[yt-dev] Good benchmark?
Britton Smith
brittonsmith at gmail.com
Mon Mar 4 10:02:44 PST 2013
The halo profiling script in the cookbook should work fine. The only thing
I would change is the halo finding to work with the ParallelHop or
something else configured for larger datasets.
On Fri, Mar 1, 2013 at 4:34 PM, Matthew Turk <matthewturk at gmail.com> wrote:
> That sounds great. I have the Santa Fe Light Cone. I think focusing
> on Enzo data (since FLASH data in 2.x has poor performance) would be
> best for now.
>
> Would you be able to provide a relatively simple, but compute-heavy,
> halo profiling script? Would the cookbook one work pretty well for
> this? I can handle the other aspects.
>
> On Fri, Mar 1, 2013 at 3:48 PM, Britton Smith <brittonsmith at gmail.com>
> wrote:
> > If we do want to go with some big datasets, I can provide some 1024^3 and
> > 1536^3 unigrids. I'm sure others have better AMR data than I do.
> >
> >
> > On Fri, Mar 1, 2013 at 3:41 PM, Matthew Turk <matthewturk at gmail.com>
> wrote:
> >>
> >> Hey Sam,
> >>
> >> On Fri, Mar 1, 2013 at 2:38 PM, Sam Skillman <samskillman at gmail.com>
> >> wrote:
> >> > I think in terms of providing a test for the cluster, the benchmark
> >> > should
> >> > not require the shipment of data. For the benchmarking of yt for yt's
> >> > own
> >> > sake, then we do need to test the IO performance.
> >>
> >> I'm not really sure that we want to avoid IO...
> >>
> >> >
> >> > I think it'd be great to make an in-memory dataset that can then be
> used
> >> > for
> >> > testing performance. For example, set up a bunch of refined spheres
> and
> >> > then project/slice/profile/render/halo find?
> >>
> >> Perhaps, but will our current IC generators work at really, really big
> >> scale? I didn't think they would. Plus it's hard to get them to
> >> subdivide -- you end up with ltos of nested grids.
> >>
> >> >
> >> > Sam
> >> >
> >> >
> >> > On Fri, Mar 1, 2013 at 12:31 PM, Matthew Turk <matthewturk at gmail.com>
> >> > wrote:
> >> >>
> >> >> Hi Jeff,
> >> >>
> >> >> Sure. I got asked for a standard yt performance benchmark to be run
> >> >> to figure out performance of an analysis cluster and evaluate its
> >> >> readiness. :) I think it's safe to sya that we should be pushing
> >> >> things like IO, memory capacity and communication performance.
> >> >>
> >> >> Adding such a set of scripts (and their results!) would be very
> useful
> >> >> going forward, along with a little description of why we chose the
> >> >> routines we did.
> >> >>
> >> >> -Matt
> >> >>
> >> >> On Fri, Mar 1, 2013 at 2:17 PM, j s oishi <jsoishi at gmail.com> wrote:
> >> >> > Matt,
> >> >> >
> >> >> > It might be helpful if you shared some more details of this
> >> >> > particular
> >> >> > benchmarking exercise, if you can. It would be helpful for making
> >> >> > sure
> >> >> > we present the most usefil information to the people asking for it
> as
> >> >> > well as info that is useful to us going forwards.
> >> >> >
> >> >> > j
> >> >> >
> >> >> > On Fri, Mar 1, 2013 at 2:05 PM, Matthew Turk <
> matthewturk at gmail.com>
> >> >> > wrote:
> >> >> >> Definitely, yes. For what it's worth, the specific use case I
> have
> >> >> >> in
> >> >> >> mind is for performance testing a system, so I think scalability
> >> >> >> will
> >> >> >> be important.
> >> >> >>
> >> >> >> On Fri, Mar 1, 2013 at 2:01 PM, Cameron Hummels <
> chummels at gmail.com>
> >> >> >> wrote:
> >> >> >>> It might be worth showing how well this works on a single proc as
> >> >> >>> well
> >> >> >>> as
> >> >> >>> how well it works using parallel mode on a few different numbers
> of
> >> >> >>> processors.
> >> >> >>>
> >> >> >>>
> >> >> >>> On Fri, Mar 1, 2013 at 1:57 PM, Christopher Moody
> >> >> >>> <chrisemoody at gmail.com>
> >> >> >>> wrote:
> >> >> >>>>
> >> >> >>>> Perhaps a benchmark for simply calculating a derived field? This
> >> >> >>>> would
> >> >> >>>> then profile a much smaller codebase.
> >> >> >>>>
> >> >> >>>> Also benchmarking projections/fields for AMR/octree/particles of
> >> >> >>>> similar
> >> >> >>>> resolutions would be pretty cool.
> >> >> >>>>
> >> >> >>>> chris
> >> >> >>>>
> >> >> >>>>
> >> >> >>>> On Fri, Mar 1, 2013 at 10:53 AM, Matthew Turk
> >> >> >>>> <matthewturk at gmail.com>
> >> >> >>>> wrote:
> >> >> >>>>>
> >> >> >>>>> Okay, I like that idea. So a unified script with timing for in
> >> >> >>>>> each
> >> >> >>>>> section might include:
> >> >> >>>>>
> >> >> >>>>> * Halo profiling
> >> >> >>>>> * Global projection
> >> >> >>>>> * Global profiles
> >> >> >>>>> * Global VR (CTF and OffAxisProj)
> >> >> >>>>>
> >> >> >>>>> I think we probably want a large unigrid and a large AMR
> dataset
> >> >> >>>>> to
> >> >> >>>>> run these on, too.
> >> >> >>>>>
> >> >> >>>>> On Fri, Mar 1, 2013 at 1:50 PM, Nathan Goldbaum
> >> >> >>>>> <goldbaum at ucolick.org>
> >> >> >>>>> wrote:
> >> >> >>>>> > Probably a good idea to try some off axis projections or
> simple
> >> >> >>>>> > volume
> >> >> >>>>> > renderings to test the VR code.
> >> >> >>>>> >
> >> >> >>>>> >
> >> >> >>>>> > On Fri, Mar 1, 2013 at 10:48 AM, Matthew Turk
> >> >> >>>>> > <matthewturk at gmail.com>
> >> >> >>>>> > wrote:
> >> >> >>>>> >>
> >> >> >>>>> >> Hi all,
> >> >> >>>>> >>
> >> >> >>>>> >> I got an email asking for a benchmark of yt. I think this
> is
> >> >> >>>>> >> very,
> >> >> >>>>> >> very valuable to have going forward. I was wondering if
> >> >> >>>>> >> anyone
> >> >> >>>>> >> had
> >> >> >>>>> >> any suggestions?
> >> >> >>>>> >>
> >> >> >>>>> >> I'm thinking that we probably want to test things like the
> >> >> >>>>> >> halo
> >> >> >>>>> >> finder, projections, and phase plots. Would a medium
> (1536^3)
> >> >> >>>>> >> halo
> >> >> >>>>> >> profiling run do that? Do we want to add on some global
> >> >> >>>>> >> projections
> >> >> >>>>> >> and phase plots as well?
> >> >> >>>>> >>
> >> >> >>>>> >> -Matt
> >> >> >>>>> >> _______________________________________________
> >> >> >>>>> >> yt-dev mailing list
> >> >> >>>>> >> yt-dev at lists.spacepope.org
> >> >> >>>>> >>
> http://lists.spacepope.org/listinfo.cgi/yt-dev-spacepope.org
> >> >> >>>>> >
> >> >> >>>>> >
> >> >> >>>>> >
> >> >> >>>>> > _______________________________________________
> >> >> >>>>> > yt-dev mailing list
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> >> >> >>>>> > http://lists.spacepope.org/listinfo.cgi/yt-dev-spacepope.org
> >> >> >>>>> >
> >> >> >>>>> _______________________________________________
> >> >> >>>>> yt-dev mailing list
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> >> >> >>>>
> >> >> >>>>
> >> >> >>>>
> >> >> >>>> _______________________________________________
> >> >> >>>> yt-dev mailing list
> >> >> >>>> yt-dev at lists.spacepope.org
> >> >> >>>> http://lists.spacepope.org/listinfo.cgi/yt-dev-spacepope.org
> >> >> >>>>
> >> >> >>>
> >> >> >>>
> >> >> >>>
> >> >> >>> --
> >> >> >>> Cameron Hummels
> >> >> >>> Postdoctoral Researcher
> >> >> >>> Steward Observatory
> >> >> >>> University of Arizona
> >> >> >>> http://chummels.org
> >> >> >>>
> >> >> >>> _______________________________________________
> >> >> >>> yt-dev mailing list
> >> >> >>> yt-dev at lists.spacepope.org
> >> >> >>> http://lists.spacepope.org/listinfo.cgi/yt-dev-spacepope.org
> >> >> >>>
> >> >> >> _______________________________________________
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> >> >> > _______________________________________________
> >> >> > yt-dev mailing list
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> >> >> _______________________________________________
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> >> >
> >> >
> >> >
> >> > _______________________________________________
> >> > yt-dev mailing list
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> >> >
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> >
> >
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