380_offline_performance_tools.doxy 24 KB

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  1. /*
  2. * This file is part of the StarPU Handbook.
  3. * Copyright (C) 2009--2011 Universit@'e de Bordeaux
  4. * Copyright (C) 2010, 2011, 2012, 2013, 2014, 2016 CNRS
  5. * Copyright (C) 2011, 2012 INRIA
  6. * See the file version.doxy for copying conditions.
  7. */
  8. /*! \page OfflinePerformanceTools Offline Performance Tools
  9. To get an idea of what is happening, a lot of performance feedback is available,
  10. detailed in this chapter. The various informations should be checked for.
  11. <ul>
  12. <li>
  13. What does the Gantt diagram look like? (see \ref CreatingAGanttDiagram)
  14. <ul>
  15. <li> If it's mostly green (tasks running in the initial context) or context specific
  16. color prevailing, then the machine is properly
  17. utilized, and perhaps the codelets are just slow. Check their performance, see
  18. \ref PerformanceOfCodelets.
  19. </li>
  20. <li> If it's mostly purple (FetchingInput), tasks keep waiting for data
  21. transfers, do you perhaps have far more communication than computation? Did
  22. you properly use CUDA streams to make sure communication can be
  23. overlapped? Did you use data-locality aware schedulers to avoid transfers as
  24. much as possible?
  25. </li>
  26. <li> If it's mostly red (Blocked), tasks keep waiting for dependencies,
  27. do you have enough parallelism? It might be a good idea to check what the DAG
  28. looks like (see \ref CreatingADAGWithGraphviz).
  29. </li>
  30. <li> If only some workers are completely red (Blocked), for some reason the
  31. scheduler didn't assign tasks to them. Perhaps the performance model is bogus,
  32. check it (see \ref PerformanceOfCodelets). Do all your codelets have a
  33. performance model? When some of them don't, the schedulers switches to a
  34. greedy algorithm which thus performs badly.
  35. </li>
  36. </ul>
  37. </li>
  38. </ul>
  39. You can also use the Temanejo task debugger (see \ref UsingTheTemanejoTaskDebugger) to
  40. visualize the task graph more easily.
  41. \section Off-linePerformanceFeedback Off-line Performance Feedback
  42. \subsection GeneratingTracesWithFxT Generating Traces With FxT
  43. StarPU can use the FxT library (see
  44. https://savannah.nongnu.org/projects/fkt/) to generate traces
  45. with a limited runtime overhead.
  46. You can either get a tarball:
  47. \verbatim
  48. $ wget http://download.savannah.gnu.org/releases/fkt/fxt-0.2.11.tar.gz
  49. \endverbatim
  50. or use the FxT library from CVS (autotools are required):
  51. \verbatim
  52. $ cvs -d :pserver:anonymous\@cvs.sv.gnu.org:/sources/fkt co FxT
  53. $ ./bootstrap
  54. \endverbatim
  55. Compiling and installing the FxT library in the <c>$FXTDIR</c> path is
  56. done following the standard procedure:
  57. \verbatim
  58. $ ./configure --prefix=$FXTDIR
  59. $ make
  60. $ make install
  61. \endverbatim
  62. In order to have StarPU to generate traces, StarPU should be configured with
  63. the option \ref with-fxt "--with-fxt" :
  64. \verbatim
  65. $ ./configure --with-fxt=$FXTDIR
  66. \endverbatim
  67. Or you can simply point the <c>PKG_CONFIG_PATH</c> to
  68. <c>$FXTDIR/lib/pkgconfig</c> and pass
  69. \ref with-fxt "--with-fxt" to <c>./configure</c>
  70. When FxT is enabled, a trace is generated when StarPU is terminated by calling
  71. starpu_shutdown(). The trace is a binary file whose name has the form
  72. <c>prof_file_XXX_YYY</c> where <c>XXX</c> is the user name, and
  73. <c>YYY</c> is the pid of the process that used StarPU. This file is saved in the
  74. <c>/tmp/</c> directory by default, or by the directory specified by
  75. the environment variable \ref STARPU_FXT_PREFIX.
  76. The additional configure option \ref enable-fxt-lock "--enable-fxt-lock" can
  77. be used to generate trace events which describes the locks behaviour during
  78. the execution. It is however very heavy and should not be used unless debugging
  79. StarPU's internal locking.
  80. The environment variable \ref STARPU_FXT_TRACE can be set to 0 to disable the
  81. generation of the <c>prof_file_XXX_YYY</c> file.
  82. \subsection CreatingAGanttDiagram Creating a Gantt Diagram
  83. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  84. generate a trace in the Paje format by calling:
  85. \verbatim
  86. $ starpu_fxt_tool -i /tmp/prof_file_something
  87. \endverbatim
  88. Or alternatively, setting the environment variable \ref STARPU_GENERATE_TRACE
  89. to <c>1</c> before application execution will make StarPU do it automatically at
  90. application shutdown.
  91. This will create a file <c>paje.trace</c> in the current directory that
  92. can be inspected with the ViTE (http://vite.gforge.inria.fr/) trace
  93. visualizing open-source tool. It is possible to open the
  94. file <c>paje.trace</c> with ViTE by using the following command:
  95. \verbatim
  96. $ vite paje.trace
  97. \endverbatim
  98. To get names of tasks instead of "unknown", fill the optional
  99. starpu_codelet::name, or use a performance model for them.
  100. In the MPI execution case, \ref STARPU_GENERATE_TRACE will not work as expected
  101. (each node will try to generate paje.trace, thus mixing outputs...), you have to
  102. collect the trace files from the MPI nodes, and
  103. specify them all on the command <c>starpu_fxt_tool</c>, for instance:
  104. \verbatim
  105. $ starpu_fxt_tool -i /tmp/prof_file_something*
  106. \endverbatim
  107. By default, all tasks are displayed using a green color. To display tasks with
  108. varying colors, pass option <c>-c</c> to <c>starpu_fxt_tool</c>.
  109. By default, the trace contains all informations. To reduce the trace size,
  110. various <c>-no-foo</c> options can be passed to <c>starpu_fxt_tool</c>, see
  111. <c>starpu_fxt_tool --help</c> .
  112. To identify tasks precisely, the application can set the starpu_task::tag_id field of the
  113. task (or use \ref STARPU_TAG_ONLY when using starpu_task_insert()), and
  114. the value of the tag will show up in the trace.
  115. It can also set the starpu_task::name field of the task (or use \ref STARPU_NAME)
  116. when using starpu_task_insert()), to replace in traces the name of the codelet
  117. with an arbitrarily chosen name.
  118. It can also set the iteration number, by just calling starpu_iteration_push()
  119. at the beginning of submission loops and starpu_iteration_pop() at the end of
  120. submission loops. These iteration numbers will show up in traces for all tasks
  121. submitted from there.
  122. Coordinates can also be given to data with the starpu_data_set_coordinates() or
  123. starpu_data_set_coordinates_array() function. In the trace, tasks will then be
  124. assigned the coordinates of the first data they write to.
  125. Traces can also be inspected by hand by using the tool <c>fxt_print</c>, for instance:
  126. \verbatim
  127. $ fxt_print -o -f /tmp/prof_file_something
  128. \endverbatim
  129. Timings are in nanoseconds (while timings as seen in ViTE are in milliseconds).
  130. \subsection CreatingADAGWithGraphviz Creating a DAG With Graphviz
  131. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  132. generate a task graph in the DOT format by calling:
  133. \verbatim
  134. $ starpu_fxt_tool -i /tmp/prof_file_something
  135. \endverbatim
  136. This will create a <c>dag.dot</c> file in the current directory. This file is a
  137. task graph described using the DOT language. It is possible to get a
  138. graphical output of the graph by using the graphviz library:
  139. \verbatim
  140. $ dot -Tpdf dag.dot -o output.pdf
  141. \endverbatim
  142. \subsection TraceTaskDetails Getting Task Details
  143. When the FxT trace file <c>prof_file_something</c> has been generated, details on the
  144. executed tasks can be retrieved by calling:
  145. \verbatim
  146. $ starpu_fxt_tool -i /tmp/prof_file_something
  147. \endverbatim
  148. This will create a <c>tasks.rec</c> file in the current directory. This file
  149. is in the recutils format, i.e. <c>Field: value</c> lines, and empty lines to
  150. separate each task. This can be used as a convenient input for various ad-hoc
  151. analysis tools. By default it only contains information about the actual
  152. execution. Performance models can be obtained by running
  153. <c>starpu_tasks_rec_complete</c> on it:
  154. \verbatim
  155. $ starpu_tasks_rec_complete tasks.rec tasks2.rec
  156. \endverbatim
  157. which will add <c>EstimatedTime</c> lines which contain the performance
  158. model-estimated time (in µs) for each worker starting from 0. Since it needs
  159. the performance models, it needs to be run the same way as the application
  160. execution, or at least with <c>STARPU_HOSTNAME</c> set to the hostname of the
  161. machine used for execution, to get the performance models of that machine.
  162. \subsection MonitoringActivity Monitoring Activity
  163. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  164. generate an activity trace by calling:
  165. \verbatim
  166. $ starpu_fxt_tool -i /tmp/prof_file_something
  167. \endverbatim
  168. This will create a file <c>activity.data</c> in the current
  169. directory. A profile of the application showing the activity of StarPU
  170. during the execution of the program can be generated:
  171. \verbatim
  172. $ starpu_workers_activity activity.data
  173. \endverbatim
  174. This will create a file named <c>activity.eps</c> in the current directory.
  175. This picture is composed of two parts.
  176. The first part shows the activity of the different workers. The green sections
  177. indicate which proportion of the time was spent executed kernels on the
  178. processing unit. The red sections indicate the proportion of time spent in
  179. StartPU: an important overhead may indicate that the granularity may be too
  180. low, and that bigger tasks may be appropriate to use the processing unit more
  181. efficiently. The black sections indicate that the processing unit was blocked
  182. because there was no task to process: this may indicate a lack of parallelism
  183. which may be alleviated by creating more tasks when it is possible.
  184. The second part of the picture <c>activity.eps</c> is a graph showing the
  185. evolution of the number of tasks available in the system during the execution.
  186. Ready tasks are shown in black, and tasks that are submitted but not
  187. schedulable yet are shown in grey.
  188. \subsection Animation Getting Modular Schedular Animation
  189. When using modular schedulers (i.e. schedulers which use a modular architecture,
  190. and whose name start with "modular-"), the command
  191. \verbatim
  192. $ starpu_fxt_tool -i /tmp/prof_file_something
  193. \endverbatim
  194. will also produce a <c>trace.html</c> file which can be viewed in a
  195. javascript-enabled web browser. It shows the flow of tasks between the
  196. components of the modular scheduler.
  197. \subsection LimitingScopeTrace Limiting The Scope Of The Trace
  198. For computing statistics, it is useful to limit the trace to a given portion of
  199. the time of the whole execution. This can be achieved by calling
  200. \code{.c}
  201. starpu_fxt_autostart_profiling(0)
  202. \endcode
  203. before calling starpu_init(), to
  204. prevent tracing from starting immediately. Then
  205. \code{.c}
  206. starpu_fxt_start_profiling();
  207. \endcode
  208. and
  209. \code{.c}
  210. starpu_fxt_stop_profiling();
  211. \endcode
  212. can be used around the portion of code to be traced. This will show up as marks
  213. in the trace, and states of workers will only show up for that portion.
  214. \section PerformanceOfCodelets Performance Of Codelets
  215. The performance model of codelets (see \ref PerformanceModelExample)
  216. can be examined by using the tool <c>starpu_perfmodel_display</c>:
  217. \verbatim
  218. $ starpu_perfmodel_display -l
  219. file: <malloc_pinned.hannibal>
  220. file: <starpu_slu_lu_model_21.hannibal>
  221. file: <starpu_slu_lu_model_11.hannibal>
  222. file: <starpu_slu_lu_model_22.hannibal>
  223. file: <starpu_slu_lu_model_12.hannibal>
  224. \endverbatim
  225. Here, the codelets of the example <c>lu</c> are available. We can examine the
  226. performance of the kernel <c>22</c> (in micro-seconds), which is history-based:
  227. \verbatim
  228. $ starpu_perfmodel_display -s starpu_slu_lu_model_22
  229. performance model for cpu
  230. # hash size mean dev n
  231. 57618ab0 19660800 2.851069e+05 1.829369e+04 109
  232. performance model for cuda_0
  233. # hash size mean dev n
  234. 57618ab0 19660800 1.164144e+04 1.556094e+01 315
  235. performance model for cuda_1
  236. # hash size mean dev n
  237. 57618ab0 19660800 1.164271e+04 1.330628e+01 360
  238. performance model for cuda_2
  239. # hash size mean dev n
  240. 57618ab0 19660800 1.166730e+04 3.390395e+02 456
  241. \endverbatim
  242. We can see that for the given size, over a sample of a few hundreds of
  243. execution, the GPUs are about 20 times faster than the CPUs (numbers are in
  244. us). The standard deviation is extremely low for the GPUs, and less than 10% for
  245. CPUs.
  246. This tool can also be used for regression-based performance models. It will then
  247. display the regression formula, and in the case of non-linear regression, the
  248. same performance log as for history-based performance models:
  249. \verbatim
  250. $ starpu_perfmodel_display -s non_linear_memset_regression_based
  251. performance model for cpu_impl_0
  252. Regression : #sample = 1400
  253. Linear: y = alpha size ^ beta
  254. alpha = 1.335973e-03
  255. beta = 8.024020e-01
  256. Non-Linear: y = a size ^b + c
  257. a = 5.429195e-04
  258. b = 8.654899e-01
  259. c = 9.009313e-01
  260. # hash size mean stddev n
  261. a3d3725e 4096 4.763200e+00 7.650928e-01 100
  262. 870a30aa 8192 1.827970e+00 2.037181e-01 100
  263. 48e988e9 16384 2.652800e+00 1.876459e-01 100
  264. 961e65d2 32768 4.255530e+00 3.518025e-01 100
  265. ...
  266. \endverbatim
  267. The same can also be achieved by using StarPU's library API, see
  268. \ref API_Performance_Model and notably the function
  269. starpu_perfmodel_load_symbol(). The source code of the tool
  270. <c>starpu_perfmodel_display</c> can be a useful example.
  271. The tool <c>starpu_perfmodel_plot</c> can be used to draw performance
  272. models. It writes a <c>.gp</c> file in the current directory, to be
  273. run with the tool <c>gnuplot</c>, which shows the corresponding curve.
  274. \image html starpu_non_linear_memset_regression_based.png
  275. \image latex starpu_non_linear_memset_regression_based.eps "" width=\textwidth
  276. When the field starpu_task::flops is set (or \ref STARPU_FLOPS is passed to
  277. starpu_task_insert()), <c>starpu_perfmodel_plot</c> can directly draw a GFlops
  278. curve, by simply adding the <c>-f</c> option:
  279. \verbatim
  280. $ starpu_perfmodel_plot -f -s chol_model_11
  281. \endverbatim
  282. This will however disable displaying the regression model, for which we can not
  283. compute GFlops.
  284. \image html starpu_chol_model_11_type.png
  285. \image latex starpu_chol_model_11_type.eps "" width=\textwidth
  286. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  287. get a profiling of each codelet by calling:
  288. \verbatim
  289. $ starpu_fxt_tool -i /tmp/prof_file_something
  290. $ starpu_codelet_profile distrib.data codelet_name
  291. \endverbatim
  292. This will create profiling data files, and a <c>distrib.data.gp</c> file in the current
  293. directory, which draws the distribution of codelet time over the application
  294. execution, according to data input size.
  295. \image html distrib_data.png
  296. \image latex distrib_data.eps "" width=\textwidth
  297. This is also available in the tool <c>starpu_perfmodel_plot</c>, by passing it
  298. the fxt trace:
  299. \verbatim
  300. $ starpu_perfmodel_plot -s non_linear_memset_regression_based -i /tmp/prof_file_foo_0
  301. \endverbatim
  302. It will produce a <c>.gp</c> file which contains both the performance model
  303. curves, and the profiling measurements.
  304. \image html starpu_non_linear_memset_regression_based_2.png
  305. \image latex starpu_non_linear_memset_regression_based_2.eps "" width=\textwidth
  306. If you have the statistical tool <c>R</c> installed, you can additionally use
  307. \verbatim
  308. $ starpu_codelet_histo_profile distrib.data
  309. \endverbatim
  310. Which will create one <c>.pdf</c> file per codelet and per input size, showing a
  311. histogram of the codelet execution time distribution.
  312. \image html distrib_data_histo.png
  313. \image latex distrib_data_histo.eps "" width=\textwidth
  314. \section TraceStatistics Trace Statistics
  315. More than just codelet performance, it is interesting to get statistics over all
  316. kinds of StarPU states (allocations, data transfers, etc.). This is particularly
  317. useful to check what may have gone wrong in the accurracy of the simgrid
  318. simulation.
  319. This requires the <c>R</c> statistical tool, with the <c>plyr</c>,
  320. <c>ggplot2</c> and <c>data.table</c> packages. If your system
  321. distribution does not have packages for these, one can fetch them from
  322. <c>CRAN</c>:
  323. \verbatim
  324. $ R
  325. > install.packages("plyr")
  326. > install.packages("ggplot2")
  327. > install.packages("data.table")
  328. > install.packages("knitr")
  329. \endverbatim
  330. The <c>pj_dump</c> tool from <c>pajeng</c> is also needed (see
  331. https://github.com/schnorr/pajeng)
  332. One can then get textual or <c>.csv</c> statistics over the trace states:
  333. \verbatim
  334. $ starpu_paje_state_stats -v native.trace simgrid.trace
  335. "Value" "Events_native.csv" "Duration_native.csv" "Events_simgrid.csv" "Duration_simgrid.csv"
  336. "Callback" 220 0.075978 220 0
  337. "chol_model_11" 10 565.176 10 572.8695
  338. "chol_model_21" 45 9184.828 45 9170.719
  339. "chol_model_22" 165 64712.07 165 64299.203
  340. $ starpu_paje_state_stats native.trace simgrid.trace
  341. \endverbatim
  342. An other way to get statistics of StarPU states (without installing <c>R</c> and
  343. <c>pj_dump</c>) is to use the <c>starpu_trace_state_stats.py</c> script which parses the
  344. generated <c>trace.rec</c> file instead of the <c>paje.trace</c> file. The output is similar
  345. to the previous script but it doesn't need any dependencies.
  346. The different prefixes used in <c>trace.rec</c> are:
  347. \verbatim
  348. E: Event type
  349. N: Event name
  350. C: Event category
  351. W: Worker ID
  352. T: Thread ID
  353. S: Start time
  354. \endverbatim
  355. Here's an example on how to use it:
  356. \verbatim
  357. $ python starpu_trace_state_stats.py trace.rec | column -t -s ","
  358. "Name" "Count" "Type" "Duration"
  359. "Callback" 220 Runtime 0.075978
  360. "chol_model_11" 10 Task 565.176
  361. "chol_model_21" 45 Task 9184.828
  362. "chol_model_22" 165 Task 64712.07
  363. \endverbatim
  364. <c>starpu_trace_state_stats.py</c> can also be used to compute the different
  365. efficiencies. Refer to the usage description to show some examples.
  366. And one can plot histograms of execution times, of several states for instance:
  367. \verbatim
  368. $ starpu_paje_draw_histogram -n chol_model_11,chol_model_21,chol_model_22 native.trace simgrid.trace
  369. \endverbatim
  370. and see the resulting pdf file:
  371. \image html paje_draw_histogram.png
  372. \image latex paje_draw_histogram.eps "" width=\textwidth
  373. A quick statistical report can be generated by using:
  374. \verbatim
  375. $ starpu_paje_summary native.trace simgrid.trace
  376. \endverbatim
  377. it includes gantt charts, execution summaries, as well as state duration charts
  378. and time distribution histograms.
  379. Other external Paje analysis tools can be used on these traces, one just needs
  380. to sort the traces by timestamp order (which not guaranteed to make recording
  381. more efficient):
  382. \verbatim
  383. $ starpu_paje_sort paje.trace
  384. \endverbatim
  385. \section TheoreticalLowerBoundOnExecutionTime Theoretical Lower Bound On Execution Time
  386. StarPU can record a trace of what tasks are needed to complete the
  387. application, and then, by using a linear system, provide a theoretical lower
  388. bound of the execution time (i.e. with an ideal scheduling).
  389. The computed bound is not really correct when not taking into account
  390. dependencies, but for an application which have enough parallelism, it is very
  391. near to the bound computed with dependencies enabled (which takes a huge lot
  392. more time to compute), and thus provides a good-enough estimation of the ideal
  393. execution time.
  394. \ref TheoreticalLowerBoundOnExecutionTimeExample provides an example on how to
  395. use this.
  396. \section TheoreticalLowerBoundOnExecutionTimeExample Theoretical Lower Bound On Execution Time Example
  397. For kernels with history-based performance models (and provided that
  398. they are completely calibrated), StarPU can very easily provide a
  399. theoretical lower bound for the execution time of a whole set of
  400. tasks. See for instance <c>examples/lu/lu_example.c</c>: before
  401. submitting tasks, call the function starpu_bound_start(), and after
  402. complete execution, call starpu_bound_stop().
  403. starpu_bound_print_lp() or starpu_bound_print_mps() can then be used
  404. to output a Linear Programming problem corresponding to the schedule
  405. of your tasks. Run it through <c>lp_solve</c> or any other linear
  406. programming solver, and that will give you a lower bound for the total
  407. execution time of your tasks. If StarPU was compiled with the library
  408. <c>glpk</c> installed, starpu_bound_compute() can be used to solve it
  409. immediately and get the optimized minimum, in ms. Its parameter
  410. <c>integer</c> allows to decide whether integer resolution should be
  411. computed and returned
  412. The <c>deps</c> parameter tells StarPU whether to take tasks, implicit
  413. data, and tag dependencies into account. Tags released in a callback
  414. or similar are not taken into account, only tags associated with a task are.
  415. It must be understood that the linear programming
  416. problem size is quadratic with the number of tasks and thus the time to solve it
  417. will be very long, it could be minutes for just a few dozen tasks. You should
  418. probably use <c>lp_solve -timeout 1 test.pl -wmps test.mps</c> to convert the
  419. problem to MPS format and then use a better solver, <c>glpsol</c> might be
  420. better than <c>lp_solve</c> for instance (the <c>--pcost</c> option may be
  421. useful), but sometimes doesn't manage to converge. <c>cbc</c> might look
  422. slower, but it is parallel. For <c>lp_solve</c>, be sure to try at least all the
  423. <c>-B</c> options. For instance, we often just use <c>lp_solve -cc -B1 -Bb
  424. -Bg -Bp -Bf -Br -BG -Bd -Bs -BB -Bo -Bc -Bi</c> , and the <c>-gr</c> option can
  425. also be quite useful. The resulting schedule can be observed by using
  426. the tool <c>starpu_lp2paje</c>, which converts it into the Paje
  427. format.
  428. Data transfer time can only be taken into account when <c>deps</c> is set. Only
  429. data transfers inferred from implicit data dependencies between tasks are taken
  430. into account. Other data transfers are assumed to be completely overlapped.
  431. Setting <c>deps</c> to 0 will only take into account the actual computations
  432. on processing units. It however still properly takes into account the varying
  433. performances of kernels and processing units, which is quite more accurate than
  434. just comparing StarPU performances with the fastest of the kernels being used.
  435. The <c>prio</c> parameter tells StarPU whether to simulate taking into account
  436. the priorities as the StarPU scheduler would, i.e. schedule prioritized
  437. tasks before less prioritized tasks, to check to which extend this results
  438. to a less optimal solution. This increases even more computation time.
  439. \section MemoryFeedback Memory Feedback
  440. It is possible to enable memory statistics. To do so, you need to pass
  441. the option \ref enable-memory-stats "--enable-memory-stats" when running <c>configure</c>. It is then
  442. possible to call the function starpu_data_display_memory_stats() to
  443. display statistics about the current data handles registered within StarPU.
  444. Moreover, statistics will be displayed at the end of the execution on
  445. data handles which have not been cleared out. This can be disabled by
  446. setting the environment variable \ref STARPU_MEMORY_STATS to <c>0</c>.
  447. For example, if you do not unregister data at the end of the complex
  448. example, you will get something similar to:
  449. \verbatim
  450. $ STARPU_MEMORY_STATS=0 ./examples/interface/complex
  451. Complex[0] = 45.00 + 12.00 i
  452. Complex[0] = 78.00 + 78.00 i
  453. Complex[0] = 45.00 + 12.00 i
  454. Complex[0] = 45.00 + 12.00 i
  455. \endverbatim
  456. \verbatim
  457. $ STARPU_MEMORY_STATS=1 ./examples/interface/complex
  458. Complex[0] = 45.00 + 12.00 i
  459. Complex[0] = 78.00 + 78.00 i
  460. Complex[0] = 45.00 + 12.00 i
  461. Complex[0] = 45.00 + 12.00 i
  462. #---------------------
  463. Memory stats:
  464. #-------
  465. Data on Node #3
  466. #-----
  467. Data : 0x553ff40
  468. Size : 16
  469. #--
  470. Data access stats
  471. /!\ Work Underway
  472. Node #0
  473. Direct access : 4
  474. Loaded (Owner) : 0
  475. Loaded (Shared) : 0
  476. Invalidated (was Owner) : 0
  477. Node #3
  478. Direct access : 0
  479. Loaded (Owner) : 0
  480. Loaded (Shared) : 1
  481. Invalidated (was Owner) : 0
  482. #-----
  483. Data : 0x5544710
  484. Size : 16
  485. #--
  486. Data access stats
  487. /!\ Work Underway
  488. Node #0
  489. Direct access : 2
  490. Loaded (Owner) : 0
  491. Loaded (Shared) : 1
  492. Invalidated (was Owner) : 1
  493. Node #3
  494. Direct access : 0
  495. Loaded (Owner) : 1
  496. Loaded (Shared) : 0
  497. Invalidated (was Owner) : 0
  498. \endverbatim
  499. \section DataStatistics Data Statistics
  500. Different data statistics can be displayed at the end of the execution
  501. of the application. To enable them, you need to define the environment
  502. variable \ref STARPU_ENABLE_STATS. When calling
  503. starpu_shutdown() various statistics will be displayed,
  504. execution, MSI cache statistics, allocation cache statistics, and data
  505. transfer statistics. The display can be disabled by setting the
  506. environment variable \ref STARPU_STATS to <c>0</c>.
  507. \verbatim
  508. $ ./examples/cholesky/cholesky_tag
  509. Computation took (in ms)
  510. 518.16
  511. Synthetic GFlops : 44.21
  512. #---------------------
  513. MSI cache stats :
  514. TOTAL MSI stats hit 1622 (66.23 %) miss 827 (33.77 %)
  515. ...
  516. \endverbatim
  517. \verbatim
  518. $ STARPU_STATS=0 ./examples/cholesky/cholesky_tag
  519. Computation took (in ms)
  520. 518.16
  521. Synthetic GFlops : 44.21
  522. \endverbatim
  523. // TODO: data transfer stats are similar to the ones displayed when
  524. // setting STARPU_BUS_STATS
  525. */