While the peak performance and energy efficiency of computing hardware are constantly growing, the development of fast scientific software is experiencing an important paradigm shift. Efficient algorithm implementations face rigid constraints about memory layouts, access patterns and FLOP/Byte ratios.
Diego Rossinelli (ETH Zurich) discusses the design of wavelet-based adaptive solvers for compressible flow simulations that run effectively on multi- and many-core architectures.
We terminate our series of videos from the CSCS User day with an invited presentation of Rustan Khaliullin.
Rustan is from the group led by Michele Parrinello, a professor at the ETH Zurich and the Università della Svizzera italiana, concluded the series of scientific lectures at the CSCS User Day 2011 with a presentation of the latest research breakthrough in the simulation of molecular dynamic processes. The team has succeeded in using molecular dynamic simulations to show how diamonds are formed from graphite under high pressure (see the full presentation).
An animation produced by Swiss scientists about the Reversing Magnetic Field of Planet Earth is one of the 16 selected animations for SC11 Scientific Visualization Showcase.
The visualization showcase relies on competitive selection visualizations with a goal to have an event and place at the conference that collects and showcases state-of-the-art scientific visualizations that relate to HPC problems. The Scientific Visualization Showcase will be presented at SC11 in a museum/art exhibit-style environment so that attendees can experience and enjoy the latest in science and engineering HPC results expressed through state-of-the-art visualization technologies.
The visualization about the Reversing Magnetic Field of Planet Earth has been created by Jean M. Favre (CSCS), Jon Rotvig (ETH Zurich) and Andrew Jackson (ETH Zurich).
The magnetic field generated in the fluid metallic core of planet Earth is shown. Numerical simulations of the dynamo mechanism, such as this one, exhibit polarity reversals, whereby the north pole moves by 180 degrees; this mimics the behaviour documented many times within the geological record. Our simulation solves the equations of momentum transfer, heat transfer and electrodynamics in an electrically conducting and rapidly-rotating fluid at each point in time. High temperatures in the central part of the core drive thermal convection. The total simulation is equivalent to approximately 40,000 years on Earth. Our movie shows the magnetic field lines that enter and exit the core. High magnetic field strength is shown by red and yellow colours, and lower strengths by blue. On each field line we place a small compass needle with red and white ends, which orient itself in the direction of the field.
Dr. Daniele Passerone is leading the group of Computational Chemistry in the Nanotech and Surfaces Laboratory at EMPA. At the user day, he presented a poster on “Nanoscience surfaces: from substrate to adsorbate”.
Andrey Sheyko, PhD student in the group of Professor Andrew Jackson in the Institute for Geophysics at ETH Zurich presents his poster on “Equatorial dynamics and secular variation in rapidly rotating convection-driven numerical dynamo”.