optimize_performance.doxy 23 KB

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  1. /*
  2. * This file is part of the StarPU Handbook.
  3. * Copyright (C) 2009--2011 Universit@'e de Bordeaux 1
  4. * Copyright (C) 2010, 2011, 2012, 2013 Centre National de la Recherche Scientifique
  5. * Copyright (C) 2011, 2012 Institut National de Recherche en Informatique et Automatique
  6. * See the file version.doxy for copying conditions.
  7. */
  8. /*! \page optimizePerformance How to optimize performance with StarPU
  9. TODO: improve!
  10. Simply encapsulating application kernels into tasks already permits to
  11. seamlessly support CPU and GPUs at the same time. To achieve good performance, a
  12. few additional changes are needed.
  13. \section Data_management Data management
  14. When the application allocates data, whenever possible it should use the
  15. starpu_malloc() function, which will ask CUDA or
  16. OpenCL to make the allocation itself and pin the corresponding allocated
  17. memory. This is needed to permit asynchronous data transfer, i.e. permit data
  18. transfer to overlap with computations. Otherwise, the trace will show that the
  19. <c>DriverCopyAsync</c> state takes a lot of time, this is because CUDA or OpenCL
  20. then reverts to synchronous transfers.
  21. By default, StarPU leaves replicates of data wherever they were used, in case they
  22. will be re-used by other tasks, thus saving the data transfer time. When some
  23. task modifies some data, all the other replicates are invalidated, and only the
  24. processing unit which ran that task will have a valid replicate of the data. If the application knows
  25. that this data will not be re-used by further tasks, it should advise StarPU to
  26. immediately replicate it to a desired list of memory nodes (given through a
  27. bitmask). This can be understood like the write-through mode of CPU caches.
  28. \code{.c}
  29. starpu_data_set_wt_mask(img_handle, 1<<0);
  30. \endcode
  31. will for instance request to always automatically transfer a replicate into the
  32. main memory (node 0), as bit 0 of the write-through bitmask is being set.
  33. \code{.c}
  34. starpu_data_set_wt_mask(img_handle, ~0U);
  35. \endcode
  36. will request to always automatically broadcast the updated data to all memory
  37. nodes.
  38. Setting the write-through mask to <c>~0U</c> can also be useful to make sure all
  39. memory nodes always have a copy of the data, so that it is never evicted when
  40. memory gets scarse.
  41. Implicit data dependency computation can become expensive if a lot
  42. of tasks access the same piece of data. If no dependency is required
  43. on some piece of data (e.g. because it is only accessed in read-only
  44. mode, or because write accesses are actually commutative), use the
  45. starpu_data_set_sequential_consistency_flag() function to disable implicit
  46. dependencies on that data.
  47. In the same vein, accumulation of results in the same data can become a
  48. bottleneck. The use of the <c>STARPU_REDUX</c> mode permits to optimize such
  49. accumulation (see \ref Data_reduction).
  50. Applications often need a data just for temporary results. In such a case,
  51. registration can be made without an initial value, for instance this produces a vector data:
  52. \code{.c}
  53. starpu_vector_data_register(&handle, -1, 0, n, sizeof(float));
  54. \endcode
  55. StarPU will then allocate the actual buffer only when it is actually needed,
  56. e.g. directly on the GPU without allocating in main memory.
  57. In the same vein, once the temporary results are not useful any more, the
  58. data should be thrown away. If the handle is not to be reused, it can be
  59. unregistered:
  60. \code{.c}
  61. starpu_unregister_submit(handle);
  62. \endcode
  63. actual unregistration will be done after all tasks working on the handle
  64. terminate.
  65. If the handle is to be reused, instead of unregistering it, it can simply be invalidated:
  66. \code{.c}
  67. starpu_invalidate_submit(handle);
  68. \endcode
  69. the buffers containing the current value will then be freed, and reallocated
  70. only when another task writes some value to the handle.
  71. \section Task_granularity Task granularity
  72. Like any other runtime, StarPU has some overhead to manage tasks. Since
  73. it does smart scheduling and data management, that overhead is not always
  74. neglectable. The order of magnitude of the overhead is typically a couple of
  75. microseconds, which is actually quite smaller than the CUDA overhead itself. The
  76. amount of work that a task should do should thus be somewhat
  77. bigger, to make sure that the overhead becomes neglectible. The offline
  78. performance feedback can provide a measure of task length, which should thus be
  79. checked if bad performance are observed. To get a grasp at the scalability
  80. possibility according to task size, one can run
  81. <c>tests/microbenchs/tasks_size_overhead.sh</c> which draws curves of the
  82. speedup of independent tasks of very small sizes.
  83. The choice of scheduler also has impact over the overhead: for instance, the
  84. <c>dmda</c> scheduler takes time to make a decision, while <c>eager</c> does
  85. not. <c>tasks_size_overhead.sh</c> can again be used to get a grasp at how much
  86. impact that has on the target machine.
  87. \section Task_submission Task submission
  88. To let StarPU make online optimizations, tasks should be submitted
  89. asynchronously as much as possible. Ideally, all the tasks should be
  90. submitted, and mere calls to starpu_task_wait_for_all() or
  91. starpu_data_unregister() be done to wait for
  92. termination. StarPU will then be able to rework the whole schedule, overlap
  93. computation with communication, manage accelerator local memory usage, etc.
  94. \section Task_priorities Task priorities
  95. By default, StarPU will consider the tasks in the order they are submitted by
  96. the application. If the application programmer knows that some tasks should
  97. be performed in priority (for instance because their output is needed by many
  98. other tasks and may thus be a bottleneck if not executed early enough), the
  99. <c>priority</c> field of the task structure should be set to transmit the
  100. priority information to StarPU.
  101. \section Task_scheduling_policy Task scheduling policy
  102. By default, StarPU uses the <c>eager</c> simple greedy scheduler. This is
  103. because it provides correct load balance even if the application codelets do not
  104. have performance models. If your application codelets have performance models
  105. (\ref Performance_model_example for example showing how to do it),
  106. you should change the scheduler thanks to the <c>STARPU_SCHED</c> environment
  107. variable. For instance <c>export STARPU_SCHED=dmda</c> . Use <c>help</c> to get
  108. the list of available schedulers.
  109. The <b>eager</b> scheduler uses a central task queue, from which workers draw tasks
  110. to work on. This however does not permit to prefetch data since the scheduling
  111. decision is taken late. If a task has a non-0 priority, it is put at the front of the queue.
  112. The <b>prio</b> scheduler also uses a central task queue, but sorts tasks by
  113. priority (between -5 and 5).
  114. The <b>random</b> scheduler distributes tasks randomly according to assumed worker
  115. overall performance.
  116. The <b>ws</b> (work stealing) scheduler schedules tasks on the local worker by
  117. default. When a worker becomes idle, it steals a task from the most loaded
  118. worker.
  119. The <b>dm</b> (deque model) scheduler uses task execution performance models into account to
  120. perform an HEFT-similar scheduling strategy: it schedules tasks where their
  121. termination time will be minimal.
  122. The <b>dmda</b> (deque model data aware) scheduler is similar to dm, it also takes
  123. into account data transfer time.
  124. The <b>dmdar</b> (deque model data aware ready) scheduler is similar to dmda,
  125. it also sorts tasks on per-worker queues by number of already-available data
  126. buffers.
  127. The <b>dmdas</b> (deque model data aware sorted) scheduler is similar to dmda, it
  128. also supports arbitrary priority values.
  129. The <b>heft</b> (heterogeneous earliest finish time) scheduler is deprecated. It
  130. is now just an alias for <b>dmda</b>.
  131. The <b>pheft</b> (parallel HEFT) scheduler is similar to heft, it also supports
  132. parallel tasks (still experimental).
  133. The <b>peager</b> (parallel eager) scheduler is similar to eager, it also
  134. supports parallel tasks (still experimental).
  135. \section Performance_model_calibration Performance model calibration
  136. Most schedulers are based on an estimation of codelet duration on each kind
  137. of processing unit. For this to be possible, the application programmer needs
  138. to configure a performance model for the codelets of the application (see
  139. \ref Performance_model_example for instance). History-based performance models
  140. use on-line calibration. StarPU will automatically calibrate codelets
  141. which have never been calibrated yet, and save the result in
  142. <c>$STARPU_HOME/.starpu/sampling/codelets</c>.
  143. The models are indexed by machine name. To share the models between machines (e.g. for a homogeneous cluster), use <c>export STARPU_HOSTNAME=some_global_name</c>. To force continuing calibration, use
  144. <c>export STARPU_CALIBRATE=1</c> . This may be necessary if your application
  145. has not-so-stable performance. StarPU will force calibration (and thus ignore
  146. the current result) until 10 (_STARPU_CALIBRATION_MINIMUM) measurements have been
  147. made on each architecture, to avoid badly scheduling tasks just because the
  148. first measurements were not so good. Details on the current performance model status
  149. can be obtained from the <c>starpu_perfmodel_display</c> command: the <c>-l</c>
  150. option lists the available performance models, and the <c>-s</c> option permits
  151. to choose the performance model to be displayed. The result looks like:
  152. \verbatim
  153. $ starpu_perfmodel_display -s starpu_dlu_lu_model_22
  154. performance model for cpu
  155. # hash size mean dev n
  156. 880805ba 98304 2.731309e+02 6.010210e+01 1240
  157. b50b6605 393216 1.469926e+03 1.088828e+02 1240
  158. 5c6c3401 1572864 1.125983e+04 3.265296e+03 1240
  159. \endverbatim
  160. Which shows that for the LU 22 kernel with a 1.5MiB matrix, the average
  161. execution time on CPUs was about 11ms, with a 3ms standard deviation, over
  162. 1240 samples. It is a good idea to check this before doing actual performance
  163. measurements.
  164. A graph can be drawn by using the <c>starpu_perfmodel_plot</c>:
  165. \verbatim
  166. $ starpu_perfmodel_plot -s starpu_dlu_lu_model_22
  167. 98304 393216 1572864
  168. $ gnuplot starpu_starpu_dlu_lu_model_22.gp
  169. $ gv starpu_starpu_dlu_lu_model_22.eps
  170. \endverbatim
  171. If a kernel source code was modified (e.g. performance improvement), the
  172. calibration information is stale and should be dropped, to re-calibrate from
  173. start. This can be done by using <c>export STARPU_CALIBRATE=2</c>.
  174. Note: due to CUDA limitations, to be able to measure kernel duration,
  175. calibration mode needs to disable asynchronous data transfers. Calibration thus
  176. disables data transfer / computation overlapping, and should thus not be used
  177. for eventual benchmarks. Note 2: history-based performance models get calibrated
  178. only if a performance-model-based scheduler is chosen.
  179. The history-based performance models can also be explicitly filled by the
  180. application without execution, if e.g. the application already has a series of
  181. measurements. This can be done by using starpu_perfmodel_update_history(),
  182. for instance:
  183. \code{.c}
  184. static struct starpu_perfmodel perf_model = {
  185. .type = STARPU_HISTORY_BASED,
  186. .symbol = "my_perfmodel",
  187. };
  188. struct starpu_codelet cl = {
  189. .where = STARPU_CUDA,
  190. .cuda_funcs = { cuda_func1, cuda_func2, NULL },
  191. .nbuffers = 1,
  192. .modes = {STARPU_W},
  193. .model = &perf_model
  194. };
  195. void feed(void) {
  196. struct my_measure *measure;
  197. struct starpu_task task;
  198. starpu_task_init(&task);
  199. task.cl = &cl;
  200. for (measure = &measures[0]; measure < measures[last]; measure++) {
  201. starpu_data_handle_t handle;
  202. starpu_vector_data_register(&handle, -1, 0, measure->size, sizeof(float));
  203. task.handles[0] = handle;
  204. starpu_perfmodel_update_history(&perf_model, &task,
  205. STARPU_CUDA_DEFAULT + measure->cudadev, 0,
  206. measure->implementation, measure->time);
  207. starpu_task_clean(&task);
  208. starpu_data_unregister(handle);
  209. }
  210. }
  211. \endcode
  212. Measurement has to be provided in milliseconds for the completion time models,
  213. and in Joules for the energy consumption models.
  214. \section Task_distribution_vs_Data_transfer Task distribution vs Data transfer
  215. Distributing tasks to balance the load induces data transfer penalty. StarPU
  216. thus needs to find a balance between both. The target function that the
  217. <c>dmda</c> scheduler of StarPU
  218. tries to minimize is <c>alpha * T_execution + beta * T_data_transfer</c>, where
  219. <c>T_execution</c> is the estimated execution time of the codelet (usually
  220. accurate), and <c>T_data_transfer</c> is the estimated data transfer time. The
  221. latter is estimated based on bus calibration before execution start,
  222. i.e. with an idle machine, thus without contention. You can force bus re-calibration by running
  223. <c>starpu_calibrate_bus</c>. The beta parameter defaults to 1, but it can be
  224. worth trying to tweak it by using <c>export STARPU_SCHED_BETA=2</c> for instance,
  225. since during real application execution, contention makes transfer times bigger.
  226. This is of course imprecise, but in practice, a rough estimation already gives
  227. the good results that a precise estimation would give.
  228. \section Data_prefetch Data prefetch
  229. The <c>heft</c>, <c>dmda</c> and <c>pheft</c> scheduling policies perform data prefetch (see @ref{STARPU_PREFETCH}):
  230. as soon as a scheduling decision is taken for a task, requests are issued to
  231. transfer its required data to the target processing unit, if needeed, so that
  232. when the processing unit actually starts the task, its data will hopefully be
  233. already available and it will not have to wait for the transfer to finish.
  234. The application may want to perform some manual prefetching, for several reasons
  235. such as excluding initial data transfers from performance measurements, or
  236. setting up an initial statically-computed data distribution on the machine
  237. before submitting tasks, which will thus guide StarPU toward an initial task
  238. distribution (since StarPU will try to avoid further transfers).
  239. This can be achieved by giving the starpu_data_prefetch_on_node() function
  240. the handle and the desired target memory node.
  241. \section Power-based_scheduling Power-based scheduling
  242. If the application can provide some power performance model (through
  243. the <c>power_model</c> field of the codelet structure), StarPU will
  244. take it into account when distributing tasks. The target function that
  245. the <c>dmda</c> scheduler minimizes becomes <c>alpha * T_execution +
  246. beta * T_data_transfer + gamma * Consumption</c> , where <c>Consumption</c>
  247. is the estimated task consumption in Joules. To tune this parameter, use
  248. <c>export STARPU_SCHED_GAMMA=3000</c> for instance, to express that each Joule
  249. (i.e kW during 1000us) is worth 3000us execution time penalty. Setting
  250. <c>alpha</c> and <c>beta</c> to zero permits to only take into account power consumption.
  251. This is however not sufficient to correctly optimize power: the scheduler would
  252. simply tend to run all computations on the most energy-conservative processing
  253. unit. To account for the consumption of the whole machine (including idle
  254. processing units), the idle power of the machine should be given by setting
  255. <c>export STARPU_IDLE_POWER=200</c> for 200W, for instance. This value can often
  256. be obtained from the machine power supplier.
  257. The power actually consumed by the total execution can be displayed by setting
  258. <c>export STARPU_PROFILING=1 STARPU_WORKER_STATS=1</c> .
  259. On-line task consumption measurement is currently only supported through the
  260. <c>CL_PROFILING_POWER_CONSUMED</c> OpenCL extension, implemented in the MoviSim
  261. simulator. Applications can however provide explicit measurements by using the
  262. starpu_perfmodel_update_history() function (examplified in \ref Performance_model_example
  263. with the <c>power_model</c> performance model. Fine-grain
  264. measurement is often not feasible with the feedback provided by the hardware, so
  265. the user can for instance run a given task a thousand times, measure the global
  266. consumption for that series of tasks, divide it by a thousand, repeat for
  267. varying kinds of tasks and task sizes, and eventually feed StarPU
  268. with these manual measurements through starpu_perfmodel_update_history().
  269. \section Static_scheduling Static scheduling
  270. In some cases, one may want to force some scheduling, for instance force a given
  271. set of tasks to GPU0, another set to GPU1, etc. while letting some other tasks
  272. be scheduled on any other device. This can indeed be useful to guide StarPU into
  273. some work distribution, while still letting some degree of dynamism. For
  274. instance, to force execution of a task on CUDA0:
  275. \code{.c}
  276. task->execute_on_a_specific_worker = 1;
  277. task->worker = starpu_worker_get_by_type(STARPU_CUDA_WORKER, 0);
  278. \endcode
  279. \section Profiling Profiling
  280. A quick view of how many tasks each worker has executed can be obtained by setting
  281. <c>export STARPU_WORKER_STATS=1</c> This is a convenient way to check that
  282. execution did happen on accelerators without penalizing performance with
  283. the profiling overhead.
  284. A quick view of how much data transfers have been issued can be obtained by setting
  285. <c>export STARPU_BUS_STATS=1</c> .
  286. More detailed profiling information can be enabled by using <c>export STARPU_PROFILING=1</c> or by
  287. calling starpu_profiling_status_set() from the source code.
  288. Statistics on the execution can then be obtained by using <c>export
  289. STARPU_BUS_STATS=1</c> and <c>export STARPU_WORKER_STATS=1</c> .
  290. More details on performance feedback are provided by the next chapter.
  291. \section CUDA-specific_optimizations CUDA-specific optimizations
  292. Due to CUDA limitations, StarPU will have a hard time overlapping its own
  293. communications and the codelet computations if the application does not use a
  294. dedicated CUDA stream for its computations instead of the default stream,
  295. which synchronizes all operations of the GPU. StarPU provides one by the use
  296. of starpu_cuda_get_local_stream() which can be used by all CUDA codelet
  297. operations to avoid this issue. For instance:
  298. \code{.c}
  299. func <<<grid,block,0,starpu_cuda_get_local_stream()>>> (foo, bar);
  300. cudaStreamSynchronize(starpu_cuda_get_local_stream());
  301. \endcode
  302. StarPU already does appropriate calls for the CUBLAS library.
  303. Unfortunately, some CUDA libraries do not have stream variants of
  304. kernels. That will lower the potential for overlapping.
  305. \section Performance_debugging Performance debugging
  306. To get an idea of what is happening, a lot of performance feedback is available,
  307. detailed in the next chapter. The various informations should be checked for.
  308. <ul>
  309. <li>
  310. What does the Gantt diagram look like? (see \ref Creating_a_Gantt_Diagram)
  311. <ul>
  312. <li> If it's mostly green (tasks running in the initial context) or context specific
  313. color prevailing, then the machine is properly
  314. utilized, and perhaps the codelets are just slow. Check their performance, see
  315. \ref Performance_of_codelets.
  316. </li>
  317. <li> If it's mostly purple (FetchingInput), tasks keep waiting for data
  318. transfers, do you perhaps have far more communication than computation? Did
  319. you properly use CUDA streams to make sure communication can be
  320. overlapped? Did you use data-locality aware schedulers to avoid transfers as
  321. much as possible?
  322. </li>
  323. <li> If it's mostly red (Blocked), tasks keep waiting for dependencies,
  324. do you have enough parallelism? It might be a good idea to check what the DAG
  325. looks like (see \ref Creating_a_DAG_with_graphviz).
  326. </li>
  327. <li> If only some workers are completely red (Blocked), for some reason the
  328. scheduler didn't assign tasks to them. Perhaps the performance model is bogus,
  329. check it (see \ref Performance_of_codelets). Do all your codelets have a
  330. performance model? When some of them don't, the schedulers switches to a
  331. greedy algorithm which thus performs badly.
  332. </li>
  333. </ul>
  334. </li>
  335. </ul>
  336. You can also use the Temanejo task debugger (see \ref Using_the_Temanejo_task_debugger) to
  337. visualize the task graph more easily.
  338. \section Simulated_performance Simulated performance
  339. StarPU can use Simgrid in order to simulate execution on an arbitrary
  340. platform.
  341. \subsection Calibration Calibration
  342. The idea is to first compile StarPU normally, and run the application,
  343. so as to automatically benchmark the bus and the codelets.
  344. \verbatim
  345. $ ./configure && make
  346. $ STARPU_SCHED=dmda ./examples/matvecmult/matvecmult
  347. [starpu][_starpu_load_history_based_model] Warning: model matvecmult
  348. is not calibrated, forcing calibration for this run. Use the
  349. STARPU_CALIBRATE environment variable to control this.
  350. $ ...
  351. $ STARPU_SCHED=dmda ./examples/matvecmult/matvecmult
  352. TEST PASSED
  353. \endverbatim
  354. Note that we force to use the dmda scheduler to generate performance
  355. models for the application. The application may need to be run several
  356. times before the model is calibrated.
  357. \subsection Simulation Simulation
  358. Then, recompile StarPU, passing <c>--enable-simgrid</c> to <c>./configure</c>, and re-run the
  359. application:
  360. \verbatim
  361. $ ./configure --enable-simgrid && make
  362. $ STARPU_SCHED=dmda ./examples/matvecmult/matvecmult
  363. TEST FAILED !!!
  364. \endverbatim
  365. It is normal that the test fails: since the computation are not actually done
  366. (that is the whole point of simgrid), the result is wrong, of course.
  367. If the performance model is not calibrated enough, the following error
  368. message will be displayed
  369. \verbatim
  370. $ STARPU_SCHED=dmda ./examples/matvecmult/matvecmult
  371. [starpu][_starpu_load_history_based_model] Warning: model matvecmult
  372. is not calibrated, forcing calibration for this run. Use the
  373. STARPU_CALIBRATE environment variable to control this.
  374. [starpu][_starpu_simgrid_execute_job][assert failure] Codelet
  375. matvecmult does not have a perfmodel, or is not calibrated enough
  376. \endverbatim
  377. The number of devices can be chosen as usual with <c>STARPU_NCPU</c>,
  378. <c>STARPU_NCUDA</c>, and <c>STARPU_NOPENCL</c>. For now, only the number of
  379. cpus can be arbitrarily chosen. The number of CUDA and OpenCL devices have to be
  380. lower than the real number on the current machine.
  381. The amount of simulated GPU memory is for now unbound by default, but
  382. it can be chosen by hand through the <c>STARPU_LIMIT_CUDA_MEM</c>,
  383. <c>STARPU_LIMIT_CUDA_devid_MEM</c>, <c>STARPU_LIMIT_OPENCL_MEM</c>, and
  384. <c>STARPU_LIMIT_OPENCL_devid_MEM</c> environment variables.
  385. The Simgrid default stack size is small; to increase it use the
  386. parameter <c>--cfg=contexts/stack_size</c>, for example:
  387. \verbatim
  388. $ ./example --cfg=contexts/stack_size:8192
  389. TEST FAILED !!!
  390. \endverbatim
  391. Note: of course, if the application uses <c>gettimeofday</c> to make its
  392. performance measurements, the real time will be used, which will be bogus. To
  393. get the simulated time, it has to use starpu_timing_now() which returns the
  394. virtual timestamp in ms.
  395. \subsection Simulation_on_another_machine Simulation on another machine
  396. The simgrid support even permits to perform simulations on another machine, your
  397. desktop, typically. To achieve this, one still needs to perform the Calibration
  398. step on the actual machine to be simulated, then copy them to your desktop
  399. machine (the <c>$STARPU_HOME/.starpu</c> directory). One can then perform the
  400. Simulation step on the desktop machine, by setting the <c>STARPU_HOSTNAME</c>
  401. environment variable to the name of the actual machine, to make StarPU use the
  402. performance models of the simulated machine even on the desktop machine.
  403. If the desktop machine does not have CUDA or OpenCL, StarPU is still able to
  404. use simgrid to simulate execution with CUDA/OpenCL devices, but the application
  405. source code will probably disable the CUDA and OpenCL codelets in that
  406. case. Since during simgrid execution, the functions of the codelet are actually
  407. not called, one can use dummy functions such as the following to still permit
  408. CUDA or OpenCL execution:
  409. \code{.c}
  410. static struct starpu_codelet cl11 =
  411. {
  412. .cpu_funcs = {chol_cpu_codelet_update_u11, NULL},
  413. #ifdef STARPU_USE_CUDA
  414. .cuda_funcs = {chol_cublas_codelet_update_u11, NULL},
  415. #elif defined(STARPU_SIMGRID)
  416. .cuda_funcs = {(void*)1, NULL},
  417. #endif
  418. .nbuffers = 1,
  419. .modes = {STARPU_RW},
  420. .model = &chol_model_11
  421. };
  422. \endcode
  423. */