 Iustin Pop
     * node7  32762  1280  6000  1861  1026   5   3 0.03907 0.55179
502 49148d15 Iustin Pop
       node8  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
503 49148d15 Iustin Pop
       node9  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
504 49148d15 Iustin Pop
     * node10 32762  7280 12000  1861  1026   4   4 0.22221 0.55179
505 49148d15 Iustin Pop
       node11 32762  7280  6000  1861   922   4   5 0.22221 0.49577
506 49148d15 Iustin Pop
       node12 32762  7280  6000  1861  1026   4   4 0.22221 0.55179
507 49148d15 Iustin Pop
       node13 32762  7280  6000  1861   922   4   5 0.22221 0.49577
508 49148d15 Iustin Pop
       node14 32762  7280  6000  1861   922   4   5 0.22221 0.49577
509 49148d15 Iustin Pop
     * node15 32762  7280 12000  1861  1131   4   3 0.22221 0.60782
510 49148d15 Iustin Pop
       node16 32762 31280     0  1861  1860   0   0 0.95476 1.00000
511 49148d15 Iustin Pop
       node17 32762  7280  6000  1861  1106   5   3 0.22221 0.59479
512 49148d15 Iustin Pop
     * node18 32762  1280  6000  1396   561   5   3 0.03907 0.40239
513 49148d15 Iustin Pop
     * node19 32762  1280  6000  1861  1026   5   3 0.03907 0.55179
514 49148d15 Iustin Pop
       node20 32762 13280 12000  1861   689   3   9 0.40535 0.37068
515 49148d15 Iustin Pop
516 49148d15 Iustin Pop
    Initial score: 0.52329131
517 49148d15 Iustin Pop
    Trying to minimize the CV...
518 49148d15 Iustin Pop
        1. instance14  node1:node10  => node16:node10 0.42109120 a=f r:node16 f
519 49148d15 Iustin Pop
        2. instance54  node4:node15  => node16:node15 0.31904594 a=f r:node16 f
520 49148d15 Iustin Pop
        3. instance4   node5:node2   => node2:node16  0.26611015 a=f r:node16
521 49148d15 Iustin Pop
        4. instance48  node18:node20 => node2:node18  0.21361717 a=r:node2 f
522 49148d15 Iustin Pop
        5. instance93  node19:node18 => node16:node19 0.16166425 a=r:node16 f
523 49148d15 Iustin Pop
        6. instance89  node3:node20  => node2:node3   0.11005629 a=r:node2 f
524 49148d15 Iustin Pop
        7. instance5   node6:node2   => node16:node6  0.05841589 a=r:node16 f
525 49148d15 Iustin Pop
        8. instance94  node7:node20  => node20:node16 0.00658759 a=f r:node16
526 49148d15 Iustin Pop
        9. instance44  node20:node2  => node2:node15  0.00438740 a=f r:node15
527 49148d15 Iustin Pop
       10. instance62  node14:node18 => node14:node16 0.00390087 a=r:node16
528 49148d15 Iustin Pop
       11. instance13  node11:node14 => node11:node16 0.00361787 a=r:node16
529 49148d15 Iustin Pop
       12. instance19  node10:node11 => node10:node7  0.00336636 a=r:node7
530 49148d15 Iustin Pop
       13. instance43  node12:node13 => node12:node1  0.00305681 a=r:node1
531 49148d15 Iustin Pop
       14. instance1   node1:node2   => node1:node4   0.00263124 a=r:node4
532 49148d15 Iustin Pop
       15. instance58  node19:node20 => node19:node17 0.00252594 a=r:node17
533 49148d15 Iustin Pop
    Cluster score improved from 0.52329131 to 0.00252594
534 49148d15 Iustin Pop
535 49148d15 Iustin Pop
    Commands to run to reach the above solution:
536 49148d15 Iustin Pop
      echo step 1
537 49148d15 Iustin Pop
      echo gnt-instance migrate instance14
538 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance14
539 49148d15 Iustin Pop
      echo gnt-instance migrate instance14
540 49148d15 Iustin Pop
      echo step 2
541 49148d15 Iustin Pop
      echo gnt-instance migrate instance54
542 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance54
543 49148d15 Iustin Pop
      echo gnt-instance migrate instance54
544 49148d15 Iustin Pop
      echo step 3
545 49148d15 Iustin Pop
      echo gnt-instance migrate instance4
546 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance4
547 49148d15 Iustin Pop
      echo step 4
548 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node2 instance48
549 49148d15 Iustin Pop
      echo gnt-instance migrate instance48
550 49148d15 Iustin Pop
      echo step 5
551 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance93
552 49148d15 Iustin Pop
      echo gnt-instance migrate instance93
553 49148d15 Iustin Pop
      echo step 6
554 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node2 instance89
555 49148d15 Iustin Pop
      echo gnt-instance migrate instance89
556 49148d15 Iustin Pop
      echo step 7
557 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance5
558 49148d15 Iustin Pop
      echo gnt-instance migrate instance5
559 49148d15 Iustin Pop
      echo step 8
560 49148d15 Iustin Pop
      echo gnt-instance migrate instance94
561 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance94
562 49148d15 Iustin Pop
      echo step 9
563 49148d15 Iustin Pop
      echo gnt-instance migrate instance44
564 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node15 instance44
565 49148d15 Iustin Pop
      echo step 10
566 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance62
567 49148d15 Iustin Pop
      echo step 11
568 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node16 instance13
569 49148d15 Iustin Pop
      echo step 12
570 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node7 instance19
571 49148d15 Iustin Pop
      echo step 13
572 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node1 instance43
573 49148d15 Iustin Pop
      echo step 14
574 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node4 instance1
575 49148d15 Iustin Pop
      echo step 15
576 49148d15 Iustin Pop
      echo gnt-instance replace-disks -n node17 instance58
577 49148d15 Iustin Pop
578 49148d15 Iustin Pop
    Final cluster status:
579 49148d15 Iustin Pop
    N1 Name   t_mem f_mem r_mem t_dsk f_dsk pri sec  p_fmem  p_fdsk
580 49148d15 Iustin Pop
       node1  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
581 49148d15 Iustin Pop
       node2  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
582 49148d15 Iustin Pop
       node3  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
583 49148d15 Iustin Pop
       node4  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
584 49148d15 Iustin Pop
       node5  32762  7280  6000  1861  1078   4   5 0.22221 0.57947
585 49148d15 Iustin Pop
       node6  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
586 49148d15 Iustin Pop
       node7  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
587 49148d15 Iustin Pop
       node8  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
588 49148d15 Iustin Pop
       node9  32762  7280  6000  1861  1026   4   4 0.22221 0.55179
589 49148d15 Iustin Pop
       node10 32762  7280  6000  1861  1026   4   4 0.22221 0.55179
590 49148d15 Iustin Pop
       node11 32762  7280  6000  1861  1022   4   4 0.22221 0.54951
591 49148d15 Iustin Pop
       node12 32762  7280  6000  1861  1026   4   4 0.22221 0.55179
592 49148d15 Iustin Pop
       node13 32762  7280  6000  1861  1022   4   4 0.22221 0.54951
593 49148d15 Iustin Pop
       node14 32762  7280  6000  1861  1022   4   4 0.22221 0.54951
594 49148d15 Iustin Pop
       node15 32762  7280  6000  1861  1031   4   4 0.22221 0.55408
595 49148d15 Iustin Pop
       node16 32762  7280  6000  1861  1060   4   4 0.22221 0.57007
596 49148d15 Iustin Pop
       node17 32762  7280  6000  1861  1006   5   4 0.22221 0.54105
597 49148d15 Iustin Pop
       node18 32762  7280  6000  1396   761   4   2 0.22221 0.54570
598 49148d15 Iustin Pop
       node19 32762  7280  6000  1861  1026   4   4 0.22221 0.55179
599 49148d15 Iustin Pop
       node20 32762 13280  6000  1861  1089   3   5 0.40535 0.58565
600 49148d15 Iustin Pop
601 49148d15 Iustin Pop
Here we see, beside the step list, the initial and final cluster
602 49148d15 Iustin Pop
status, with the final one showing all nodes being N+1 compliant, and
603 49148d15 Iustin Pop
the command list to reach the final solution. In the initial listing,
604 49148d15 Iustin Pop
we see which nodes are not N+1 compliant.
605 49148d15 Iustin Pop
606 49148d15 Iustin Pop
The algorithm is stable as long as each step above is fully completed,
607 49148d15 Iustin Pop
e.g. in step 8, both the migrate and the replace-disks are
608 49148d15 Iustin Pop
done. Otherwise, if only the migrate is done, the input data is
609 49148d15 Iustin Pop
changed in a way that the program will output a different solution
610 49148d15 Iustin Pop
list (but hopefully will end in the same state).
611 9ff4f2c0 Michael Hanselmann
612 9ff4f2c0 Michael Hanselmann
.. vim: set textwidth=72 :
613 9ff4f2c0 Michael Hanselmann
.. Local Variables:
614 9ff4f2c0 Michael Hanselmann
.. mode: rst
615 9ff4f2c0 Michael Hanselmann
.. fill-column: 72
616 9ff4f2c0 Michael Hanselmann
.. End: