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. One can also introduce user-defined events in the diagram thanks to the
  101. starpu_fxt_trace_user_event_string() function.
  102. In the MPI execution case, \ref STARPU_GENERATE_TRACE will not work as expected
  103. (each node will try to generate paje.trace, thus mixing outputs...), you have to
  104. collect the trace files from the MPI nodes, and
  105. specify them all on the command <c>starpu_fxt_tool</c>, for instance:
  106. \verbatim
  107. $ starpu_fxt_tool -i /tmp/prof_file_something*
  108. \endverbatim
  109. By default, all tasks are displayed using a green color. To display tasks with
  110. varying colors, pass option <c>-c</c> to <c>starpu_fxt_tool</c>.
  111. By default, the trace contains all informations. To reduce the trace size,
  112. various <c>-no-foo</c> options can be passed to <c>starpu_fxt_tool</c>, see
  113. <c>starpu_fxt_tool --help</c> .
  114. To identify tasks precisely, the application can set the starpu_task::tag_id field of the
  115. task (or use \ref STARPU_TAG_ONLY when using starpu_task_insert()), and
  116. the value of the tag will show up in the trace.
  117. It can also set the starpu_task::name field of the task (or use \ref STARPU_NAME)
  118. when using starpu_task_insert()), to replace in traces the name of the codelet
  119. with an arbitrarily chosen name.
  120. It can also set the iteration number, by just calling starpu_iteration_push()
  121. at the beginning of submission loops and starpu_iteration_pop() at the end of
  122. submission loops. These iteration numbers will show up in traces for all tasks
  123. submitted from there.
  124. Coordinates can also be given to data with the starpu_data_set_coordinates() or
  125. starpu_data_set_coordinates_array() function. In the trace, tasks will then be
  126. assigned the coordinates of the first data they write to.
  127. Traces can also be inspected by hand by using the tool <c>fxt_print</c>, for instance:
  128. \verbatim
  129. $ fxt_print -o -f /tmp/prof_file_something
  130. \endverbatim
  131. Timings are in nanoseconds (while timings as seen in ViTE are in milliseconds).
  132. \subsection CreatingADAGWithGraphviz Creating a DAG With Graphviz
  133. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  134. generate a task graph in the DOT format by calling:
  135. \verbatim
  136. $ starpu_fxt_tool -i /tmp/prof_file_something
  137. \endverbatim
  138. This will create a <c>dag.dot</c> file in the current directory. This file is a
  139. task graph described using the DOT language. It is possible to get a
  140. graphical output of the graph by using the graphviz library:
  141. \verbatim
  142. $ dot -Tpdf dag.dot -o output.pdf
  143. \endverbatim
  144. \subsection TraceTaskDetails Getting Task Details
  145. When the FxT trace file <c>prof_file_something</c> has been generated, details on the
  146. executed tasks can be retrieved by calling:
  147. \verbatim
  148. $ starpu_fxt_tool -i /tmp/prof_file_something
  149. \endverbatim
  150. This will create a <c>tasks.rec</c> file in the current directory. This file
  151. is in the recutils format, i.e. <c>Field: value</c> lines, and empty lines to
  152. separate each task. This can be used as a convenient input for various ad-hoc
  153. analysis tools. By default it only contains information about the actual
  154. execution. Performance models can be obtained by running
  155. <c>starpu_tasks_rec_complete</c> on it:
  156. \verbatim
  157. $ starpu_tasks_rec_complete tasks.rec tasks2.rec
  158. \endverbatim
  159. which will add <c>EstimatedTime</c> lines which contain the performance
  160. model-estimated time (in µs) for each worker starting from 0. Since it needs
  161. the performance models, it needs to be run the same way as the application
  162. execution, or at least with <c>STARPU_HOSTNAME</c> set to the hostname of the
  163. machine used for execution, to get the performance models of that machine.
  164. \subsection MonitoringActivity Monitoring Activity
  165. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  166. generate an activity trace by calling:
  167. \verbatim
  168. $ starpu_fxt_tool -i /tmp/prof_file_something
  169. \endverbatim
  170. This will create a file <c>activity.data</c> in the current
  171. directory. A profile of the application showing the activity of StarPU
  172. during the execution of the program can be generated:
  173. \verbatim
  174. $ starpu_workers_activity activity.data
  175. \endverbatim
  176. This will create a file named <c>activity.eps</c> in the current directory.
  177. This picture is composed of two parts.
  178. The first part shows the activity of the different workers. The green sections
  179. indicate which proportion of the time was spent executed kernels on the
  180. processing unit. The red sections indicate the proportion of time spent in
  181. StartPU: an important overhead may indicate that the granularity may be too
  182. low, and that bigger tasks may be appropriate to use the processing unit more
  183. efficiently. The black sections indicate that the processing unit was blocked
  184. because there was no task to process: this may indicate a lack of parallelism
  185. which may be alleviated by creating more tasks when it is possible.
  186. The second part of the picture <c>activity.eps</c> is a graph showing the
  187. evolution of the number of tasks available in the system during the execution.
  188. Ready tasks are shown in black, and tasks that are submitted but not
  189. schedulable yet are shown in grey.
  190. \subsection Animation Getting Modular Schedular Animation
  191. When using modular schedulers (i.e. schedulers which use a modular architecture,
  192. and whose name start with "modular-"), the command
  193. \verbatim
  194. $ starpu_fxt_tool -i /tmp/prof_file_something
  195. \endverbatim
  196. will also produce a <c>trace.html</c> file which can be viewed in a
  197. javascript-enabled web browser. It shows the flow of tasks between the
  198. components of the modular scheduler.
  199. \subsection LimitingScopeTrace Limiting The Scope Of The Trace
  200. For computing statistics, it is useful to limit the trace to a given portion of
  201. the time of the whole execution. This can be achieved by calling
  202. \code{.c}
  203. starpu_fxt_autostart_profiling(0)
  204. \endcode
  205. before calling starpu_init(), to
  206. prevent tracing from starting immediately. Then
  207. \code{.c}
  208. starpu_fxt_start_profiling();
  209. \endcode
  210. and
  211. \code{.c}
  212. starpu_fxt_stop_profiling();
  213. \endcode
  214. can be used around the portion of code to be traced. This will show up as marks
  215. in the trace, and states of workers will only show up for that portion.
  216. \section PerformanceOfCodelets Performance Of Codelets
  217. The performance model of codelets (see \ref PerformanceModelExample)
  218. can be examined by using the tool <c>starpu_perfmodel_display</c>:
  219. \verbatim
  220. $ starpu_perfmodel_display -l
  221. file: <malloc_pinned.hannibal>
  222. file: <starpu_slu_lu_model_21.hannibal>
  223. file: <starpu_slu_lu_model_11.hannibal>
  224. file: <starpu_slu_lu_model_22.hannibal>
  225. file: <starpu_slu_lu_model_12.hannibal>
  226. \endverbatim
  227. Here, the codelets of the example <c>lu</c> are available. We can examine the
  228. performance of the kernel <c>22</c> (in micro-seconds), which is history-based:
  229. \verbatim
  230. $ starpu_perfmodel_display -s starpu_slu_lu_model_22
  231. performance model for cpu
  232. # hash size mean dev n
  233. 57618ab0 19660800 2.851069e+05 1.829369e+04 109
  234. performance model for cuda_0
  235. # hash size mean dev n
  236. 57618ab0 19660800 1.164144e+04 1.556094e+01 315
  237. performance model for cuda_1
  238. # hash size mean dev n
  239. 57618ab0 19660800 1.164271e+04 1.330628e+01 360
  240. performance model for cuda_2
  241. # hash size mean dev n
  242. 57618ab0 19660800 1.166730e+04 3.390395e+02 456
  243. \endverbatim
  244. We can see that for the given size, over a sample of a few hundreds of
  245. execution, the GPUs are about 20 times faster than the CPUs (numbers are in
  246. us). The standard deviation is extremely low for the GPUs, and less than 10% for
  247. CPUs.
  248. This tool can also be used for regression-based performance models. It will then
  249. display the regression formula, and in the case of non-linear regression, the
  250. same performance log as for history-based performance models:
  251. \verbatim
  252. $ starpu_perfmodel_display -s non_linear_memset_regression_based
  253. performance model for cpu_impl_0
  254. Regression : #sample = 1400
  255. Linear: y = alpha size ^ beta
  256. alpha = 1.335973e-03
  257. beta = 8.024020e-01
  258. Non-Linear: y = a size ^b + c
  259. a = 5.429195e-04
  260. b = 8.654899e-01
  261. c = 9.009313e-01
  262. # hash size mean stddev n
  263. a3d3725e 4096 4.763200e+00 7.650928e-01 100
  264. 870a30aa 8192 1.827970e+00 2.037181e-01 100
  265. 48e988e9 16384 2.652800e+00 1.876459e-01 100
  266. 961e65d2 32768 4.255530e+00 3.518025e-01 100
  267. ...
  268. \endverbatim
  269. The same can also be achieved by using StarPU's library API, see
  270. \ref API_Performance_Model and notably the function
  271. starpu_perfmodel_load_symbol(). The source code of the tool
  272. <c>starpu_perfmodel_display</c> can be a useful example.
  273. The tool <c>starpu_perfmodel_plot</c> can be used to draw performance
  274. models. It writes a <c>.gp</c> file in the current directory, to be
  275. run with the tool <c>gnuplot</c>, which shows the corresponding curve.
  276. \image html starpu_non_linear_memset_regression_based.png
  277. \image latex starpu_non_linear_memset_regression_based.eps "" width=\textwidth
  278. When the field starpu_task::flops is set (or \ref STARPU_FLOPS is passed to
  279. starpu_task_insert()), <c>starpu_perfmodel_plot</c> can directly draw a GFlops
  280. curve, by simply adding the <c>-f</c> option:
  281. \verbatim
  282. $ starpu_perfmodel_plot -f -s chol_model_11
  283. \endverbatim
  284. This will however disable displaying the regression model, for which we can not
  285. compute GFlops.
  286. \image html starpu_chol_model_11_type.png
  287. \image latex starpu_chol_model_11_type.eps "" width=\textwidth
  288. When the FxT trace file <c>prof_file_something</c> has been generated, it is possible to
  289. get a profiling of each codelet by calling:
  290. \verbatim
  291. $ starpu_fxt_tool -i /tmp/prof_file_something
  292. $ starpu_codelet_profile distrib.data codelet_name
  293. \endverbatim
  294. This will create profiling data files, and a <c>distrib.data.gp</c> file in the current
  295. directory, which draws the distribution of codelet time over the application
  296. execution, according to data input size.
  297. \image html distrib_data.png
  298. \image latex distrib_data.eps "" width=\textwidth
  299. This is also available in the tool <c>starpu_perfmodel_plot</c>, by passing it
  300. the fxt trace:
  301. \verbatim
  302. $ starpu_perfmodel_plot -s non_linear_memset_regression_based -i /tmp/prof_file_foo_0
  303. \endverbatim
  304. It will produce a <c>.gp</c> file which contains both the performance model
  305. curves, and the profiling measurements.
  306. \image html starpu_non_linear_memset_regression_based_2.png
  307. \image latex starpu_non_linear_memset_regression_based_2.eps "" width=\textwidth
  308. If you have the statistical tool <c>R</c> installed, you can additionally use
  309. \verbatim
  310. $ starpu_codelet_histo_profile distrib.data
  311. \endverbatim
  312. Which will create one <c>.pdf</c> file per codelet and per input size, showing a
  313. histogram of the codelet execution time distribution.
  314. \image html distrib_data_histo.png
  315. \image latex distrib_data_histo.eps "" width=\textwidth
  316. \section TraceStatistics Trace Statistics
  317. More than just codelet performance, it is interesting to get statistics over all
  318. kinds of StarPU states (allocations, data transfers, etc.). This is particularly
  319. useful to check what may have gone wrong in the accurracy of the simgrid
  320. simulation.
  321. This requires the <c>R</c> statistical tool, with the <c>plyr</c>,
  322. <c>ggplot2</c> and <c>data.table</c> packages. If your system
  323. distribution does not have packages for these, one can fetch them from
  324. <c>CRAN</c>:
  325. \verbatim
  326. $ R
  327. > install.packages("plyr")
  328. > install.packages("ggplot2")
  329. > install.packages("data.table")
  330. > install.packages("knitr")
  331. \endverbatim
  332. The <c>pj_dump</c> tool from <c>pajeng</c> is also needed (see
  333. https://github.com/schnorr/pajeng)
  334. One can then get textual or <c>.csv</c> statistics over the trace states:
  335. \verbatim
  336. $ starpu_paje_state_stats -v native.trace simgrid.trace
  337. "Value" "Events_native.csv" "Duration_native.csv" "Events_simgrid.csv" "Duration_simgrid.csv"
  338. "Callback" 220 0.075978 220 0
  339. "chol_model_11" 10 565.176 10 572.8695
  340. "chol_model_21" 45 9184.828 45 9170.719
  341. "chol_model_22" 165 64712.07 165 64299.203
  342. $ starpu_paje_state_stats native.trace simgrid.trace
  343. \endverbatim
  344. An other way to get statistics of StarPU states (without installing <c>R</c> and
  345. <c>pj_dump</c>) is to use the <c>starpu_trace_state_stats.py</c> script which parses the
  346. generated <c>trace.rec</c> file instead of the <c>paje.trace</c> file. The output is similar
  347. to the previous script but it doesn't need any dependencies.
  348. The different prefixes used in <c>trace.rec</c> are:
  349. \verbatim
  350. E: Event type
  351. N: Event name
  352. C: Event category
  353. W: Worker ID
  354. T: Thread ID
  355. S: Start time
  356. \endverbatim
  357. Here's an example on how to use it:
  358. \verbatim
  359. $ python starpu_trace_state_stats.py trace.rec | column -t -s ","
  360. "Name" "Count" "Type" "Duration"
  361. "Callback" 220 Runtime 0.075978
  362. "chol_model_11" 10 Task 565.176
  363. "chol_model_21" 45 Task 9184.828
  364. "chol_model_22" 165 Task 64712.07
  365. \endverbatim
  366. <c>starpu_trace_state_stats.py</c> can also be used to compute the different
  367. efficiencies. Refer to the usage description to show some examples.
  368. And one can plot histograms of execution times, of several states for instance:
  369. \verbatim
  370. $ starpu_paje_draw_histogram -n chol_model_11,chol_model_21,chol_model_22 native.trace simgrid.trace
  371. \endverbatim
  372. and see the resulting pdf file:
  373. \image html paje_draw_histogram.png
  374. \image latex paje_draw_histogram.eps "" width=\textwidth
  375. A quick statistical report can be generated by using:
  376. \verbatim
  377. $ starpu_paje_summary native.trace simgrid.trace
  378. \endverbatim
  379. it includes gantt charts, execution summaries, as well as state duration charts
  380. and time distribution histograms.
  381. Other external Paje analysis tools can be used on these traces, one just needs
  382. to sort the traces by timestamp order (which not guaranteed to make recording
  383. more efficient):
  384. \verbatim
  385. $ starpu_paje_sort paje.trace
  386. \endverbatim
  387. \section TheoreticalLowerBoundOnExecutionTime Theoretical Lower Bound On Execution Time
  388. StarPU can record a trace of what tasks are needed to complete the
  389. application, and then, by using a linear system, provide a theoretical lower
  390. bound of the execution time (i.e. with an ideal scheduling).
  391. The computed bound is not really correct when not taking into account
  392. dependencies, but for an application which have enough parallelism, it is very
  393. near to the bound computed with dependencies enabled (which takes a huge lot
  394. more time to compute), and thus provides a good-enough estimation of the ideal
  395. execution time.
  396. \ref TheoreticalLowerBoundOnExecutionTimeExample provides an example on how to
  397. use this.
  398. \section TheoreticalLowerBoundOnExecutionTimeExample Theoretical Lower Bound On Execution Time Example
  399. For kernels with history-based performance models (and provided that
  400. they are completely calibrated), StarPU can very easily provide a
  401. theoretical lower bound for the execution time of a whole set of
  402. tasks. See for instance <c>examples/lu/lu_example.c</c>: before
  403. submitting tasks, call the function starpu_bound_start(), and after
  404. complete execution, call starpu_bound_stop().
  405. starpu_bound_print_lp() or starpu_bound_print_mps() can then be used
  406. to output a Linear Programming problem corresponding to the schedule
  407. of your tasks. Run it through <c>lp_solve</c> or any other linear
  408. programming solver, and that will give you a lower bound for the total
  409. execution time of your tasks. If StarPU was compiled with the library
  410. <c>glpk</c> installed, starpu_bound_compute() can be used to solve it
  411. immediately and get the optimized minimum, in ms. Its parameter
  412. <c>integer</c> allows to decide whether integer resolution should be
  413. computed and returned
  414. The <c>deps</c> parameter tells StarPU whether to take tasks, implicit
  415. data, and tag dependencies into account. Tags released in a callback
  416. or similar are not taken into account, only tags associated with a task are.
  417. It must be understood that the linear programming
  418. problem size is quadratic with the number of tasks and thus the time to solve it
  419. will be very long, it could be minutes for just a few dozen tasks. You should
  420. probably use <c>lp_solve -timeout 1 test.pl -wmps test.mps</c> to convert the
  421. problem to MPS format and then use a better solver, <c>glpsol</c> might be
  422. better than <c>lp_solve</c> for instance (the <c>--pcost</c> option may be
  423. useful), but sometimes doesn't manage to converge. <c>cbc</c> might look
  424. slower, but it is parallel. For <c>lp_solve</c>, be sure to try at least all the
  425. <c>-B</c> options. For instance, we often just use <c>lp_solve -cc -B1 -Bb
  426. -Bg -Bp -Bf -Br -BG -Bd -Bs -BB -Bo -Bc -Bi</c> , and the <c>-gr</c> option can
  427. also be quite useful. The resulting schedule can be observed by using
  428. the tool <c>starpu_lp2paje</c>, which converts it into the Paje
  429. format.
  430. Data transfer time can only be taken into account when <c>deps</c> is set. Only
  431. data transfers inferred from implicit data dependencies between tasks are taken
  432. into account. Other data transfers are assumed to be completely overlapped.
  433. Setting <c>deps</c> to 0 will only take into account the actual computations
  434. on processing units. It however still properly takes into account the varying
  435. performances of kernels and processing units, which is quite more accurate than
  436. just comparing StarPU performances with the fastest of the kernels being used.
  437. The <c>prio</c> parameter tells StarPU whether to simulate taking into account
  438. the priorities as the StarPU scheduler would, i.e. schedule prioritized
  439. tasks before less prioritized tasks, to check to which extend this results
  440. to a less optimal solution. This increases even more computation time.
  441. \section MemoryFeedback Memory Feedback
  442. It is possible to enable memory statistics. To do so, you need to pass
  443. the option \ref enable-memory-stats "--enable-memory-stats" when running <c>configure</c>. It is then
  444. possible to call the function starpu_data_display_memory_stats() to
  445. display statistics about the current data handles registered within StarPU.
  446. Moreover, statistics will be displayed at the end of the execution on
  447. data handles which have not been cleared out. This can be disabled by
  448. setting the environment variable \ref STARPU_MEMORY_STATS to <c>0</c>.
  449. For example, if you do not unregister data at the end of the complex
  450. example, you will get something similar to:
  451. \verbatim
  452. $ STARPU_MEMORY_STATS=0 ./examples/interface/complex
  453. Complex[0] = 45.00 + 12.00 i
  454. Complex[0] = 78.00 + 78.00 i
  455. Complex[0] = 45.00 + 12.00 i
  456. Complex[0] = 45.00 + 12.00 i
  457. \endverbatim
  458. \verbatim
  459. $ STARPU_MEMORY_STATS=1 ./examples/interface/complex
  460. Complex[0] = 45.00 + 12.00 i
  461. Complex[0] = 78.00 + 78.00 i
  462. Complex[0] = 45.00 + 12.00 i
  463. Complex[0] = 45.00 + 12.00 i
  464. #---------------------
  465. Memory stats:
  466. #-------
  467. Data on Node #3
  468. #-----
  469. Data : 0x553ff40
  470. Size : 16
  471. #--
  472. Data access stats
  473. /!\ Work Underway
  474. Node #0
  475. Direct access : 4
  476. Loaded (Owner) : 0
  477. Loaded (Shared) : 0
  478. Invalidated (was Owner) : 0
  479. Node #3
  480. Direct access : 0
  481. Loaded (Owner) : 0
  482. Loaded (Shared) : 1
  483. Invalidated (was Owner) : 0
  484. #-----
  485. Data : 0x5544710
  486. Size : 16
  487. #--
  488. Data access stats
  489. /!\ Work Underway
  490. Node #0
  491. Direct access : 2
  492. Loaded (Owner) : 0
  493. Loaded (Shared) : 1
  494. Invalidated (was Owner) : 1
  495. Node #3
  496. Direct access : 0
  497. Loaded (Owner) : 1
  498. Loaded (Shared) : 0
  499. Invalidated (was Owner) : 0
  500. \endverbatim
  501. \section DataStatistics Data Statistics
  502. Different data statistics can be displayed at the end of the execution
  503. of the application. To enable them, you need to define the environment
  504. variable \ref STARPU_ENABLE_STATS. When calling
  505. starpu_shutdown() various statistics will be displayed,
  506. execution, MSI cache statistics, allocation cache statistics, and data
  507. transfer statistics. The display can be disabled by setting the
  508. environment variable \ref STARPU_STATS to <c>0</c>.
  509. \verbatim
  510. $ ./examples/cholesky/cholesky_tag
  511. Computation took (in ms)
  512. 518.16
  513. Synthetic GFlops : 44.21
  514. #---------------------
  515. MSI cache stats :
  516. TOTAL MSI stats hit 1622 (66.23 %) miss 827 (33.77 %)
  517. ...
  518. \endverbatim
  519. \verbatim
  520. $ STARPU_STATS=0 ./examples/cholesky/cholesky_tag
  521. Computation took (in ms)
  522. 518.16
  523. Synthetic GFlops : 44.21
  524. \endverbatim
  525. // TODO: data transfer stats are similar to the ones displayed when
  526. // setting STARPU_BUS_STATS
  527. */