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Monday, July 13, 2020

Oak Ridge National Laboratory

From Wikipedia, the free encyclopedia
 
Oak Ridge National Laboratory
Oak Ridge National Laboratory logo.svg
Established1943
Research typeMultiprogram
Budget$1.4 billion
DirectorThomas Zacharia
Staff4,750
LocationOak Ridge, Tennessee, U.S.
35.93°N 84.31°WCoordinates: 35.93°N 84.31°W
CampusORNL occupies about 10,000 acres (40 km2) of the approximately 35,000 acres (140 km2) Oak Ridge Reservation
Operating agency
UT–Battelle
Websiteornl.gov
Map
Oak Ridge National Laboratory is located in Tennessee
Oak Ridge National Laboratory
Location in Tennessee

Oak Ridge National Laboratory (ORNL) is an American multiprogram science and technology national laboratory sponsored by the U.S. Department of Energy (DOE) and administered, managed, and operated by UT–Battelle as a federally funded research and development center (FFRDC) under a contract with the DOE. Established in 1942, ORNL is the largest science and energy national laboratory in the Department of Energy system (by size) and by annual budget. ORNL is located in Oak Ridge, Tennessee, near Knoxville. ORNL's scientific programs focus on materials, neutron science, energy, high-performance computing, systems biology and national security.

ORNL partners with the state of Tennessee, universities and industries, to solve challenges in energy, advanced materials, manufacturing, security and physics.

The laboratory has several of the world's top supercomputers; among these, Summit is ranked by the TOP500 as the world's most powerful supercomputer. The lab also is a leading neutron-science and nuclear-energy research facility that includes the Spallation Neutron Source and High Flux Isotope Reactor. ORNL hosts all of the following:

Overview

An aerial photo of the Oak Ridge National Laboratory campus.
The ORNL campus

Oak Ridge National Laboratory is managed by UT–Battelle, a limited liability partnership between the University of Tennessee and the Battelle Memorial Institute, formed in 2000 for that purpose. The annual budget is US$1.65 billion, 80% of which is from the Department of Energy; the remainder is from various sources paying for use of the facilities. As of 2012 there are 4,400 staff working at ORNL, 1,600 of whom are directly conducting research, and an additional 3,000 guest researchers annually.

There are five campuses on the Department of Energy's Oak Ridge reservation; the National Laboratory, the Y-12 National Security Complex, the East Tennessee Technology Park (formerly the Oak Ridge Gaseous Diffusion Plant), the Oak Ridge Institute for Science and Education, and the developing Oak Ridge Science and Technology Park, although the four other facilities are unrelated to the National Laboratory. The total area of the reservation 150 square kilometres (58 sq mi) of which the lab takes up 18 square kilometres (7 sq mi).

History

Workers in 1943 loading uranium slugs into the X-10 Graphite Reactor (now a National Historic Landmark)

The town of Oak Ridge was established by the Army Corps of Engineers as part of the Clinton Engineer Works in 1942 on isolated farm land as part of the Manhattan Project. During the war, advanced research for the government was managed at the site by the University of Chicago's Metallurgical Laboratory. In 1943, construction of the "Clinton Laboratories" was completed, later renamed to "Oak Ridge National Laboratory". The site was chosen for the X-10 Graphite Reactor, used to show that plutonium can be created from enriched uranium. Enrico Fermi and his colleagues developed the world's second self-sustaining nuclear reactor after Fermi's previous experiment, the Chicago Pile-1. The X-10 was the first reactor designed for continuous operation. After the end of World War II the demand for weapons-grade plutonium fell and the reactor and the laboratory's 1000 employees were no longer involved in nuclear weapons. Instead, it was used for scientific research. In 1946 the first medical isotopes were produced in the X-10 reactor, and by 1950 almost 20,000 samples had been shipped to various hospitals. As the demand for military science had fallen dramatically, the future of the lab was uncertain. Management of the lab was contracted by the US government to Monsanto; however, they withdrew in 1947. The University of Chicago re-assumed responsibility, until in December 1947, when Union Carbide and Carbon Co., which already operated two other facilities at Oak Ridge, took control of the laboratory. Alvin Weinberg was named Director of Research, ORNL, and in 1955 Director of the Laboratory.


In 1950 the Oak Ridge School of Reactor Technology was established with two courses in reactor operation and safety; almost 1000 students graduated. Much of the research performed at ORNL in the 1950s was relating to nuclear reactors as a form of energy production, both for propulsion and electricity. More reactors were built in the 1950s than in the rest of the ORNL's history combined.

Another project was the world's first light water reactor. With its principles of neutron moderation and fuel cooling by ordinary water, it is the direct ancestor of most modern nuclear power stations. The US Military funded much of its development, for nuclear-powered submarines and ships of the US Navy.

The US Army contracted portable nuclear reactors in 1953 for heat and electricity generation in remote military bases. The reactors were designed at ORNL, produced by American Locomotive Company and used in Greenland, the Panama Canal Zone and Antarctica. The United States Air Force (USAF) also contributed funding to three reactors, the lab's first computers, and its first particle accelerators. ORNL designed and tested a nuclear-powered aircraft in 1954 as a proof-of-concept for a proposed USAF fleet of long-range bombers, although it never flew.

The provision of radionuclides by X-10 for medicine grew steadily in the 1950s with more isotopes available. ORNL was the only Western source of californium-252. ORNL scientists lowered the immune systems of mice and performed the world's first successful bone marrow transplant.

In the early 1960s there was a large push at ORNL to develop nuclear-powered desalination plants, where deserts met the sea, to provide water. The project, called Water for Peace, was backed by John F. Kennedy and Lyndon B. Johnson, and presented at a 1964 United Nations conference, but increases in the cost of construction and falling public confidence in nuclear power caused the plan to fail. The Health Physics Research Reactor built in 1962 was used for radiation exposure experiments leading to more accurate dosage limits and dosimeters, and improved radiation shielding.

In 1964 the Molten-Salt Reactor Experiment began with the construction of the reactor. It was operated from 1966 until 1969 (with six months down time to move from U-235 to U-233 fuel), and proved the viability of molten salt reactors, while also producing fuel for other reactors as a byproduct of its own reaction.

The High Flux Isotope Reactor built in 1965 had the highest neutron flux of any reactor at the time. It improved upon the work of the X-10 reactor, producing more medical isotopes, as well as allowing higher fidelity of materials research.

Researchers in the Biology Division studied the effects of chemicals on mice, including petrol fumes, pesticides, and tobacco.

In the late 1960s, cuts in funding led to the cancellation of plans for another particle accelerator, and the United States Atomic Energy Commission cut the breeder reactor program by two-thirds, leading to a downsizing in staff from 5000 to 3800.

The inside of ORMAK, an early tokamak, was gold plated for reflectivity
 
In the 1970s, the prospect of fusion power was strongly considered, sparking research at ORNL. A tokamak called ORMAK, made operational in 1971, was the first tokamak to achieve a plasma temperature of 20 million Kelvin. After the success of the fusion experiments, it was enlarged and renamed ORMAK II in 1973; however, the experiments ultimately failed to lead to fusion power plants.

The US Atomic Energy Commission required improved safety standards in the early 1970s for nuclear reactors, so ORNL staff wrote almost 100 requirements covering many factors including fuel transport and earthquake resistance. In 1972 the AEC held a series of public hearings where emergency cooling requirements were highlighted and the safety requirements became more stringent.

ORNL was involved in analysing the damage to the core of the Three Mile Island Nuclear Generating Station after the accident in 1979.

Also in 1972, Peter Mazur, a biologist at ORNL, froze with liquid nitrogen, thawed and implanted mouse embryos in a surrogate mother. The mouse pups were born healthy. The technique is popular in the livestock industry, as it allows the embryos of valuable cattle to be transported easily and a prize cow can have multiple eggs extracted and thus, through in vitro fertilisation, have many more offspring than would naturally be possible.

In 1974 Alvin Weinberg, director of the lab for 19 years, was replaced by Herman Postma, a fusion scientist.

In 1977 construction began for 6 metre (20 foot) superconducting electromagnets, intended to control fusion reactions. The project was an international effort: three electromagnets were produced in the US, one in Japan, one in Switzerland and the final by remaining European states. Experimentation continued into the 1980s.

The 1980s brought more changes to ORNL: a focus on efficiency became paramount. 

An accelerated climate simulation chamber was built that applied varying weather conditions to insulation to test its efficacy and durability faster than real time. Materials research into heat resistant ceramics for use in truck and high-tech car engines was performed, building upon the materials research that began in the nuclear reactors of the 1950s. In 1987 the High Temperature Materials Laboratory was established, where ORNL and industry researchers cooperated on ceramic and alloy projects. The materials research budget at ORNL doubled after initial uncertainty regarding Reagan's economic policy of less government expenditure.

In 1981, the Holifield Heavy Ion Research Facility, a 25 MV particle accelerator, was opened at ORNL. At the time, Holifield had the widest range of ion species and was twice as powerful as other accelerators, attracting hundreds of guest researchers each year.

The Department of Energy was concerned with the pollution surrounding ORNL and it began clean-up efforts. Burial trenches and leaking pipes had contaminated the groundwater beneath the lab, and radiation tanks were sitting idle, full of waste. Estimates of the total cost of clean-up were into the hundreds of millions of US dollars.

The five older reactors were subjected to safety reviews in 1987, ordered to be deactivated until the reviews were complete. By 1989 when the High Flux Isotope Reactor was restarted the US supply of certain medical isotopes was depleted.

In 1989 the former executive officer of the American Association for the Advancement of Science, Alvin Trivelpiece, became director of ORNL; he remained in the role until 2000.

In 1992, a whistleblower, Charles Varnadore, filed complaints against ORNL, alleging safety violations and retaliation by his superiors. While an administrative law judge ruled in Varnadore's favor, the Secretary of Labor, Robert Reich, overturned that ruling. However, Varnadore's case saw prime contractor Martin Marietta cited for safety violations, and ultimately led to additional whistleblower protection within DOE.

In January 2019 ORNL announced a major breakthrough in its capacity to automate Pu-238 production which helped push annual production from 50 grams to 400 grams, moving closer to NASA's goal of 1.5 kilograms per year by 2025 in order to sustain its space exploration programs.

Areas of research

ORNL conducts research and development activities that span a wide range of scientific disciplines. Many research areas have a significant overlap with each other; researchers often work in two or more of the fields listed here. The laboratory's major research areas are described briefly below.
  • Chemical sciences – ORNL conducts both fundamental and applied research in a number of areas, including catalysis, surface science and interfacial chemistry; molecular transformations and fuel chemistry; heavy element chemistry and radioactive materials characterization; aqueous solution chemistry and geochemistry; mass spectrometry and laser spectroscopy; separations chemistry; materials chemistry including synthesis and characterization of polymers and other soft materials; chemical biosciences; and neutron science.
  • Electron microscopy – ORNL's electron microscopy program investigates key issues in condensed matter, materials, chemical and nanosciences.
  • Nuclear medicine – The laboratory's nuclear medicine research is focused on the development of improved reactor production and processing methods to provide medical radioisotopes, the development of new radionuclide generator systems, the design and evaluation of new radiopharmaceuticals for applications in nuclear medicine and oncology.
  • Physics – Physics research at ORNL is focused primarily on studies of the fundamental properties of matter at the atomic, nuclear, and subnuclear levels and the development of experimental devices in support of these studies.
  • Population – ORNL provides federal, state and international organizations with a gridded population database, called Landscan, for estimating ambient population. LandScan is a raster image, or grid, of population counts, which provides human population estimates every 30 x 30 arc seconds, which translates roughly to population estimates for 1 kilometer square windows or grid cells at the equator, with cell width decreasing at higher latitudes. Though many population datasets exist, LandScan is the best spatial population dataset, which also covers the globe. Updated annually (although data releases are generally one year behind the current year) offers continuous, updated values of population, based on the most recent information. Landscan data are accessible through GIS applications and a USAID public domain application called Population Explorer.

Energy

The laboratory has a long history of energy research; nuclear reactor experiments have been conducted since the end of World War II in 1945. Because of the availability of reactors and high-performance computing resources an emphasis on improving the efficiency of nuclear reactors is present. The programs develop more efficient materials, more accurate simulations of aging reactor cores, sensors and controls as well as safety procedures for regulatory authorities.

The Energy Efficiency and Electricity Technologies Program (EEETP) aims to improve air quality in the US and reduce dependence on foreign oil supplies. There are three key areas of research; electricity, manufacturing and mobility. The electricity division focuses on reducing electricity consumption and finding alternative sources for production. Buildings, which account for 39% of US electricity consumption as of 2012, are a key area of research as the program aims to create affordable, carbon-neutral homes by 2020. Research also takes place into higher efficiency solar panels, geothermal electricity and heating, lower cost wind generators and the economic and environmental feasibility of potential hydro power plants.

Fusion is another area with a history of research at ORNL, dating back to the 1970s. The Fusion Energy Division pursues short-term goals to develop components such as high temperature superconductors, high-speed hydrogen pellet injectors and suitable materials for future fusion research. Much research into the behaviour and maintenance of a plasma takes place at the Fusion Energy Division to further the understanding of plasma physics, a crucial area for developing a fusion power plant. The US ITER office is at ORNL with partners at Princeton Plasma Physics Laboratory and Savannah River National Laboratory. The US contribution to the ITER project is 9.1% which is expected to be in excess of US$1.6 billion throughout the contract.[33][34]

Biology

A simulation of CelS, a type of Cellobiohydrolase that hydrolyzes the glycosidic bonds of cellulose (cellulolysis)
 
Oak Ridge National Laboratory's biological research covers genomics, computational biology, structural biology and bioinformatics. The BioEnergy Program aims to improve the efficiency of all stages of the biofuel process to improve the energy security of the United States. The program aims to make genetic improvements to the potential biomass used, formulate methods for refineries that can accept a diverse range of fuels and to improve the efficiency of energy delivery both to power plants and end users.

The Center for Molecular Biophysics conducts research into the behaviour of biological molecules in various conditions. The center hosts projects that examine cell walls for biofuel production, use neutron scattering to analyse protein folding and simulate the effect of catalysis on a conventional and quantum scale.

Neutron science

There are three neutron sources at ORNL; the High Flux Isotope Reactor (HFIR), the Oak Ridge Electron Linear Accelerator (ORELA) and the Spallation Neutron Source. HFIR provides neutrons in a stable beam resulting from a constant nuclear reaction whereas ORELA and SNS produce pulses of neutrons as they are particle accelerators. HFIR went critical in 1965 and has been used for materials research and as a major source of medical radioisotopes since. As of 2013, HFIR provides the world's highest constant neutron flux as a result of various upgrades. As part of a US non-proliferation effort the HFIR is scheduled to switch from highly enriched uranium (>90%, weapons grade) to low-enriched (3–4%) in 2020; the last reactor in the US to do so. Berkelium used to produce the world's first sample of tennessine was produced in the High Flux Isotope Reactor as part of an international effort. HFIR is likely to operate until approximately 2060 before the reactor vessel is considered unsafe for continued use.

The Spallation Neutron Source (SNS) is a particle accelerator that has the highest intensity neutron pulses of any man-made neutron source. SNS was made operational in 2006 and has since been upgraded to 1 megawatts with plans to continue up to 3 megawatts. High power neutron pulses permit clearer images of the targets meaning smaller samples can be analysed and accurate results require fewer pulses.

Materials

A particulate filter housing for a regenerative burner made of CF8C Plus stainless steel

Oak Ridge National Laboratory conducts research into materials science in a range of areas. Between 2002 and 2008 ORNL partnered with Caterpillar Inc. (CAT) to form a new material for their diesel engines that can withstand large temperature fluctuations. The new steel, named CF8C Plus, is based on conventional CF8C stainless steel with added manganese and nitrogen; the result has better high–temperature properties and is easier to cast at a similar cost. In 2003 the partners received an R&D 100 award from R&D magazine and in 2009 received an award for "excellence in technology transfer" from the Federal Laboratory Consortium for the commercialisation of the steel.

There is a high-temperature materials lab at ORNL that permits researchers from universities, private companies and other government initiatives to use their facilities. The lab is available for free if the results are published; private research is permitted but requires payment. A separate lab, the Shared Equipment User Facility, is one of three DOE sponsored facilities with nano-scale microscopy and tomography facilities.

The Center for Nanophase Materials Sciences (CNMS) researches the behaviour and fabrication of nanomaterials. The center emphasises discovery of new materials and the understanding of underlying physical and chemical interactions that enable creation of nanomaterials. In 2012, CNMS produced a lithium-sulfide battery with a theoretical energy density three to five times greater than existing lithium ion batteries.

Security

Oak Ridge National Laboratory provides resources to the US Department of Homeland Security and other defense programs. The Global Security and Nonproliferation (GS&N) program develops and implements policies, both US based and international, to prevent the proliferation of nuclear material. The program has developed safeguards for nuclear arsenals, guidelines for dismantling arsenals, plans of action should nuclear material fall into unauthorised hands, detection methods for stolen or missing nuclear material and trade of nuclear material between the US and Russia. The GS&N's work overlaps with that of the Homeland Security Programs Office, providing detection of nuclear material and nonproliferation guidelines. Other areas concerning the Department Homeland Security include nuclear and radiological forensics, chemical and biological agent detection using mass spectrometry and simulations of potential national hazards.

High-performance computing

Throughout the history of the Oak Ridge National Laboratory it has been the site of various supercomputers, home to the fastest on several occasions. In 1953, ORNL partnered with the Argonne National Laboratory to build ORACLE (Oak Ridge Automatic Computer and Logical Engine), a computer to research nuclear physics, chemistry, biology and engineering. ORACLE had 2048 words (80 Kibit) of memory and took approximately 590 microseconds to perform addition or multiplications of integers. In the 1960s ORNL was also equipped with an IBM 360/91 and an IBM 360/65. In 1995 ORNL bought an Intel Paragon based computer called the Intel Paragon XP/S 150 that performed at 154 gigaFLOPS and ranked third on the TOP500 list of supercomputers. In 2005 Jaguar was built, a Cray XT3-based system that performed at 25 teraFLOPS and received incremental upgrades up to the XT5 platform that performed at 2.3 petaFLOPS in 2009. It was recognised as the world's fastest from November 2009 until November 2010. Summit was built for Oak Ridge National Laboratory during 2018, which benchedmarked at 122.3 petaflops. As of June 2018, Summit stands as the world's fasted [clocked] supercomputer with 202,752 CPU cores, 27,648 Nvidia Tesla GPUs and 250 Petabytes of storage.

Since 1992 the National Center for Computational Sciences (NCCS) has overseen high performance computing at ORNL. It manages the Oak Ridge Leadership Computing Facility that contains the machines. In 2012, Jaguar was upgraded to the XK7 platform, a fundamental change as GPUs are used for the majority of processing, and renamed Titan. Titan performs at 17.59 petaFLOPS and holds the number 1 spot on the TOP500 list for November 2012. Other computers include a 77 node cluster to visualise data that the larger machines output in the Exploratory Visualization Environment for Research in Science and Technology (EVEREST), a visualisation room with a 10 by 3 metre (30 by 10 ft) wall that displays 35 megapixel projections. Smoky is an 80 node linux cluster used for application development. Research projects are refined and tested on Smoky before running on larger machines such as Titan.

In 1989 programmers at the Oak Ridge National Lab wrote the first version of Parallel Virtual Machine (PVM), software that enables distributed computing on machines of differing specifications. PVM is free software and has become the de facto standard for distributed computing. Jack Dongarra of ORNL and the University of Tennessee wrote the LINPACK software library and LINPACK benchmarks, used to calculate linear algebra and the standard method of measuring floating point performance of a supercomputer as used by the TOP500 organisation.

Lawrence Berkeley National Laboratory

From Wikipedia, the free encyclopedia
 
 
Lawrence Berkeley National Laboratory
Molecular Foundry Berkeley.jpg
MottoBringing science solutions to the world
EstablishedAugust 26, 1931
(89 years ago)
Research typescientific research and energy technologies
Budget$803 million (2016)
DirectorMichael Witherell
Staff3,816
Students800
LocationBerkeley, California, United States
Campus200 acres (81 ha)
Operating agency
University of California
13
Websitelbl.gov

The Lawrence Berkeley National Laboratory (LBNL), commonly referred to as Berkeley Lab, is a United States national laboratory that conducts scientific research on behalf of the Department of Energy. Located in the hills of Berkeley, California, the lab overlooks the campus of the University of California, Berkeley.

History

1931–1941

The laboratory was founded in August 26, 1931, by Ernest Lawrence, as the Radiation Laboratory of the University of California, Berkeley, associated with the Physics Department. It centered physics research around his new instrument, the cyclotron, a type of particle accelerator for which he was awarded the Nobel Prize in Physics in 1939. Throughout the 1930s, Lawrence pushed to create larger and larger machines for physics research, courting private philanthropists for funding. He was the first to develop a large team to build big projects to make discoveries in basic research. Eventually these machines grew too large to be held on the university grounds, and in 1940 the lab moved to its current site atop the hill above campus. Part of the team put together during this period includes two other young scientists who went on to establish large laboratories; J. Robert Oppenheimer founded Los Alamos Laboratory, and Robert Wilson founded Fermilab.

1942–1950

Leslie Groves visited Lawrence's Radiation Laboratory in late 1942 as he was organizing the Manhattan Project, meeting J. Robert Oppenheimer for the first time. Oppenheimer was tasked with organizing the nuclear bomb development effort and founded today's Los Alamos National Laboratory to help keep the work secret. At the RadLab, Lawrence and his colleagues developed the technique of electromagnetic enrichment of uranium using their experience with cyclotrons. The calutrons (named after the University) became the basic unit of the massive Y-12 facility in Oak Ridge, Tennessee. Lawrence's lab helped contribute to what have been judged to be the three most valuable technology developments of the war (the atomic bomb, proximity fuse, and radar). The cyclotron, whose construction was stalled during the war, was finished in November 1946. The Manhattan Project shut down two months later.

1951–2018

After the war, the Radiation Laboratory became one of the first laboratories to be incorporated into the Atomic Energy Commission (AEC) (now Department of Energy, DOE). The most highly classified work remained at Los Alamos, but the RadLab remained involved. Edward Teller suggested setting up a second lab similar to Los Alamos to compete with their designs. This led to the creation of an offshoot of the RadLab (now the Lawrence Livermore National Laboratory) in 1952. Some of the RadLab's work was transferred to the new lab, but some classified research continued at Berkeley Lab until the 1970s, when it became a laboratory dedicated only to unclassified scientific research.

Shortly after the death of Lawrence in August 1958, the UC Radiation Laboratory (both branches) was renamed the Lawrence Radiation Laboratory. The Berkeley location became the Lawrence Berkeley Laboratory in 1971, although many continued to call it the RadLab. Gradually, another shortened form came into common usage, LBL. Its formal name was amended to Ernest Orlando Lawrence Berkeley National Laboratory in 1995, when "National" was added to the names of all DOE labs. "Ernest Orlando" was later dropped to shorten the name. Today, the lab is commonly referred to as Berkeley Lab.

The Alvarez Physics Memos are a set of informal working papers of the large group of physicists, engineers, computer programmers, and technicians led by Luis W. Alvarez from the early 1950s until his death in 1988. Over 1700 memos are available on-line, hosted by the Laboratory.

In 2018, the lab remains owned by the U.S. Department of Energy, with management from the University of California. Companies such as Intel were funding the lab's research into computing chips.

University of California Radiation Laboratory staff on the magnet yoke for the 60-inch cyclotron, 1938; Nobel prizewinners Ernest Lawrence, Edwin McMillan, and Luis Alvarez are shown, in addition to J. Robert Oppenheimer and Robert R. Wilson.

Laboratory directors

Science mission

From the 1950s through the present, Berkeley Lab has maintained its status as a major international center for physics research, and has also diversified its research program into almost every realm of scientific investigation. Its mission is to solve the most pressing and profound scientific problems facing humanity, conduct basic research for a secure energy future, understand living systems to improve the environment, health, and energy supply, understand matter and energy in the universe, build and safely operate leading scientific facilities for the nation, and train the next generation of scientists and engineers.

The Laboratory's 20 scientific divisions are organized within six areas of research: Computing Sciences, Physical Sciences, Earth and Environmental Sciences, Biosciences, Energy Sciences, and Energy Technologies. Berkeley Lab has six main science thrusts: advancing integrated fundamental energy science, integrative biological and environmental system science, advanced computing for science impact, discovering the fundamental properties of matter and energy, accelerators for the future, and developing energy technology innovations for a sustainable future. It was Lawrence's belief that scientific research is best done through teams of individuals with different fields of expertise, working together. His teamwork concept is a Berkeley Lab tradition that continues today.
Berkeley Lab operates five major National User Facilities for the DOE Office of Science:
  1. The Advanced Light Source (ALS) is a synchrotron light source with 41 beam lines providing ultraviolet, soft x-ray, and hard x-ray light to scientific experiments. The ALS is one of the world's brightest sources of soft x-rays, which are used to characterize the electronic structure of matter and to reveal microscopic structures with elemental and chemical specificity. About 2,500 scientist-users carry out research at ALS every year. Berkeley Lab is proposing an upgrade of ALS which would increase the coherent flux of soft x-rays by two-three orders of magnitude.
  2. The Joint Genome Institute (JGI) supports genomic research in support of the DOE missions in alternative energy, global carbon cycling, and environmental management. The JGI's partner laboratories are Berkeley Lab, Lawrence Livermore National Lab (LLNL), Oak Ridge National Laboratory (ORNL), Pacific Northwest National Laboratory (PNNL), and the HudsonAlpha Institute for Biotechnology. The JGI's central role is the development of a diversity of large-scale experimental and computational capabilities to link sequence to biological insights relevant to energy and environmental research. Approximately 1,200 scientist-users take advantage of JGI's capabilities for their research every year.
  3. The Molecular Foundry is a multidisciplinary nanoscience research facility. Its seven research facilities focus on Imaging and Manipulation of Nanostructures, Nanofabrication, Theory of Nanostructured Materials, Inorganic Nanostructures, Biological Nanostructures, Organic and Macromolecular Synthesis, and Electron Microscopy. Approximately 700 scientist-users make use of these facilities in their research every year.
  4. The National Energy Research Scientific Computing Center (NERSC) is the scientific computing facility that provides large-scale computing for the DOE's unclassified research programs. Its current systems provide over 3 billion computational hours annually. NERSC supports 6,000 scientific users from universities, national laboratories, and industry.
  5. The Energy Sciences Network (ESnet) is a high-speed network infrastructure optimized for very large scientific data flows. ESNet provides connectivity for all major DOE sites and facilities, and the network transports roughly 35 petabytes of traffic each month.
Berkeley Lab is the lead partner in the Joint BioEnergy Institute (JBEI), located in Emeryville, California. Other partners are the Sandia National Laboratories, the University of California (UC) campuses of Berkeley and Davis, the Carnegie Institution for Science, and Lawrence Livermore National Laboratory (LLNL). JBEI's primary scientific mission is to advance the development of the next generation of biofuels – liquid fuels derived from the solar energy stored in plant biomass. JBEI is one of three new U.S. Department of Energy (DOE) Bioenergy Research Centers (BRCs).

Berkeley Lab has a major role in two DOE Energy Innovation Hubs. The mission of the Joint Center for Artificial Photosynthesis (JCAP) is to find a cost-effective method to produce fuels using only sunlight, water, and carbon dioxide. The lead institution for JCAP is the California Institute of Technology and Berkeley Lab is the second institutional center. The mission of the Joint Center for Energy Storage Research (JCESR) is to create next-generation battery technologies that will transform transportation and the electricity grid. Argonne National Laboratory leads JCESR and Berkeley Lab is a major partner.

Operations and governance

The University of California operates Lawrence Berkeley National Laboratory under a contract with the Department of Energy. The site consists of 76 buildings (owned by the U.S. Department of Energy) located on 200 acres (0.81 km2) owned by the university in the Berkeley Hills. Altogether, the Lab has some 4,000 UC employees, of whom about 800 are students or postdocs, and each year it hosts more than 3,000 participating guest scientists. There are approximately two dozen DOE employees stationed at the laboratory to provide federal oversight of Berkeley Lab's work for the DOE. The laboratory director, Michael Witherell, is appointed by the university regents and reports to the university president. Although Berkeley Lab is governed by UC independently of the Berkeley campus, the two entities are closely interconnected: more than 200 Berkeley Lab researchers hold joint appointments as UC Berkeley faculty.

The Lab's budget for the fiscal year 2019 was 1.1 billion dollars.

Scientific achievements, inventions, and discoveries

Notable scientific accomplishments at the Lab since World War II include the observation of the antiproton, the discovery of several transuranic elements, and the discovery of the accelerating universe


Seventy Berkeley Lab scientists are members of the U.S. National Academy of Sciences (NAS), one of the highest honors for a scientist in the United States. Thirteen Berkeley Lab scientists have won the National Medal of Science, the nation's highest award for lifetime achievement in fields of scientific research. Eighteen Berkeley Lab engineers have been elected to the National Academy of Engineering, and three Berkeley Lab scientists have been elected into the National Academy of Medicine. Nature Index rates the Lab sixth in the world among government research organizations; it is the only one of the top six that is a single laboratory, rather than a system of laboratories. 

Elements discovered by Berkeley Lab physicists include astatine, neptunium, plutonium, curium, americium, berkelium*, californium*, einsteinium, fermium, mendelevium, nobelium, lawrencium*, dubnium, and seaborgium*. Those elements listed with asterisks (*) are named after the University Professors Lawrence and Seaborg. Seaborg was the principal scientist involved in their discovery. The element technetium was discovered after Ernest Lawrence gave Emilio Segrè a molybdenum strip from the Berkeley Lab cyclotron. The fabricated evidence used to claim the creation of oganesson and livermorium by Victor Ninov, a researcher employed at Berkeley Lab, led to the retraction of two articles.

Inventions and discoveries to come out of Berkeley Lab include: "smart" windows with embedded electrodes that enable window glass to respond to changes in sunlight, synthetic genes for antimalaria and anti-AIDS superdrugs based on breakthroughs in synthetic biology, electronic ballasts for more efficient lighting, Home Energy Saver, the web's first do-it-yourself home energy audit tool, a pocket-sized DNA sampler called the PhyloChip, and the Berkeley Darfur Stove, which uses one-quarter as much firewood as traditional cook stoves. One of Berkeley Lab's most notable breakthroughs is the discovery of dark energy. During the 1980s and 1990s Berkeley Lab physicists and astronomers formed the Supernova Cosmology Project (SCP), using Type Ia supernovae as "standard candles" to measure the expansion rate of the universe. Their successful methods inspired competition, with the result that early in 1998 both the SCP and the High-Z Supernova Search Team announced the surprising discovery that expansion is accelerating; the cause was soon named dark energy.

Arthur Rosenfeld, a senior scientist at Berkeley Lab, was the nation's leading advocate for energy efficiency from 1975 until his death in 2017. He led efforts at the Lab that produced several technologies that radically improved efficiency: compact fluorescent lamps, low-energy refrigerators, and windows that trap heat. He established the Center for Building Science at the Lab, which developed into the Building Technology and Urban Systems Division. He developed the first energy-efficiency standards for buildings and appliances in California, which helped the state to sustain constant electricity use per capita, a phenomenon called the Rosenfeld effect. The Energy Efficiency and Environmental Impacts Division continues to set the research foundation for the national energy efficiency standards and works with China, India, and other countries to help develop their standards.

Carl Haber and Vitaliy Fadeyev of Berkeley Lab developed the IRENE system for optical scanning of audio discs and cylinders.

In December 2018, researchers at Intel Corp. and the Lawrence Berkeley National Laboratory published a paper in Nature, which outlined a chip "made with quantum materials called magnetoelectric multiferroics instead of the conventional silicon," to allow for increased processing and reduced energy consumption to support technology such as artificial intelligence.

South African Astronomical Observatory

From Wikipedia, the free encyclopedia
 
South African Astronomical Observatory
South African Astronomical Observatory (sutherland aerial view).jpg
The Sutherland site of the South African Astronomical Observatory. With the Southern African Large Telescope.
Alternative namesSAAO Edit this on Wikidata
OrganizationNational Research Foundation of South Africa
Observatory code51, B31, A60
LocationHeadquarters in Observatory, Cape Town
Major telescopes in Sutherland, Northern Cape
CoordinatesHeadquarters: 33.9347°S 18.4776°ECoordinates: 33.9347°S 18.4776°E
Sutherland: 32.3783°S 20.8105°E
EstablishedJanuary 1972
Websitewww.saao.ac.za
Telescopes
SALT11m reflector
1.9m1.9m reflector
Infrared Survey Facility1.4m reflector
MONET1.2m reflector
1.0m1m reflector
SuperWASP-South8x Canon 200mm f/1.8
ACT75 cm reflector
Solaris-10.5m f/15 Ritchey–Chrétien
Solaris-10.5m f/15 Ritchey–Chrétien
South African Astronomical Observatory is located in South Africa
South African Astronomical Observatory
Location of South African Astronomical Observatory

South African Astronomical Observatory (SAAO) is the national centre for optical and infrared astronomy in South Africa. It was established in 1972. The observatory is run by the National Research Foundation of South Africa. The facility's function is to conduct research in astronomy and astrophysics. The primary telescopes are located in Sutherland, which is 370 kilometres (230 mi) from Observatory, Cape Town, where the headquarters is located.

The SAAO has links worldwide for scientific and technological collaboration. Instrumental contributions from the South African Astronomical Observatory include the development of a spherical aberration corrector and the Southern African Large Telescope (SALT).

The Noon Gun on Cape Town's Signal Hill is fired remotely by a time signal from the Observatory.

History

The buildings of the South African Astronomical Observatory in Cape Town.

The history of the SAAO began when the Royal Observatory at the Cape of Good Hope was founded in 1820, the first scientific institution in Africa. Construction of the main buildings was completed in 1829 at a cost of £30,000 (equivalent to £2.7 million in 2020). The post of Her Majesty's astronomer at the Cape of Good Hope was awarded the Royal Medal on two occasions; the first to Thomas Maclear in 1869 for measurement of an arc of the meridian at the Cape of Good Hope and the second to David Gill in 1903 for researches in solar and stellar parallax, and his energetic direction of the Royal Observatory at the Cape of Good Hope.

The Republic Observatory, Johannesburg, was merged with the much older Royal Observatory, Cape of Good Hope in January 1972 to form the South African Astronomical Observatory. In 1974 the Radcliffe Observatory telescope was purchased by the CSIR and moved to Sutherland, where it recommenced work in 1976.

SAAO was established in January 1972, as a result of a joint agreement by the Council for Scientific and Industrial Research (CSIR) of South Africa and Science and Engineering Research Council (SERC) of United Kingdom. The headquarters are located on the grounds of the old Royal Observatory where the main building, offices, national library for astronomy and computer facilities are housed. Historic telescopes are also found at the headquarters in a number of domes and a small museum that displays scientific instruments. The South African Astronomical Observatory is administered at present as a National Facility under management of the National Research Foundation (NRF), formerly the Foundation for Research Development (FRD). In 1974, when the Radcliffe Observatory in Pretoria closed, the Council for Scientific and Industrial Research (CSIR) purchased the 1.9-m Radcliffe telescope and transported it to Sutherland.

Facilities

Sign at the entrance to Sutherland Observatory near Sutherland, Northern Cape
 
The observatory operates from the campus of the Royal Observatory, Cape of Good Hope that was established in 1820 in the suburb of Observatory, Cape Town.

The major observing facilities are however located near the town of Sutherland some 370 kilometres (230 mi) from Cape Town.

Telescopes

Two telescope domes at the South African Astronomical Observatory

0.50m telescope

This 0.5 metres (20 in) reflector was originally built for the Republic Observatory in 1967, but was moved to the Sutherland site in 1972.

0.75m telescope

A 0.75 metres (30 in) Grubb Parsons reflector.

1.0m Telescope

The 40-inch (1-m) Elizabeth Telescope at the South African Astronomical Observatory

This 40 inches (1.0 m) telescope was originally located at SAAO Head office in Observatory, Cape Town, but has since moved to the Sutherland site. This telescope participates in the PLANET network.

1.9m Telescope

The 74" Reflector
The 1.9-m (74-inch) Radcliffe Telescope was commissioned for the Radcliffe Observatory in Pretoria where it was in use between 1948 and 1974. Following the closure of the Radcliffe Observatory it was moved to Sutherland where it became operational again in January 1976. Between 1951 and 2004 it was the largest telescope in South Africa. The telescope was manufactured by Sir Howard Grubb, Parsons and Co.

Alan Cousins Telescope (ACT)

This 29.5 inches (75 cm) telescope was originally called the Automatic Photometric Telescope, but has been renamed the Alan Cousins Telescope in honour of Alan William James Cousins.

BiSON

One of six telescopes in the Birmingham Solar Oscillations Network

Infrared Survey Facility (IRSF)

The IRSF is a 140 centimetres (55 in) reflector fitted with a 3 colour Infrared Imager. Originally built as part of the Magellanic Clouds – A Thorough Study grant from the Japanese Ministry of Education, Culture, Sports, Science and Technology in 2000. Other studies the telescope participated in include:

Las Cumbres Observatory Global Telescope Network

Three 1 metre (39 in) telescopes to form part of the LCOGT network were installed in early 2013.

MASTER

The MASTER-SAAO Telescope (obs. code: K95) is part of the Russian Mobile Astronomical System of Telescope-Robots. It saw first light on 21 December 2014. It consists of two paired 0.4-m telescopes. In April 2015 it discovered the first comet from South Africa in 35 years, C/2015 G2 (MASTER).

MONET

One of the two 1.20 metres (47 in) telescopes of the MOnitoring NEtwork of Telescopes Project is located at Sutherland. Its twin can be found at the McDonald Observatory in Texas. The MONET telescopes are Robotic telescope controllable via the Internet and was constructed by the University of Göttingen. Remote Telescope Markup Language is used to control the telescopes remotely.

Project Solaris

Solaris-1 and Solaris-2
 
Two telescopes forming part of Project Solaris is located at the Sutherland site. Solaris-1 and Solaris-2 are both 0.5m f/15 Ritchey–Chrétien telescope. The aims of Project Solaris is to detect circumbinary planets around eclipsing binary stars and to characterise these binaries to improve stellar models.

SALT

Southern African Large Telescope (SALT)

SALT was inaugurated in November 2005. It is the largest single optical telescope in the Southern Hemisphere, with a hexagonal mirror array 11 meters across. SALT shares similarities with the Hobby-Eberly Telescope (HET) in Texas. The Southern African Large Telescope gathers twenty-five times as much light as any other existing African Telescope. With this larger mirror array, SALT can record distant stars, galaxies and quasars.

SuperWASP-South

SuperWASP-South

The Wide Angle Search for Planets consists of two robotic telescopes, the one located at SAAO Sutherland and the other at Roque de los Muchachos Observatory on the island of La Palma in the Canaries. WASP-17b, the first exoplanet known to have a retrograde orbit was discovered in 2009 using this array.

KELT-South

KELT-South (Kilodegree Extremely Little Telescope – South) is a small robotic telescope that is designed to detect transiting extrasolar planets. The telescope is owned and operated by Vanderbilt University and was based on the design of KELT-North, which was conceived and designed at the Ohio State University, Department of Astronomy. The KELT-South telescope will serve as a counterpart to its northern twin, surveying the southern sky for transiting planets over the next few years.

Yonsei Survey Telescopes for Astronomical Research (YSTAR)

The Yonsei Survey Telescopes for Astronomical Research (YSTAR), decommissioned in 2012, was used for the monitoring of variable stars and other transient events. YSTAR was a joint project between SAAO and the Yonsei University, Korea.

Geophysical

South African Geodynamic Observatory Sutherland (SAGOS)

The GeoForschungsZentrum, Potsdam in co-operation with the National Research Foundation of South Africa constructed the SAGOS between 1998 and 2000.

SAGOS consist of a 1 Hz permanent GPS station, a superconducting gravimeter, meteorological sensors, and a tri-axial magnetometer. The GPS station is also used in support of the CHAllenging Minisatellite Payload (CHAMP) and Gravity Recovery and Climate Experiment (GRACE) space missions.

SUR Station

Biodiversity loss

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