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  •  The Laboratory for Computational Science & Engineering (LCSE)

    The Laboratory for Computational Science & Engineering  (LCSE)
    provides a facility within the University of Minnesota’s Digital Technology Center in which innovative hardware and system software solutions to problems in computational science and engineering can be tested and applied.  The LCSE has a broad mandate to develop innovative high performance computing and data visualization technologies in collaboration with both government and industry.  The lab is open to the University’s Institute of Technology faculty and their students.
    Work in the LCSE has been supported by a series of NSF equipment grants, with the latest a CRI grant No. CNS-0708822.


    High Performance Computing
    research in the LCSE has been focused since the lab’s founding in 1995 on the SMP cluster architecture, with which LCSE researchers did pioneering work with Silicon Graphics in 1993.  SMP cluste rs containing thousands of nodes today have only 2 to 4 processors in each SMP.   However, thanks to a generous donation from Unisys, the LCSE is now working with a Unisys ES7000 machine, which houses two SMPs, each with 16 Intel Itanium-2 CPUs running at 1 GHz and each with 32 GB of memory. Such powerful new SMPs offer the potential to build more attractive SMP clusters based on the Intel IA-64 CPU architecture in the near future. The LCSE is an NCSA Alliance partner, and is developing methods to exploit geographically distributed SMP clusters such as the NSF TeraGrid.  Through support from the DoE ASCI program, the LCSE is also targeting very large, tightly coupled SMP clusters. In addition to the classic emphasis on single node performance and parallel algorithm structure, these new cluster systems demand more flexible computing techniques that are latency tolerant, fault tolerant, and that adapt dynamically to changing system loads.   The LCSE’s SHMOD (SHared Memory On Disk)  and PPMlib libraries have been used to compute the billion-cell simulation of homogeneous, compressible turbulence, from which the vorticity distribution in a slice of the domain is visualized here at the left (using the LCSE's HVR volume rendering utility). All this LCSE software is available for download from this Web site. See for the SHMOD library, example code, and documentation. See for the PPMlib library and documentation. See for the HVR volume rendering utility and documentation.

    Scientific Visualization has driven much of the work on systems and software at the LCSE.  The need to extract scientific understanding from the terabytes of numerical data produced by supercomputer simulations has driven LCSE researchers to develop powerful visualization systems and software.  The LCSE worked with Silicon Graphics, Seagate, and Ciprico to develop the PowerWall visualization system in 1994.  The LCSE’s latest refinement of the PowerWall, now installed in the first floor of the Digital Technology Center, has been supported by NSF and the DoE through NCSA and the ASCI program, as well as generous support from SGI, Cray, Seagate, Ciprico, Ancor, and Brocade.  The 13 million pixels of the PowerWall display allow researchers to see simulation or other data in unprecedented detail.  The PowerWall can also be used to present multiple related views simultaneously.  An example is given by the 6 visualizations below on this page showing different physical variables from the same simulation of a giant star in the late stages of its life. The LCSE is presently working with Unisys to experiment with driving the entire PowerWall from a single Unisys ES7000 machine.

    PC Clusters and Storage Area Networks have provided the principal engines for data analysis, image rendering, and movie animation at the LCSE until the recent arrival of the Unisys ES7000.  A heterogeneous cluster of 10 PCs now handles movie animation on the PowerWall display.  This system exploits the powerful new graphics cards develped for PC gamers to render images in parallel for the PowerWall from multi-terabyte data sets.  We are in the process of rebuilding the LCSE infrastructure, so that the new Unisys ES7000 machine, attached to a Fibre Channel storage area network (SAN) of 4.8 TB capacity, can act as the central nervous center of the system.  With a Gigabit Ethernet link to the University’s OC-12 Internet-2 connection, massive data sets can be streamed onto the LCSE SAN for data analysis and visualization.  The LCSE is developing software ( to allow remote users to steer the visualization of such data and to stream the resulting movie animations to their local displays.


    An experiment in Grid computing is now underway at the LCSE. With support from an NSF CISE Research Resources grant, and from the Digital Technology Center (DTC) through the Minnesota Supercomputing Institute (MSI), the LCSE is connecting its recently donated Unisys ES7000 to 66 Dell PCs and 32 Macs in a student lab operated by the University of Minnesota's Academic and Distributed Computing Services. This student lab is located on the same floor of the DTC building as the LCSE. We are adding to the Dell PCs dual 200 GB 7200 RPM Maxtor ATA-133 drives, with file systems striped by the Microsoft Windows 2000 operating system. We are also adding new Nvidia-based graphics cards and Gigabit Ethernet NICS to interconnect these machines on an extensive switching fabric. A TCP/IP version of our SHMOD framework's sRIO remote I/O server utility is being installed on each PC, making this a powerful storage area network. When the students are not using these machines, we plan to run both our PPM gas dynamics simulation code and our data analysis and visualization software on this system, coordinated by the Unisys ES7000 in the LCSE via the SHMOD framework. This is an experiment in Grid computing in which we are collaborating with the University of Minnesota's Center for Computational Genomics and Bioinformatics as well as the Fond du Lac Tribal and Commmunity College in Cloquet, Minnesota.

    Pushing the Limits of Disk System Capacity and Speed  is a constant occupation for the LCSE.  Its data visualization applications have provided a demanding testbed for the latest products of the visualization and storage industries.  This led to early experimentation with storage area networks and shared file systems in collaboration with SGI, Seagate, Ciprico, Ancor, and Brocade.  Two new companies, Sistina Software and DataPlow, came out of this work.  The LCSE invites collaboration with industry to jointly explore new mechanisms to deal with the extremely large simulation data sets that will soon be coming into the lab.  Each simulation on the 8-billion-cell grids now possible can generate as much as 100 TB, which will need to be condensed in the lab and converted to visual form in order to enable scientific discovery.

    Contact Information:  Laboratory for Computational Science & Engineering,  499 Walter Library,  117 Pleasant St. S.E.,  Minneapolis,  MN  55455. 612-625-4097.

     Prof. Paul R. Woodard,  LCSE Director;  Dept. of Astronomy;

    Mr. Michael Knox,  Systems Administrator;

    Simulations Featured in the PowerWall Demo:

     1. Richtmyer-Meshkov Instability. 
    This simulation was carried out in collaboration with the Lawrence Livermore National Lab and IBM.  The LCSE’s sPPM gas dynamics code was run on a grid of 8 billion cells on 3840 processors of the IBM ASCI system at LLNL.  This calculation was awarded the 1999 Gordon Bell Prize in the performance category.  The movie shows a sequence of roughly 3000 images of the gas entropy, which reveals the degree of mixing between two gases whose unstable multifluid interface has been forced through a wire mesh by a Mack 1.5 shock.

    2.  Turbulence. 
    This simulation (see image earlier on this page) with the LCSE’s PPM gas dynamics code was carried out on a grid of 1 billion cells on NCSA’s new Itanium cluster.   A more refined, 8-billion-cell simulation is underway as a “charter application” for the NSF TeraGrid. Data from this new simulation will be accurate enough to use as a numerical experiment that can serve to constrain and validate potential subgrid-scale models of turbulence.

     3.  Red Giant Star. 
    The LCSE team has studied the process of convection in stars like the sun for many years, funded by both NSF and NASA Grand Challenge grants.  More recently, studies have shifted to convection in the extended envelopes of giant stars near the ends of their lives.  At the right, 6 related variables are visualized in a simplified model of a three solar mass giant star.  In the image at the top left, a plume of relatively cool gas is seen (in blue) plunging into the central stellar core, being heated (yellow), and rising again on the other side. The apparent elliptical shapes of these views comes from the perspective on this star that has been sliced in half, so that we may see the global convection pattern in the interior.

    Play with a 2-D Version of the PPM Gas Dynamics Code on your own Windows PC. A 2-D version of the LCSE's PPM gas dynamics code can be downloaded from this Web site that will run a standard fluid dynamics test problem on your own PC. You might encounter a bug or two in the functioning of the window's controls, but this program has been run by University of Minnesota freshman successfully. If they can do it, you can too. Compressible fluid dynamics fans will recognize this test problem as the one first introduced by Emery in 1967. This is an updated version, with lots more interest than the original, so our freshmen would not get bored. Read about an earlier version of this program (we think it is backwards compatible and are too lazy to update the documentation) in the LCSE Wind Tunnel Experimenter's User Guide at You can introduce streams of either smoke in air or sulfur hexafluoride smoke, which will enter the wind tunnel at the left and help to visualize the flow, just like the people who made those beautiful pictures in An Album of Fluid Motion. Give it a try. At the worst it will only crash your PC. (Be warned that this application does not run properly on Windows ME.)

    [This software is provided with no assurance of its value in any respect. By downloading it, you agree not to distribute it and not to complain in any way about any effect or side effect of your use of this software. To run the software, you must download the .exe file and the associated DLLs that are on the above referenced Web site. You must have an Intel Pentium-III processor or better or equivalent to run this software. And watch out for that sulfur hexafuoride smoke. When it comes down the duct at the same speed as Mach 2 air, it hits the step in the duct at Mach 5! That can be a bit traumatic, as you can see in the image here. Maybe you are best advised to just stick to smoke in air. It's not real sulfur hexafluoride anyway -- just a gamma-law gas with a gamma of 1.09 and 4.88 times the density of air when at the same pressure and temperature. Enjoy. Oh, by the way, the multifluid aspect of this program is under development. So if it doesn't work for you, don't worry. It won't work for us either, so we'll fix it eventually and you need not send any E-mail to anyone about how it ruined your day by hanging, burning up your processor, or any other thing. Remember, you agreed not to complain. So don't.]

    Researchers and Support Staff