View allAll Photos Tagged SuperComputer

Currently in development for delivery in late 2021, the Oak Ridge Leadership Computing Facility's Frontier supercomputer will help guide researchers to new discoveries at exascale.

 

Read more: www.olcf.ornl.gov/frontier/

 

17/07/2025. Bristol, United Kingdom. Secretary of State Peter Kyle switched on Isambard-AI, the UK's most powerful supercomputer housed at the University of Bristol. Picture by Alecsandra Dragoi / DSIT

Peter Nugent - LBL astro-computation

with Cray XT-4 supercomputer cluster at Oakland Scientific Facility

 

credit: Lawrence Berkeley Nat'l Lab - Roy Kaltschmidt, photographer

 

XBD200705-00167.TIF

Arsenal (Vienna)

The Vienna Arsenal, object 1

(Pictures you can see by clicking on the link at the end of page!)

The Arsenal in Vienna is a former military complex in the southeast of the city, located in the 3rd district of Vienna. The mighty, consisting of several brick buildings facility is located on a rectangular plan on a hill south of the Country Road Belt (Landstraßer Gürtel).

Meaning

The Arsenal is the most important secular assembly of Romantic Historicism in Vienna and was conducted in Italian-Medieval and Byzantine-Moorish forms. Essentially the complex is preserved in its original forms; only the former workshop buildings within the bounding, from the the outside visible wings were replaced by new constructions.

History to 1945

Bird's eye view of the complex, arsenal, lithography Alexander Kaiser, 1855

Vienna Arsenal (Museum of Military History)

Arsenal, with HGM (Heeresgeschichtliches Museum) from the East

The complex, with a total of 31 "objects" (buildings) was built from 1849 to 1856 on the occasion of the March Revolution of 1848 and was the first building of the fortress triangle, replacing the old Vienna's city walls, with the Rossauer Barracks and the now-defunct Franz Joseph barracks at Stubenring. These buildings should not serve to deter foreign enemies from the city, but to secure state power in the event of revolutionary upheavals in Vienna. The decision to build the Arsenal, it came from the 19-year-old Emperor Franz Joseph I who on 2 December 1848 had come to the throne.

The design for the Imperial Artillery Arsenal came from General Artillery Director Vincenz Freiherr von Augustin, to which, subsequently, the site management had been transferred. Under his leadership, the buildings under assignment of sectors have been planned of the architects Carl Roesner, Antonius Pius de Riegel, August Sicard von Sicardsburg, Eduard van der Nüll, Theophil von Hansen and Ludwig Förster and built by the company of the architect Leopold Mayr.

From 1853 to 1856, Arsenal church was built by the architect Carl Roesner. The K.K. Court Weapon Museum, later K.K. Army Museum, now Museum of Military History, housed in a separate representative free-standing wing, was completed structurally in 1856, but was only in 1869 for the first time accessible.

For the construction of the Arsenal 177 million bricks were used. Construction costs totaled $ 8.5 million guilders. In the following years, there have been extensions. During the two world wars, the complex served as a weapons factory and arsenal, especially as barracks.

The record number of employees in Arsenal was reached in the First World War, with around 20,000 staffers. After 1918, the military-industrial operation with own steel mill was transformed into a public service institution with the name "Austrian Factories Arsenal". However, there were almost insoluble conversion problems in the transition to peacetime production, the product range was too great and the mismanagement considerable. The number of employees declined steadily, and the company became one of the great economic scandals of the First Republic.

By the fall of 1938, the area belonged to the 10th District Favoriten. However, as was established during the "Third Reich" the Reich District of Greater Vienna, became the arsenal complex and the south-east of it lying areas in the wake of district boundary changes parts of the 3rd District.

During the Second World War, in the Arsenal tank repair workshops of the Waffen-SS were set up. In the last two years of the war several buildings were severely damaged by bombing. During the Battle of Vienna, in the days of 7 to 9 April 1945, was the arsenal, defended by the 3rd SS Panzer Division "Totenkopf", focus of the fighting, the Red Army before its victory facing heavy losses.

History since 1945

Ruins of the object 15 after the air raids 1944

Deposits at the Arsenal Street

After heavy bomb damages during the Second World War, the buildings of the Arsenal were largely restored to their original forms.

In the southern part and in the former courtyard of the arsenal several new buildings were added, among them 1959-1963 the decoration workshops of the Federal Theatre designed by the architects Erich Boltenstern and Robert Weinlich. From 1961 to 1963, the telecommunications central office was built by the architect Fritz Pfeffer. From 1973 to 1975 were built operation and office building of the Post and Telephone Head Office for Vienna, Lower Austria and Burgenland (now Technology Centre Arsenal of Telekom Austria) with the 150-meter high radio tower in Vienna Arsenal according to the plans of architect Kurt Eckel. In the 1990s, a rehearsal stage of the Castle Theater (Burgtheater) was built according to plans by Gustav Peichl.

Also the Austrian Research and Testing Centre Arsenal, now Arsenal Research, which has made itself wordwide a celebrity by one of the largest air chambers (now moved to Floridsdorf - 21st District), was housed in the complex. A smaller part of the complex is still used by the Austrian army as a barracks. Furthermore, the Central Institute for Disinfection of the City of Vienna and the Central Chemical Laboratory of the Federal Monuments Office are housed in the arsenal. The Military History Museum uses multiple objects as depots.

In one part of the area residential buildings were erected. The Arsenal is forming an own, two census tracts encompassing census district, which according to the census in 2001 had 2.058 inhabitants.

End of 2003, the arsenal in connection with other properties of the Federal Property Society (BIG - Bundesimmobiliengesellschaft) was sold to a private investor group. Since early 2006, the lawyer of Baden (Lower Austria, not far away from Vienna) Rudolf Fries and industrialist Walter Scherb are majority owners of the 72,000 m2 historic site that they want to refurbish and according to possibility rent new. Fries also plans to enlarge the existing living space by more than a half (about 40,000 m2).

An architectural design competition, whose jury on 28 and 29 in June 2007 met, provided proposals amounting to substantial structural changes in the complex. Such designed competition winner Hohensinn a futuristic clouds clip modeled after El Lissitzky's cloud bracket, a multi-level horizontal structure on slender stilts over the old stock on the outskirts of the Swiss Garden. The realization of these plans is considered unlikely.

Some objects are since 2013 adapted for use by the Technical University of Vienna: Object 227, the so-called "Panzerhalle" will house laboratories of the Institute for Powertrains and Automotive Technology. In object 221, the "Siemens hall", laboratories of the Institute for Energy Technology and Thermodynamics as well as of the Institute for Manufacturing Technology and High Power Laser Technology are built. In object 214 is besides the Technical Testing and Research Institute (TVFA) also the second expansion stage of the "Vienna Scientific Cluster" housed, of a supercomputer, which was built jointly by the Vienna University of Technology, the University of Vienna and the University of Agricultural Sciences.

Accessibility

The arsenal was historically especially over the Landstraßer Gürtel developed. Today passes southeast in the immediate proximity the Südosttangente called motorway A23 with it connection Gürtel/Landstraßer Hauptstrasse. Southwest of the site runs the Eastern Railway, the new Vienna Central Station closes to the west of the arsenal. Two new bridges over the Eastern Railway, the Arsenal Stay Bridge and the Southern Railway bridge and an underpass as part of Ghegastraße and Alfred- Adler-Straße establish a connection to the on the other side of the railway facilities located Sonnwendviertel in the 10th District, which is being built on the former site of the freight train station Vienna South Station.

On the center side is between Arsenal and Landstraßer Gürtel the former Maria Josefa Park located, now known as Swiss Garden. Here stands at the Arsenal street the 21er Haus, a branch of the Austrian Gallery Belvedere, on the center-side edge of the Swiss Garden has the busy suburban main railway route the stop Vienna Quartier Belvedere, next to it the Wiener Linien D (tram) and 69A (bus) run.

de.wikipedia.org/wiki/Arsenal

ORNL Deputy Director for Science and Technology Thomas Zacharia with the Cray XT5 Jaguar.

31102D, Aurora Press Conference with ANL, Intel, and Cray

 

Photographer: Mark Lopez

The Indy, code-named "Guinness", is a low-end workstation introduced on 12 July 1993. Developed and manufactured by Silicon Graphics Incorporated (SGI), it was the result of their attempt to obtain a share of the low-end computer-aided design (CAD) market, which was dominated at the time by other workstation vendors; and the desktop publishing and multimedia markets, which were mostly dominated at the time by Apple Computer. It was discontinued on 30 June 1997 and support ended on 31 December 2011.

 

en.wikipedia.org/wiki/SGI_Indy

 

Retrocomputing (a portmanteau of retro and computing) is the use of early computer hardware and software today. Retrocomputing is usually classed as a hobby and recreation rather than a practical application of technology; enthusiasts often collect rare and valuable hardware and software for sentimental reasons. However some do make use of it.[1] Retrocomputing often gets its start when a computer user realizes that expensive fantasy systems like IBM Mainframes, DEC Superminis, SGI workstations and Cray Supercomputers have become affordable on the used computer market, usually in a relatively short time after the computers' era of use.

 

en.wikipedia.org/wiki/Retrocomputing

 

Con il termine retrocomputing si indica una attività di "archeologia informatica" che consiste nel reperire, specialmente a costi minimi, computer di vecchie generazioni, che hanno rappresentato fasi importanti dell'evoluzione tecnologica, ripararli se sono danneggiati, metterli nuovamente in funzione e preservarli.

 

it.wikipedia.org/wiki/Retrocomputing

Congressman Dan Lipinski speaks of the importance supercomputers to the advancement of science.

 

31102D, Aurora Press Conference with ANL, Intel, and Cray

 

Photographer: Mark Lopez

Aaron Knoll, research scientist within the SCI Institute at the University of Utah, on  'Visualization with OSPRay: Research and Production' at the Intel Xeon Phi User's Group (IXPUG) annual meeting at Argonne.

Congressman Randy Hultgren address the press.

 

"Few other investments have as much potential to demonstrate dramatic progress and capability across a broad range of scientific fields with real-world interests."

 

31102D, Aurora Press Conference with ANL, Intel, and Cray

 

Photographer: Mark Lopez

PI: Thierry Poinsot, CERFACS

 

Fields of temperature and pressure, along with stream lines and a temperature isosurface representing the flame, are shown in a 330-million-elements simulation of a complete helicopter combustion chamber performed on the IBM Blue Gene/P at the ALCF.

 

Credit: Pierre Wolf, Turbomeca and CERFACS.

 

Celebrating "Two Billion Hours Served" by the Argonne Leadership Computing Facility are (from left to right) ALCF Director Pete Beckman, Director of Science Paul Messina and Manager of User Support and Outreach David Martin.

 

The staff of ALCF, the Mathematics and Computer Science Division and Computing, Environment, and Life Sciences recently celebrated the ALCF's surpassing two billion processor-hours of computations at a mind-boggling speed of more than 557 trillion calculations per second. The project that clicked the supercomputer Intrepid over its 2 billionth hour of science was "Uncertainty Quantification for Turbulent Mixing," a simulation of the turbulent mixing of two fluids, conducted by a group from Stony Brook University, New York.

 

Details are available on the ALCF Web site »

 

Argonne National Laboratory.

  

Summit is the fastest supercomputer in the world, according to the TOP500 list, which ranks global computing systems. Summit is the third ORNL system to top this list, preceded by the Jaguar and Titan supercomputers. Representatives from ORNL, IBM, NVIDIA, Red Hat, and Mellanox Technologies accepted the award at the ISC High Performance conference in Frankfurt, Germany.

 

+ Read more: www.ornl.gov/news/ornl-s-summit-supercomputer-named-world...

 

Image credit: NVIDIA

Eugene DePrince, a scientist whose job is funded by the Recovery Act, views a computer-generated optical image.

 

DePrince is using the laboratory's IBM Blue Gene/P supercomputer to perform basic research that will one day help scientists create invisible materials. Read the full story »

 

Argonne has received significant funding through the American Recovery and Reinvestment Act (ARRA), allowing us to accomplish a number of important goals while putting Americans back to work. We’ve interviewed several ARRA-funded employees to see how their new job has changed their lives. More profiles »

 

Argonne National Laboratory.

Oct. 25, 2012 – Sandy reached its initial peak intensity as a Category 3 hurricane over Cuba.

 

Credit: NASA's Goddard Space Flight Center and NASA Center for Climate Simulation

Video and images courtesy of NASA/GSFC/William Putman

 

--

 

A NASA computer model simulates the astonishing track and forceful winds of Hurricane Sandy.

 

Hurricane Sandy pummeled the East Coast late in 2012’s Atlantic hurricane season, causing 159 deaths and $70 billion in damages. Days before landfall, forecasts of its trajectory were still being made. Some computer models showed that a trough in the jet stream would kick the monster storm away from land and out to sea. Among the earliest to predict its true course was NASA’s GEOS-5 global atmosphere model. The model works by dividing Earth’s atmosphere into a virtual grid of stacked boxes. A supercomputer then solves mathematical equations inside each box to create a weather forecast predicting Sandy’s structure, path and other traits. The NASA model not only produced an accurate track of Sandy, but also captured fine-scale details of the storm’s changing intensity and winds. Watch the video to see it for yourself.

 

For more information, please visit:

gmao.gsfc.nasa.gov/research/atmosphericassim/tracking_hur...

 

NASA image use policy.

 

NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

 

Follow us on Twitter

 

Like us on Facebook

 

Find us on Instagram

Note the liquid cooling

i09_0214 171

2013. Senator Dick Durbin (Ill.) joined Argonne staff to celebrate the dedication of Mira, the lab's new supercomputer and the fifth fastest computer in the world today. Above: Argonne director Eric Isaacs speaks at the ceremony.

 

Read more »

 

30494D

 

Tutorials at ISC 2017 in Frankfurt, Germany (copyright: Philip Loeper)

Touring the Argonne Leadership Computing Facility's Mira supercomputer.

 

(from left) Maroš Šefčovič, European Vice President for Energy Union; Michael Papka, Deputy Associate Lab Director, Computing, Environment and Life Sciences; Peter Littlewood, Director Argonne National Laboratory; Vladimir Sucha, Dir. General of the Joint Research Center (JRC); Jury Nociar, Head of Cabinet of Vice President for Energy Union.

2000: Breaking the teraflop barrier

 

The expansion of ORNL’s IBM RS/6000 SP supercomputer pushes it past the 1 trillion calculations per second (1 teraflop) mark. Eagle and the Compaq AlphaServer SC system Falcon give ORNL more than 1.5 teraflops combined computing speed. Read more...

IBM supercomputer, named bluefire, used for climate and weather simulations at NCAR. At installation it was ranked in the 25th most powerful supercomputers in the world. The main computer consisting of 11 cabinets (weighing 3,200lbs each) are in the background. Temporary memory used by bluefire is in the foreground. Here's some details for you computer buffs:

 

4,064 POWER6 Processors, running at 4.7 Ghz

76.4 teraflops (at peak) - that's 76.4 trillion operations per second

12 terabytes of memory

150 terabytes of high performance disk

Hydro-cluster cooling - a liquid cooling system 33% more efficient than air-cooled.

 

2013. Senator Dick Durbin (Ill.) joined Argonne staff to celebrate the dedication of Mira, the lab's new supercomputer and the fifth fastest computer in the world today. Above: Argonne director Eric Isaacs speaks at the ceremony.

 

Read more »

 

30494D

   

Sequoia, a supercomputer built for NNSA, has been named the fastest in the world by Top500. Operating at 16.32 petaflops (quadrillion floating point operations per second), Sequoia helps monitor the nation's nuclear weapons stockpile by simulating weapons performance in high detail.

31102D, Aurora Press Conference with ANL, Intel, and Cray

 

Photographer: Mark Lopez

2012. Mira has been ranked the third fastest supercomputer in the world as of 2012.

Petascale quantum mechanical-molecular dynamics simulations on Argonne’s Blue Gene/P supercomputer encompass large spatiotemporal scales (multibillion atoms for nanoseconds and multimillion atoms for microseconds). They are improving our understanding of atomistic mechanisms of stress corrosion cracking of nickel-based alloys and silica glass—essential for advanced nuclear reactors and nuclear-waste management.

 

In this image: Fracture simulations for nanocrystalline nickel without and with amorphous sulfide grain-boundary phases reveal a transition from ductile, transgranular tearing to brittle, intergranular cleavage. Image courtesy Hsiu-Pin Chen of USC et al., Physical Review Letters 104, 155502.

 

For more information, visit the Argonne Leadership Computing Facility (ALCF) website.

 

Image courtesy of Argonne National Laboratory.

Dr. Patricia Falcone, Brig. Gen. Daniel P. Hughes and Sen. Ben Cardin (D-MD) join other Army officials to cut the ceremonial ribbon at the Army's Supercomputing Research Center at Aberdeen Proving Ground, Md., June 10, 2013.

 

Falcone is the associate director for National Security and International Affairs in the White House Office of Science and Technology Policy. Hughes is the deputy commanding general for the U.S. Army Research, Development and Engineering Command. Cardin has represented Maryland in the U.S. Senate since 2006.

 

The Army Research Laboratory will use the center to influence the direction of future armor solutions and other unprecedented capabilities for Soldiers.

Summit is the fastest supercomputer in the world, according to the TOP500 list, which ranks global computing systems. Summit is the third ORNL system to top this list, preceded by the Jaguar and Titan supercomputers. Representatives from ORNL, IBM, NVIDIA, Red Hat, and Mellanox Technologies accepted the award at the ISC High Performance conference in Frankfurt, Germany.

 

+ Read more: www.ornl.gov/news/ornl-s-summit-supercomputer-named-world...

Summit is the fastest supercomputer in the world, according to the TOP500 list, which ranks global computing systems. Summit is the third ORNL system to top this list, preceded by the Jaguar and Titan supercomputers. Representatives from ORNL, IBM, NVIDIA, Red Hat, and Mellanox Technologies accepted the award at the ISC High Performance conference in Frankfurt, Germany.

 

+ Read more: www.ornl.gov/news/ornl-s-summit-supercomputer-named-world...

 

Image credit: Graham Lopez/ORNL

31102D, Aurora Press Conference with ANL, Intel, and Cray

 

Photographer: Mark Lopez

Elijah Snow is hired by Jakita Wagner to join Planetary, a four-man team (3 field agents and one mysterious backer known as "the Fourth Man") looking to uncover the hidden history of the world as "mystery archeologists." Their first mission: to explore a man-made cavern in the Adirondacks, the last known destination of Doc Brass, an adventurer from the 1930s and 1940s.

 

Elijah Snow is asked by Jakita Wagner to join Planetary -- a group of archaeologists who map the secret history of the world -- as their new field agent. He joins under the promise of a million dollars a year and record of him eliminated. He is introduced to The Drummer and goes on his first investigation that of going to view the secret base of a Renaissance Man and adventurer named Dr, Axel Brass; a man who may no longer need to eat or sleep. After arriving at the headquarters Elijah and Jakita see Brass still alive but with damaged legs Doc Brass then tells them that years ago in the forties he and his fellow adventurers had secretly gathered in the same base and had created a supercomputer that harassed the 196,833 universes and realign them and merge them, Doc Brass and his associates wished to use the device and the multiverse in a attempt to create a perfect world but failed when a group of people (JLA-like beings) from another universe used the computer to come to their universe. The other beings universe was dying and these beings attempted to take the other world and kill everyone on this Earth for their Earth's population a battle ensued and all were killed except Brass who suspects the years is 1970. Planetary crew cleans up Doc Brass' headquarters while he will be placed in care. Elijah tells Jakita how strange the world is while Jakita tells him "Let's keep it that way".

 

Elijah Snow is approached in a diner in the middle of the desert by Jakita Wagner, who attempts to recruit him into Planetary -- a group of archaeologists who map the secret history of the world -- as their new field agent, or "third man". He reluctantly joins under the promise of a million dollars a year and all public records of his life eliminated. He is introduced to The Drummer -- the final member of the field team -- and accompanies his teammates on an investigation of a secret Adirondacks base of Renaissance Man and adventurer Dr, Axel Brass.

 

Upon arriving at the mountain stronghold, Elijah and Jakita discover Brass still alive within the compound, having sustained crippling injuries to his legs many years ago. Brass tells them of his companions in the 1940s -- like-minded adventurers including Hark, Kevin Sack (Lord Blackstock), and the Dark Millionaire --and the supercomputer they built that harnessed the power of 196,833 universes in order to realign and merge them. In their attempt to use the device to create a perfect world, they opened a rift into another universe where seven strangers (a pastiche of the most iconic members of the Justice League) awaited them. These strangers came from a dying universe, and they desperately fought Brass and his companions in an attempt to overtake our reality and replace this Earth's population with their own. In the enusing battle, all combatants perished save for Brass, who stayed in the stronghold to defend it against potential incursions from other dimensions. Having long since overcome the need to eat or sleep and having learned to will his body to heal itself, he has maintained his vigil over the supercomputer ever since, estimating that the year is roughly 1970.

 

After his tale, the Planetary team cleans up Brass' headquarters and takes him into their care, setting up a watch on the supercomputer and archiving the contents of the fortress. Elijah comments to Jakita how strange the world is, to which Jakita responds, "Let's keep it that way"; this statement will become the mantra of the series going forward.

 

The issue is conceptually about the rise of superhero comics, which overthrew the pulp adventure tales of the day (represented by Doc Brass and his companions, who resemble classic characters such as Tarzan and The Shadow).

Intel Xeon Phi User's Group (IXPUG) annual meeting attendee.

The Argonne Leadership Computing Facility (ALCF) major acquisition, the Blue Gene/P supercomputer, will boost the facility's total computing power to 556 teraflops, representing a fivefold increase in system capability. This advance will help to initiate the coming era of petascale computing and enable experts to answer questions that have confounded America's scientists for years. Photo courtesy of Argonne National Laboratory.

The Department of Energy's Oak Ridge National Laboratory welcomed the public to its Lab Day on Saturday, June 9, marking the laboratory's 75th anniversary with exhibits, science talks, tours, music and food.

 

Approximately 4,500 attendees experienced ORNL's Traveling Science Fair exhibits, packed tours to facilities including the High Flux Isotope Reactor, Spallation Neutron Source, Oak Ridge Leadership Computing Facility, the Historic Graphite Reactor Museum and the Building Technologies Research and Integration Center.

 

OLCF staff members gave tours of the facility to attendees, first demonstrating the power of parallel computing using the PArTI (Parallel Architecture Test Instance) and then providing an up-close experience with the Summit supercomputer at the Summit viewing area.

 

Read more: www.ornl.gov/news/ornl-marks-75th-anniversary-lab-day

 

Deep in space, giant galaxy clusters filled with vast clouds of hot, X-ray producing gas are assembled through supersonic collisions over billions of years. In order to better understand these astrophysical phenomena, called galaxy cluster mergers, scientists visualize them using supercomputers—resulting in this beautiful image.

 

ABOVE: Dark matter makes up the majority of the cluster material, up to 90% by mass, and the gravitational force of the dark matter dominates the physics of the merger. Most of the ordinary matter is in the form of a hot, diffuse plasma known as the intra-cluster medium. These gases interact directly, unlike the dark matter particles, whose motion is thought to be collisionless. However the mixing of the gas is completely driven by the violent orbital motion of the dark matter cores. Shown here are volume renderings of the gases (in blue and yellow) zoomed in so that detail of the structure involved in the interaction of dark matter particles and the gases can be seen.

 

Researchers: John Zuhone, Harvard-Smithsonian CfA; Donald Q. Lamb, University of Chicago

 

Visualizations by Brad Gallagher, University of Chicago.

 

Research supported by:

DOE/NNSA ASC Alliance Flash Center, DOE/Office of Science INCITE Program

 

Argonne National Laboratory.

2013. Senator Dick Durbin (Ill.) joined Argonne staff to celebrate the dedication of Mira, the lab's new supercomputer and the fifth fastest computer in the world today.

 

Read more »

 

30494D

Edited Chandra Space Telescope visualization of the center of the Milky Way Galaxy. Round variant in inverted grayscale.

 

Original caption: Want to take a trip to the center of the Milky Way? Check out a new immersive, ultra-high-definition visualization. This 360-movie offers an unparalleled opportunity to look around the center of the galaxy, from the vantage point of the central supermassive black hole, in any direction the user chooses.

 

By combining NASA Ames supercomputer simulations with data from NASA's Chandra X-ray Observatory, this visualization provides a new perspective of what is happening in and around the center of the Milky Way. It shows the effects of dozens of massive stellar giants with fierce winds blowing off their surfaces in the region a few light years away from the supermassive black hole known as Sagittarius A* (Sgr A* for short).

 

These winds provide a buffet of material for the supermassive black hole to potentially feed upon. As in a previous visualization, the viewer can observe dense clumps of material streaming toward Sgr A*. These clumps formed when winds from the massive stars near Sgr A* collide. Along with watching the motion of these clumps, viewers can watch as relatively low-density gas falls toward Sgr A*. In this new visualization, the blue and cyan colors represent X-ray emission from hot gas, with temperatures of tens of millions of degrees; red shows moderately dense regions of cooler gas, with temperatures of tens of thousands of degrees; and yellow shows of the cooler gas with the highest densities.

 

A collection of X-ray-emitting gas is seen to move slowly when it is far away from Sgr A*, and then pick up speed and whip around the viewer as it comes inwards. Sometimes clumps of gas will collide with gas ejected by other stars, resulting in a flash of X-rays when the gas is heated up, and then it quickly cools down. Farther away from the viewer, the movie also shows collisions of fast stellar winds producing X-rays. These collisions are thought to provide the dominant source of hot gas that is seen by Chandra.

 

When an outburst occurs from gas very near the black hole, the ejected gas collides with material flowing away from the massive stars in winds, pushing this material backwards and causing it to glow in X-rays. When the outburst dies down the winds return to normal and the X-rays fade.

 

The 360-degree video of the Galactic Center is ideally viewed through virtual reality (VR) goggles, such as Samsung Gear VR or Google Cardboard. The video can also be viewed on smartphones using the YouTube app. Moving the phone around reveals a different portion of the movie, mimicking the effect in the VR goggles. Finally, most browsers on a computer also allow 360-degree videos to be shown on YouTube. To look around, either click and drag the video, or click the direction pad in the corner.

 

Dr. Christopher Russell of the Pontificia Universidad Católica de Chile (Pontifical Catholic University) presented the new visualization at the 17th meeting of the High-Energy Astrophysics (HEAD) of the American Astronomical Society held in Monterey, Calif. NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

PI: Robert Moser, University of Texas at Austin

 

Computationally derived images, like the one shown, allow researchers to visualize the turbulent flows that affect many vehicles. A better understanding of the physics of turbulence will aid engineers in improving fuel economy.

 

Credit: Juan Sillero, Universidad Politécnica de Madrid

The Cray XT Jaguar features more than 224,000 processing cores, each with 2 gigabytes of local memory.

Jack Deslippe, acting group leader at the National Energy Research Scientific Computing Center (NERSC) covers Optimizing Codes Using the Roofline Model at the Intel Xeon Phi User's Group (IXPUG) annual meeting at Argonne.

This was the back of one of the networking panels of the sc at ANU.

A team led by P. K. Yeung, professor of aerospace engineering and mechanical engineering at the Georgia Institute of Technology, performs direct numerical simulations of turbulence using his team’s code, GPUs for Extreme-Scale Turbulence Simulations (GESTS). These simulations can accurately capture the details that arise from a wide range of scales.

 

In 2019, the team developed a new algorithm optimized for the IBM AC922 Summit supercomputer at the OLCF. With the new algorithm, the team reached a performance of less than 15 seconds of wall-clock time per time step for more than 6 trillion grid points in space—a new world record surpassing the prior state of the art in the field for the size of the problem.

 

The illustration shows intricate flow structures in turbulence from a large simulation performed using 1,024 nodes on Summit. The lower right frame shows a zoom-in view of a high-activity region.

 

Read more: www.olcf.ornl.gov/2019/11/13/a-new-parallel-strategy-for-...

 

Image Credit: Dave Pugmire and Mike Matheson, Oak Ridge National Laboratory

1 2 ••• 19 20 22 24 25 ••• 79 80