Poster ID:
Poster Title:
Poster Abstract:
Poster Flle:
Author first name:
Author surname:



Poster Author:    Christopher Ngigi Christopher Ngigi
Poster ID:   C-13
Poster Title:   Comparison of h- and p-Derived Output-Based Error Estimates for Directing Anisotropic Adaptive Mesh Refinement in Three-Dimensional Inviscid Flows
Poster Abstract:  

The use of adjoint-based error estimation in conjunction with a highly parallel and scalable, anisotropic, block-based, adaptive mesh refinement (AMR) technique is considered for the more efficient prediction of three-dimensional compressible flows. In particular, a comparison is made between the computational performances of output-based error estimates, derived via two approaches, namely one based on mesh (or h) refinement and the other based on order (or p) refinement, for directing the mesh refinement in anisotropic AMR scheme. The AMR scheme allows enhancement of local mesh resolution, with preference given to directions as dictated by the flow solution. The proposed adjoint-based error estimation technique provides a posteriori estimates of the error for an engineering functional of interest in terms of estimates of the local solution error following from the solution residual. The estimated error in the solution residual is obtained either via direct refinement of the mesh in the preferred directions (here referred to as the h-derived error indicator) or by using a higher-order spatial operator with anisotropic feature detection based on the Hessian of an appropriate solution quantity (here referred to as the p-derived error indicator). Both approaches are considered here. Additionally, two formulations of the adjoint-based error indicator are examined here for directing the output-based AMR. The first is the so-called computable correction (CC), where the residual error is weighted by the corresponding adjoint solution for the functional of interest, and the second is the so-called error in the computable correction (ECC), which is comprised of a linear combination of the residual error weighted with the adjoint solution and the adjoint residual weighted with the primal solution. The resulting output error indicator is used to direct the mesh refinement, with regions of the solution domain contributing most significantly to the functional error being selected for local enrichment of the mesh. In this way, the computed accuracy of the functional is increased while potentially greatly reducing the associated computational cost of performing the simulation. For the cases of interest, both low- and high-order upwind finite-volume spatial discretization schemes are applied in conjunction with the block-based AMR scheme to the solution of the partial differential equations governing steady-state inviscid compressible flows. The potential benefits of the proposed anisotropic block-based AMR with adjoint-based error estimation are demonstrated for a range of compressible inviscid flow problems of varying complexity. Comparisons of solution accuracy and relative computational costs for results obtained using both h- and p-derived error estimates of the solution residual are examined and discussed.

Poster Flle:   PDF document IHPCSS_ngigi.pdf
 


Poster Author:    Stefan Hofmeister Stefan Hofmeister
Poster ID:   B-8
Poster Title:   Unsupervised segmentation of solar EUV images: The SPoCA CH module
Poster Abstract:  

The satellite Solar Dynamics Observatory observes the atmosphere of the Sun in the extreme ultra-violet (EUV) at a high resolution (4kx4k) and a high cadence (12s). The continuous observations allows us to track solar coronal holes (CH), i.e., regions in the solar corona with a reduced density, temperature, and an "open" magnetic field topology. Further, these regions are the source of high-speed solar wind streams. Whenever these high-speed plasma streams hit the Earth, they cause geomagnetic storms, which are responsible for polar lights, an increased drag-force on satellites, and geomagnetically induced currents (GIC). Here, we present the revised coronal hole module of the SPoCA suite, which allows unsupervised identification and tracking of coronal holes.

Poster Flle:   application/vnd.oasis.opendocument.presentation SPoCA_CH_module.odp
 


Poster Author:    Nuttiiya Seekhao Nuttiiya Seekhao
Poster ID:   A17
Poster Title:   High-Performance 3D Agent-Based Model of Vocal Fold Inflammation and Repair
Poster Abstract:  

High-fidelity bio-simulation tools have been applied in computational medicine to decipher the underlying cellular-level mechanisms of pathophysiology, predicting treatment response and suggest the most pertinent personalized treatments. To gain accuracy by increasing the relevant biological resolution, speed is often compromised as the model produces substantial amount of data in each iteration. This work presents a high-performance scheme designed to organize subtasks of agent-based model (ABM) of vocal fold inflammation and repair to fully utilize a heterogeneous platform consisting of multi-core CPU host with attached GPUs. The subtasks are further optimized based on their execution and data access characteristics. Conjointly, with the employment of VirtualGL, the model visualizes the results in situ providing the user with computational steering capability and interactivity in real-time. This 3D biological model is capable of processing (compute and visualize remotely) 154 million vocal fold biomarker data points per second, which is 900x more powerful than popular existing ABMs framework (NetLogo).

Poster Flle:   PDF document IHPCSS2017_Presentation_Seekhao_A17.pdf
 


Poster Author:    Edoardo Carlesi Edoardo Carlesi
Poster ID:   B4
Poster Title:   Constrained Local Universe Simulations
Poster Abstract:  

The Local Universe - that is, the group of galaxies, filaments, voids and galaxy clusters that surround our Milky Way galaxy, provides the best possible observations by virtue of its vicinity. The Constrained Local UniversE Simulations (CLUES) project's main goal is to simulate the Local Universe in order to use it as a numerical laboratory to test and constrain current models of cosmological structure formation, by directly comparing the simulations' output to the observations. Furthermore, these simulations can be used to reconstruct the evolution in time of the patch of space we live in, from the very first seconds after the Big Bang up to recent times, using billions of particles to sample at each step the distribution of the different types of matter density (dark or gaseous). Cosmological codes such as GADGET, Gasoline and AREPO are used to solve the equations of gravity and hydrodynamics in the non linear regime, allowing us to study in great detail the process of formation and evolution of stars, galaxies and galaxy clusters that shaped the properties of the Universe as we see it.


Poster Flle:   application/vnd.oasis.opendocument.presentation Carlesi_PosterB4
 


Poster Author:    Jorge Luis Barrera Cruz Jorge Luis Barrera Cruz
Poster ID:   D-2
Poster Title:   Topology Optimization of Elastomeric Gels
Poster Abstract:  

Research on soft, active materials have been increasingly growing in recent years; growth driven by poten- tial applications that leverage their unique properties, such as a wide range of stimulants, large deforma- tions, and high motion complexities. Recent work in this area includes not only the development of new materials and innovative technologies, but also more complex and robust mathematical models that better describe their physics. In this paper we introduce a shape and topology optimization approach for finding the spatial arrangement of stimuli-responsive elastomeric gels. We exploit the ability of elastomeric gels to swell upon exposure to a solvent to design actuators that deform from an initially flat/simple plate into a curved/desired structure. The highly nonlinear chemo-mechanical response of the gel is described by a mathematical model that advances in time through an internal state variable that represents the swelling state of the gel. In addition, we introduce a formulation for the computation of the sensitivities of using the adjoint method for problems which formulations include dependencies on internal state variables. The proposed optimization process is studied with numerical examples where the objective is to find the mate- rial layout such that the active composite assumes one or more target shapes upon activation. The design studies demonstrate the ability of the proposed optimization method to yield a highly resolved description of the optimized material layout that can be realized by 3D printing. As the complexity of the target shape increases, the optimal spatial arrangement of the material phases becomes less intuitive, highlighting the advantages of the proposed optimization method.


Poster Flle:  
 


Poster Author:    TT Toshiki Teramura
Poster ID:   A-18
Poster Title:   Non-Gaussian effect in Ensemble Kalman filter
Poster Abstract:  

Ensemble Kalman filter (EnKF) is an algorithm of numerical weather forecast (NWF) which combines numerical simulations and various types of observations interactively. The weather system is incredibly high-dimensional space. EnKF assumes the probability density function (PDF) of the current state of systems, e.g. temperature, moisture, and wind velocity field, to be Gaussian to reduce the calculation cost due to the high-dimensionality. This approximation works well for global forecast, however, it seems bad for local severe event, where instantaneous local nonlinear dynamics are important. This study evaluates the non-Gaussian effect as a bias of ensemble estimations. The non-Gaussian bias is revealed to be state-dependent, and is critically large only on a limited case. This study is done only on a low-dimensional system, and will be extended to realistic systems using HPC techniques.


Poster Flle:   PDF document ihpcss.pdf
 


Poster Author:    Deborah Good Deborah Good
Poster ID:   A-8
Poster Title:   CHIME: Mapping the Expanding Universe with a Redundant Array
Poster Abstract:  

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is one of a new class of cosmology experiments, mapping redshifted neutral hydrogen throughout the universe to learn more about one of the great scientific questions of our time: the accelerating expansion of the universe, i.e. dark energy. CHIME is a radio transit telescope consisting of four 20 m x 100 m cylinders with over 1000 antennas located in British Columbia, Canada. When completed later this summer, CHIME will generate about 135 TB of raw data per day, which must be carefully calibrated and compressed for storage. One tool CHIME can use for both calibration and compression is redundancy within the array, the property that many data products should contain the same information once calibrated. Harnessing this redundancy and accounting for imperfections in the telescope generate interesting analytical and computational challenges. 

Poster Flle:   Powerpoint 2007 presentation IHPCSS_electronic_poster.pptx
 


Poster Author:    Srinivasan Ramesh Srinivasan Ramesh
Poster ID:   B-15
Poster Title:   A Plugin Infrastructure for MPI Performance Engineering: Integrating MVAPICH and TAU via the MPI tools interface
Poster Abstract:  

MPI libraries today are complex software's that have modular components reflecting the constantly evolving software and hardware stack underneath. They offer the user a number of tunable parameters that can affect performance. In this environment, performance variations and scalability limitations can come from a number of sources. It is thus crucial to gain a holistic understanding of MPI library performance in order to fine-tune it for a given application and hardware setup. The MPI Tools Information Interface (MPI_T) introduced as part of the MPI 3.0 standard offers a standardized mechanism through which external tools can interact with an MPI library to perform runtime introspection and performance tuning. In this work, we describe a plugin infrastructure that utilizes the MPI_T interface to perform runtime tuning of MPI libraries. This plugin infrastructure is part of TAU, a popular performance analysis toolkit. While the plugin infrastructure is generic and can support any MPI implementation, we present a study of tuning applications running on MVAPICH, a widely used high-performance MPI implementation that offers a .wide range of performance metrics and tunable parameters through the MPI_T interface.

Poster Flle:   PDF document Poster_Srinivasan_Ramesh.pdf
 


Poster Author:    Xavier Yepes Arbós Xavier Yepes Arbós
Poster ID:   D-19
Poster Title:   Developments to improve the throughput and efficiency of Earth System Models
Poster Abstract:  

Computational models require an increasing amount of resources since more resolution is needed to have more accurate results. However, this probably implies to have less efficient executions. Earth System models (ESMs) are a concrete case that need to perform a lot of simulations with a reasonable time-to-solution. As a consequence, the efficiency at such levels of performance is really low, so optimizations are crucial to overcome this problem.
Therefore, as a member of the Earth Sciences Department of the Barcelona Supercomputing Center (BSC), my main research is focused on analysing the bottlenecks of climate and weather models to then apply state-of-the-art methodologies to get the maximum performance of HPC clusters with a reasonable efficiency. To achieve it, I am currently working in three research lines: the first one is analysing the EC-Earth model using performance tools to detect bottlenecks; the second line studies how to enhance the throughput in ESM workflows by using a performance-efficiency trade-off metric; and the third research line is focused on integrating XIOS (an asynchronous input/output server) into OpenIFS (an atmospheric model) to increase the throughput and offer a more versatile output control.


Poster Flle:   PDF document IHPCSS17-XavierYepes.pdf
 


Poster Author:    Ondrej Vysocky Ondrej Vysocky
Poster ID:   D18
Poster Title:   High Performance Computing Applications Dynamism Evaluation for Energy Tuning
Poster Abstract:  

This poster introduces the Horizon 2020 READEX project (Runtime Exploitation of Application Dynamism for Energy-efficient eXascale computing) and its approach of dynamic application behavior analysis and tuning. The attention is paid to the manual application evaluation from the energy consumption point of view. This is the key step in exploring the possible gains of the runtime dynamic tuning. We present the effect of static (constant settings for the entire application runtime) and dynamic tuning (different settings for different parts of the application code) of the CPU core frequency, CPU uncore frequency and the number of active cores on the energy consumption of an HPC cluster running selected application. 
 
To show the potential dynamism we have evaluated basic kernels with various computational intensity (DGEMV, DGEMM and compute only kernel) and parallel I/O. Also, two full fledge applications: ESPRESO FEM library with FETI solvers and open-source CFD tool OpenFOAM were evaluated. The results show that these two complex applications can achieve energy savings of 21.3% and 17.7%, respectively, as a combination of static and dynamic tuning.

Poster Flle:   PDF document IHPCSS-Vysocky.pdf