Mailman 3 April 2010 - yt-dev

Quad Tree projections
by Matthew Turk May 14, 2010

May 14, 2010

Hi guys, On Monday I rewrote the (adaptive) projection backend to use Quad Trees for point placement instead of the current system. As it stands, the current system for projecting works pretty well, except for a couple caveats: - It has high peak memory usage - It can only be decomposed in the image plane, so inline projections can't be made, and load balancing AMR was poor - It's complicated, but that complication comes from wanting things to be fast Essentially, it's fast by wall-clock standards, but you need to run in parallel for big datasets. Plus, if you want to run with big datasets, you probably need to fully occupy nodes, because of the peak memory usage. Anyway, I was getting very frustrated with points #1 and #3 (but not #2, oddly) and so I wrote a new backend using Quad Trees. We did everything using int math anyway, but because joining grids was O(NxM), things got a bit slow in some domains. The conversion wasn't too bad. I ran some simple benchmarks. These were all conducted on the Triton resource, in serial, on a single node. They do not reflect time for disk IO, but they should roughly reflect real memory load. * For my 31 level PopIII binary star run (875 million cells, 8000 grids), it took 9 seconds with peak memory usage of 176 megs. * For a large, 768^3 with (peak) 12 levels of refinement (874 million cells in 125,000 grids), it takes 81 seconds with peak memory load of 840 megs. * For the 512^3 L7 lightcone run, at a time when the data had 300,000 grids, it took 170 seconds with peak memory usage of 2.5 gigs. In all cases, the results are correct according to the standard check of projecting "Ones". These are crazy improvements, especially considering that these are times for serial projections. And important note here is that this *will* parallelize independent of the image plane, although I have yet to see the need to parallelize just yet. The load balancing may be better optimized based on image plane decomposition, but the algorithm should work with independent joins. Additionally in parallel the final join at the end of the calculation may have higher peak memory usage if the decomposition is not via image plane decomposition, but it should still work. Unfortunately, right now my time is very constrained; so I am going to put out there that if someone would be willing to help me break apart the existing code and insert this code, then we can swap out the engines. But in the absence of that, I'm not sure that it'll get inserted into the main line before the Summer, or at least the late Spring. As is, I can definitely provide a very simple and manual interface to use it (and I intend to do so) but integrating it into the mainline is not going to be my priority right now. But, again, I will provide *an* interface, even if it's not a *final* interface and likely not a *nice* interface. Anyway, I'm pretty excited about this -- definitely a huge improvement over the previous algorithm, and we still retain the *adaptive* nature of the projections: project once, plot many. -Matt

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DualEPS extension
by John Wise April 30, 2010

April 30, 2010

Hi all, I just committed a new extension that can create EPS figures that have both compressed bitmaps and vector graphics. I've been wanting to do this for the past few years! I always hate making very high resolution figures for publication *just* to have the text sharp. This extension can make either a single panel or multi-panel panel with one call. Here are some examples, notice that their file sizes are similar to their JPEG file sizes. Single panel example and figures: http://paste.enzotools.org/show/485/ http://www.astro.princeton.edu/~jwise/DualEPS/example1.eps (56kB) http://www.astro.princeton.edu/~jwise/DualEPS/example1anno.eps (63kB) Multi-panel: http://paste.enzotools.org/show/486/ http://www.astro.princeton.edu/~jwise/DualEPS/example2.eps (142kB) It could use some refinements, but I've pretty pleased with its output! I hope this is useful to many of you. Cheers, John

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Remote data viewing
by Matthew Turk April 29, 2010

April 29, 2010

Hi all, I wrote a remote image viewer, so that you can interactively explore things like projections without having to copy *any* of the data locally. You can use it inside the Chaco-based explorer; all pixelization is done remotely and only pixelized buffers are sent back over the wire. I've stuck an example here: http://paste.enzotools.org/show/479/ but it'll be documented (along with the rest of the image panner stuff) in the 1.7 docs, specifically how to get the FURL info (~/.ipython/security/ipcontroller-mec.furl). Anyway, I'm finding it incredibly useful for exploring a huge amount of remote-living data. Hopefully somebody else will find it useful, too! -Matt

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error in new hg version of yt
by Eric Hallman April 29, 2010

April 29, 2010

I pulled the new hg version of yt today, when installing (on both ranger and my local mac) I get an error in the compile for _MPL.c in raven: error: Command "gcc -arch ppc -arch i386 -isysroot /Developer/SDKs/ MacOSX10.4u.sdk -fno-strict-aliasing -Wno-long-double -no-cpp-precomp - mno-fused-madd -fno-common -dynamic -DNDEBUG -g -O3 -I/Library/ Frameworks/Python.framework/Versions/2.5/lib/python2.5/site-packages/ numpy/core/include -I/Library/Frameworks/Python.framework/Versions/2.5/ include/python2.5 -c yt/raven/_MPL.c -o build/temp.macosx-10.3- i386-2.5/yt/raven/_MPL.o" failed with exit status 1 Dr. Eric J. Hallman NSF Astronomy and Astrophysics Postdoctoral Fellow Center for Astrophysics and Space Astronomy University of Colorado at Boulder hallman (at) casa.colorado.edu Phone: (312) 725-4626 http://solo.colorado.edu/~hallman/

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Quick note about mercurial 1.5
by Matthew Turk April 24, 2010

April 24, 2010

Hi all, Just a note: with mercurial 1.5, the meaning of "hg heads" has changed slightly -- it is no longer neutral to branch mechanics. This means that if a named branch has been merged, but not "closed", it will still show up in the default output of hg heads. For the most part I don't think this is really what we want, because nobody has been closing branches. So, if you use hg 1.5 right now on any repo with multiple named branches, you're going to see way more than you expected. To get around this, hg heads -t will only show revisions with no children *at all*, rather than the new default behavior, which was to show heads with no children *in that named branch*. You can alias this to "hg heads" by putting this in the [alias] section of your ~/.hgrc : heads = heads -t (Another fun alias is "nudge = push -r ." which will only push the necessary changesets to fully describe the current revision -- any other trees of development will not be included in the push. Useful for when doing local development with multiple heads!!) -Matt

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Volume Rendering branch
by Matthew Turk April 23, 2010

April 23, 2010

Hi guys, The vr-multivariate branch has been merged into the main yt-hg repository. I worked a little bit on speed today and for ColorTransferFunction it's now competitive. Additionally, I've added a Projection mechanism that should enable off-axis projections (this will be documented very soon.) The off-axis projections are pretty nice, I think -- the only hold up on that front is that I want to ensure that I understand the units. I've attached an example image, which was created by the volume renderer using this script: http://paste.enzotools.org/show/464/ note that we output directly to PNG here -- no matplotlib intervention at all! This is from data supplied by Cameron Hummels, which he was previously using a stacked cutting plane method to look at off-axis. I'm excited about the off-axis projections, because my protostars are rarely aligned with the grids -- so now off-axis projections of baryon quantities are going to become a part of my standard analysis. Again, the units need to be examined before this is finished, and I'll handle that shortly. Let me know if there are any issues. I'll probably port this back to trunk this weekend. By merging this branch we now have in the main hg repo: * Off-axis projections * Multivariate volume rendering * Planck transfer functions * Approximate Rayleigh scattering -Matt

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Multivariate Volume Rendering
by Matthew Turk April 16, 2010

April 16, 2010

Hi all, Over the last little while, the volume renderer has really taken off in popularity! I'm a bit conflicted about this, since I'd rather people were super duper into things like phase plots, radial profiles and clump finding, but it's also good to know people are using yt for volume visualization as well as other types of analysis. I used it myself to what I think was great effect at a conference last week, and I hope that other people are getting similar use out of it. Anyway, a couple months ago John wrote to yt-users and suggested that we try doing multivariate volume rendering, similar to what's in Kaehler, Wise, & Abel. For a while mostly nothing happened, but over the Friday->Sunday, Jeff and I hammered it out and it's now working. Jeff took care of the emission spectra (with some assistance from John's RGB code), I took a whack at adding multiple variables to the partitioned grids and the volume rendering itself, and we can now do multivariate rendering -- although absorption still needs some work, which I'll discuss below. The new mechanism for grid partitioning only returns the indices into the vertex-centered data. The actual processing of the vertex-centered data. This means the actual locating of sweeps is much faster -- right now we don't take advantage of that, but I can see it being useful in the future. A few weeks ago I wrote a distributed object collection so that we could do 3D domain decomp to get the bricks, then pass them around between processes for the actual volume rendering, which was parallelized via 2D image plane decomp into decomposed inclined boxes. Now the 3D decomp will only pass around single arrays that describe the indices into the bricks, and then each image-decomp processor will generate and slice up the data as necessary -- this isn't yet working, but it's a clear process and I'll try to take care of it soon. Transfer functions now have several more parameters, and I'm working to convert the old-style transfer functions to this. The idea is that now you add field interpolation tables which correspond to a specific field, link them to channels (R, Ralpha, G, Galpha, B, Balpha), and optionally have their values weighted by other fields. So for an example, here's how the Planck function sets up its various channels: http://hg.enzotools.org/yt/file/ede5d76cddd4/yt/extensions/volume_rendering… (there's a bit of cruft where I tested adding lines for density absorption.) It creates a TransferFunction, links it to a field (0) and a weighting field (2), then links it to channels. There's a lot of complexity in this, because it's a complex thing and we want to enable very complex behavior, but for the most part it will be hidden in the ColorTransferFunction, which will abstract this all away. Absorption works slightly differently now. Because we do back-to-front integration, I believe we do not have to store the accumulated opacity -- so while right now the volume renderer has 6xNxM arrays, I think it should just be 3. Additionally, we're presented with the radiative transfer equation: dI/ds = -alpha * I_0 + j Here j would be our emission at a given sample, I_0 is the current value of the image plane, and ds is the distance between samples. Since we're doing back-to-front, I believe we are directly solving this, and so our alpha fed in directly corresponds to the absorption. However, because ds is so low, careful calibration between alpha and emissivity is necessary. Alternately, converting everything back to cgs is probably not difficult... (approximate) Scattering should be easy to put in, it just hasn't been yet. However, that's neither here nor there. I believe that some exciting things can be done with this (Britton and Jeff and I have chatted about line transfer as well as LyA maps) and I think it's rapidly converging on a workable implementation. I made up some images with it. The first is a sample dataset of John's with an HII region: http://yt.enzotools.org/attachment/wiki/Screenshots/hiiregion_rgb.png The second is one of my protostars from my thesis (I had to aggressively clip the image here) just at around 1.5e4K. This image is 3AU on a side: http://yt.enzotools.org/attachment/wiki/Screenshots/protostar_rgb.png And, just for fun, I got the transfer function widget to steal the camera position from the VTK interface, so I made up an image of the two playing nicely together: http://yt.enzotools.org/attachment/wiki/Screenshots/vtk_tf_vr.png Anyway, that's my status update. All of the MultiVariate stuff went in the "vr-multivariate" branch, so feel free to take a look. (You'll probably have to re-cython.) An example script is here: http://paste.enzotools.org/show/367/ I'll shoot another, much shorter, email to the list when it's working and merged back into the main hg branch. We'll then have a parallel software volume renderer that is fully multi-channel, multi-variate, and comes with black body transfer functions. All of this is only achievable thanks to the development community we have, and our team efforts. So, thank you all for your hard work and your enthusiasm. -Matt

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Simple image writing
by Matthew Turk April 15, 2010

April 15, 2010

Hi guys, I wrote a new module (in branch yt of hg) that will do simple image writing; it only depends on libpng (no matplotlib dependencies) and does not do anything fancy: no text, no callbacks, no colormaps. But, it's really quite fast and it comes with a couple colormaps -- algae, jet, gist_stern and hot. The API is pretty easy. You can either call: import yt.extensions.image_writer as iw iw.write_image(image, filename, color_bounds = None, cmap = "algae") where image is a numpy array of values to be colormapped, or you can directly call the image writer: yt.amr_utils.write_png(some_image_data, filename) where some_image_data is uint8 and is (N,M,4). Unfortunately, generating FixedResolutionBuffers still requires that matplotlib be imported; I'll work on getting around this sometime, because if this ends up working we should be able to run on Kraken in the compute nodes without importing matplotlib. Although, Cray has now announced they're going to support dynamically linked libraries on their compute nodes, so maybe we won't need this for long. That being said, it should also be pretty handy for things like writing out volume renderings and anywhere else we previously used pylab to save images rather than plots. Let me know if you have any ideas or problems! -Matt

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Adding new codes, getting involved, and gadget pages
by Matthew Turk April 9, 2010

April 9, 2010

Hi guys, I just wanted to bring your attention to a couple pages I've written up: http://yt.enzotools.org/wiki/GettingInvolved http://yt.enzotools.org/wiki/AddingSupportForANewCode http://yt.enzotools.org/wiki/GadgetSupport Please feel free to edit these three pages -- particularly that first one, which has a list of enhancement ideas! These were written thanks to a suggestion from Tom, who thought it might be useful to have this kind of information (particularly about getting support for more codes, especially Gadget) written up as a reference. -Matt

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Test Problem Coverage
by Matthew Turk April 8, 2010

April 8, 2010

Hi all, I know several of you are or will be involved in test problem coverage for the new release of Enzo. I would like to underscore that problems, cosmetic or real, that show up in yt as a result of increasing test coverage of Enzo are *critically important* to fix. This goes even to things like the display of field names and so on. Please feel free to fix any problems that you find along the way. -Matt

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