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	<title>usa &#8211; EPICS Controls</title>
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	<title>usa &#8211; EPICS Controls</title>
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		<title>Advanced Light Source (ALS) at Lawrence Berkeley National Laboratory</title>
		<link>https://epics-controls.org/projects-archive/advanced-light-source-als-at-lawrence-berkeley-national-laboratory/</link>
		
		<dc:creator><![CDATA[Han]]></dc:creator>
		<pubDate>Wed, 05 Jul 2023 11:25:54 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=21803</guid>

					<description><![CDATA[<p>The <a href="https://als.lbl.gov/">Advanced Light Source (ALS)</a> is a third-generation synchrotron light source at <a href="https://www.lbl.gov/">Lawrence Berkeley National Laboratory</a>. Built in 1993, the ALS serves over 40 beamlines and is one of the world&#8217;s brightest ultraviolet and soft X-ray light sources. The 196.8-meter circumference storage ring has an electron beam energy of 1.9 GeV. It supports [...]]]></description>
										<content:encoded><![CDATA[<p><span class="im">The <a href="https://als.lbl.gov/">Advanced Light Source (ALS)</a> is a third-generation synchrotron light source at <a href="https://www.lbl.gov/">Lawrence Berkeley National Laboratory</a>. Built in 1993, the ALS serves over 40 beamlines and is one of the world&#8217;s brightest ultraviolet and soft X-ray light sources. The 196.8-meter circumference storage ring has an electron beam energy of 1.9 GeV. It supports experiments across various fields, including materials science, biology, chemistry, physics, and the environmental sciences. The ALS is upgrading to become a fourth-generation light source, adding a new accumulator ring and replacing the existing storage ring—the U.S. Department of Energy, Office of Science, Basic Energy Sciences program funds the ALS operation and its upgrade project.<br />
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		<title>STAR Detector at RHIC</title>
		<link>https://epics-controls.org/projects-archive/star/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Tue, 21 May 2019 11:00:31 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=4610</guid>

					<description><![CDATA[<p>The <a href="https://www.bnl.gov/rhic/STAR.asp">STAR detector</a> at Brookhaven National Lab specializes in tracking the thousands of particles produced by each ion collision at the Relativistic Heavy Ion Collider (RHIC).</p>
<p>Weighing 1,200 tons and as large as a house, STAR consists mainly of 12 subsystems. It is used to search for signatures of the form of matter that RHIC was [...]]]></description>
										<content:encoded><![CDATA[<p>The <a href="https://www.bnl.gov/rhic/STAR.asp">STAR detector</a> at Brookhaven National Lab specializes in tracking the thousands of particles produced by each ion collision at the Relativistic Heavy Ion Collider (RHIC).</p>
<p>Weighing 1,200 tons and as large as a house, STAR consists mainly of 12 subsystems. It is used to search for signatures of the form of matter that RHIC was designed to create: the quark-gluon plasma (QGP).</p>
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		<title>W. M. Keck Observatory</title>
		<link>https://epics-controls.org/projects-archive/keck-observatory/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Wed, 19 Sep 2018 07:13:18 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=3400</guid>

					<description><![CDATA[<p>From atop Maunakea on the Island of Hawaii, astronomers around the world use <a href="http://www.keckobservatory.org">W. M. Keck Observatory</a> to observe the universe with unprecedented power and precision.</p>
<p>The twin Keck Observatory telescopes are the most scientifically productive optical and infrared telescopes on Earth and operate with nanometer precision. The telescopes’ primary mirrors are 10-meters in diameter [...]]]></description>
										<content:encoded><![CDATA[<p>From atop Maunakea on the Island of Hawaii, astronomers around the world use <a href="http://www.keckobservatory.org">W. M. Keck Observatory</a> to observe the universe with unprecedented power and precision.</p>
<p>The twin Keck Observatory telescopes are the most scientifically productive optical and infrared telescopes on Earth and operate with nanometer precision. The telescopes’ primary mirrors are 10-meters in diameter and are each composed of 36 hexagonal segments that work in concert as a single piece of reflective glass. Both telescopes feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrometers, and world-leading laser guide star adaptive optics systems.</p>
<p>Keck Observatory is a private 501(c) 3 non-profit organization operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.</p>
<p>For more information, visit <a href="http://www.keckobservatory.org">www.keckobservatory.org</a></p>
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		<title>Facility for Rare Isotope Beams (FRIB)</title>
		<link>https://epics-controls.org/projects-archive/frib/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Mon, 17 Sep 2018 11:21:09 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=3357</guid>

					<description><![CDATA[<p>Michigan State University (MSU) is establishing the <a href="https://frib.msu.edu/">Facility for Rare Isotope Beams (FRIB)</a> as a scientific user facility for the Office of Nuclear Physics in the U.S. Department of Energy Office of Science (DOESC). FRIB is funded by the DOE-SC, MSU and the State of Michigan.</p>
<p>The heart of FRIB is a high-power superconducting linear [...]]]></description>
										<content:encoded><![CDATA[<p>Michigan State University (MSU) is establishing the <a href="https://frib.msu.edu/">Facility for Rare Isotope Beams (FRIB)</a> as a scientific user facility for the Office of Nuclear Physics in the U.S. Department of Energy Office of Science (DOESC). FRIB is funded by the DOE-SC, MSU and the State of Michigan.</p>
<p>The heart of FRIB is a high-power superconducting linear accelerator that accelerates heavy ions and produces rare isotopes (short-lived nuclei not normally found on Earth) by in-beam fragmentation. FRIB will enable scientific research with fast, stopped, and reaccelerated rare isotope beams, supporting a community of currently approximately 1400 scientists from around the world.</p>
<p>FRIB will enable scientists to make discoveries advancing our knowledge of the physics of atomic nuclei, nuclear astrophysics, fundamental interactions, and practical applications of rare isotopes benefiting society in fields such as medicine, materials science, national security, and industry.</p>
<p>Learn more at <a href="https://frib.msu.edu">frib.msu.edu</a>.</p>
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		<title>SLAC National Accelerator Laboratory</title>
		<link>https://epics-controls.org/projects-archive/slac/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Wed, 24 Jan 2018 12:52:28 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=1025</guid>

					<description><![CDATA[<p><a href="https://www.slac.stanford.edu/">SLAC</a> is a scientific research center with a broad program in accelerator physics, astrophysics, atomic and solid-state physics, chemistry, biology, and medicine.</p>
<p>We concentrate on building and using large particle accelerators to probe the nature of molecules using X-ray light. We are also involved in experimental and theoretical research in elementary particle physics, astrophysics, and [...]]]></description>
										<content:encoded><![CDATA[<p><a href="https://www.slac.stanford.edu/">SLAC</a> is a scientific research center with a broad program in accelerator physics, astrophysics, atomic and solid-state physics, chemistry, biology, and medicine.</p>
<p>We concentrate on building and using large particle accelerators to probe the nature of molecules using X-ray light. We are also involved in experimental and theoretical research in elementary particle physics, astrophysics, and cosmology.</p>
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		<title>East Asian Observatory (JCMT, UKIRT)</title>
		<link>https://epics-controls.org/projects-archive/eao/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Sat, 18 Nov 2017 14:00:08 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=990</guid>

					<description><![CDATA[<p>The <a href="http://www.eaobservatory.org/">EAO (East Asian Observatory)</a> is formed by <a href="https://www.eacoa.net/">EACOA (East Asian Core Observatories Association)</a> for the purpose of pursuing joint projects in astronomy within the East Asian region. In the era of very large scale astronomical instruments, East Asia will be competitive internationally by combining their funding resources, their technical expertise, and their [...]]]></description>
										<content:encoded><![CDATA[<p>The <a href="http://www.eaobservatory.org/">EAO (East Asian Observatory)</a> is formed by <a href="https://www.eacoa.net/">EACOA (East Asian Core Observatories Association)</a> for the purpose of pursuing joint projects in astronomy within the East Asian region. In the era of very large scale astronomical instruments, East Asia will be competitive internationally by combining their funding resources, their technical expertise, and their manpower. The intention of EAO is to build and operate facilities, which will enhance and leverage existing and planned regional facilities. The intention of EAO is to raise funding and to build an observatory staff, separate from that of the EACOA institutions. As partners of the EAO, the EACOA institutes will help to establish the funding and to oversee the governance of EAO. The communities represented by the partners in EAO would have full access to all EAO facilities.</p>
<p>The EAO is chartered as a non-profit Hawaii corporation. Its first task is to assume the operation of the <a href="http://www.eaobservatory.org/jcmt/">James Clerk Maxwell Submillimetre Telescope</a> (JCMT) on the summit of Maunakea, Hawai`i. Pursuant to an agreement with the University of Hawaii, the EAO also provides engineering and IT support to the <a href="http://www.ukirt.hawaii.edu/">UKIRT Observatory</a> (UKIRT).</p>
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		<title>Spallation Neutron Source (SNS)</title>
		<link>https://epics-controls.org/projects-archive/sns/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Sat, 18 Nov 2017 13:22:01 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=982</guid>

					<description><![CDATA[<p><a href="https://neutrons.ornl.gov/sns">SNS</a> is a one-of-a-kind research facility that provides the most intense pulsed neutron beams in the world for scientific research and industrial development. SNS produces neutrons with an accelerator-based system that delivers short (microsecond) proton pulses to a target/moderator system, where neutrons are produced by a process called spallation. State-of-the-art experiment stations provide a [...]]]></description>
										<content:encoded><![CDATA[<p><a href="https://neutrons.ornl.gov/sns">SNS</a> is a one-of-a-kind research facility that provides the most intense pulsed neutron beams in the world for scientific research and industrial development. SNS produces neutrons with an accelerator-based system that delivers short (microsecond) proton pulses to a target/moderator system, where neutrons are produced by a process called spallation. State-of-the-art experiment stations provide a variety of capabilities for researchers across a broad range of disciplines, such as physics, chemistry, materials science, and biology.</p>
<p>With its more intense, brighter source of neutrons and world-class instrumentation, SNS provides the neutron scattering community with unprecedented research opportunities. SNS allows for measurements of greater sensitivity, higher speed, higher resolution, and in more complex sample environments than have been possible at existing neutron facilities.</p>
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		<title>Laser Interferometer Gravitational-Wave Observatory (LIGO)</title>
		<link>https://epics-controls.org/projects-archive/ligo/</link>
		
		<dc:creator><![CDATA[Ralph Lange]]></dc:creator>
		<pubDate>Mon, 13 Nov 2017 08:42:09 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=971</guid>

					<description><![CDATA[<p>The <a href="https://www.ligo.caltech.edu/">Laser Interferometer Gravitational-Wave Observatory (LIGO)</a> is leading the way in the new and exciting field of gravitational-wave astrophysics through the direct detection of gravitational waves predicted by Einstein’s General Theory of Relativity. LIGO’s multi-kilometer-scale gravitational wave detectors use laser interferometry to measure the minute ripples in the fabric of space-time caused by passing [...]]]></description>
										<content:encoded><![CDATA[<p>The <a href="https://www.ligo.caltech.edu/">Laser Interferometer Gravitational-Wave Observatory (LIGO)</a> is leading the way in the new and exciting field of gravitational-wave astrophysics through the direct detection of gravitational waves predicted by Einstein’s General Theory of Relativity. LIGO’s multi-kilometer-scale gravitational wave detectors use laser interferometry to measure the minute ripples in the fabric of space-time caused by passing gravitational waves from cataclysmic cosmic sources, such as the mergers of pairs of neutron stars or black holes. LIGO consists of two widely separated detectors within the United States, in Hanford, Washington and Livingston, Louisiana.</p>
<p>LIGO is funded by the U.S. National Science Foundation (NSF), operated by the California Institute of Technology (Caltech) and the Massachusetts Institute of Technology (MIT), and is aided by collaborators from the over 80 scientific institutions world-wide that are members of the LIGO Scientific Collaboration (LSC).</p>
<p>The 2017 Nobel Prize in Physics has been awarded to three key players in the development and ultimate success of LIGO.</p>
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		<title>National Synchrotron Light Source II</title>
		<link>https://epics-controls.org/projects-archive/nsls2/</link>
		
		<dc:creator><![CDATA[Timo Korhonen]]></dc:creator>
		<pubDate>Mon, 11 Sep 2017 12:21:40 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=390</guid>

					<description><![CDATA[<p><a href="https://www.bnl.gov/ps/">NSLS-II</a> is a state-of-the-art 3 GeV electron storage ring. The facility offers scientific and industrial researchers an array of beamlines with x-ray, ultraviolet, and infrared light to enable discoveries in clean and affordable energy, high-temperature superconductivity, molecular electronics, and more.</p>
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										<content:encoded><![CDATA[<p><a href="https://www.bnl.gov/ps/">NSLS-II</a> is a state-of-the-art 3 GeV electron storage ring. The facility offers scientific and industrial researchers an array of beamlines with x-ray, ultraviolet, and infrared light to enable discoveries in clean and affordable energy, high-temperature superconductivity, molecular electronics, and more.</p>
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		<title>Advanced Photon Source (APS)</title>
		<link>https://epics-controls.org/projects-archive/aps/</link>
		
		<dc:creator><![CDATA[AzAdmin]]></dc:creator>
		<pubDate>Thu, 24 Aug 2017 22:35:55 +0000</pubDate>
				<guid isPermaLink="false">https://epics-controls.org/?post_type=projects&#038;p=213</guid>

					<description><![CDATA[<p>The <a href="https://www.aps.anl.gov/">Advanced Photon Source</a> consists of 34 sectors; each sector contains one or more beamlines. There are several resources available to help you find information about APS sectors and beamlines.</p>
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										<content:encoded><![CDATA[<p>The <a href="https://www.aps.anl.gov/">Advanced Photon Source</a> consists of 34 sectors; each sector contains one or more beamlines. There are several resources available to help you find information about APS sectors and beamlines.</p>
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