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&lt;div&gt;Doctoral student Guillermo Moroni works the grill, proudly serving lamb chops and hamburgers to his scientific collaborators—other postdocs, technicians, scientists and graduate students. The smell of roasted corn floats across picnic tables littered with cakes, pies and brownies.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;The gathering is more than a simple celebration of the start of summer; it marks a tipping point. The Dark Energy Camera, the first device specifically designed to search for dark energy, is on the brink of completion. Project manager Brenna Flaugher—who organized the cookout—and her colleagues are about to see the project they’ve been preparing for the past eight years transition from dream to reality.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;This fall, scientists will fire up DECam, as it’s affectionately known, on a mountaintop in Chile and see their hard work pay off.“It’s going to be very exciting for all of us to open the shutter for the first time,” Flaugher says. “Who knows what we’ll see?”&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;What they hope to see are signs of the invisible, mysterious force that seems to pull the universe apart—a force that has never been directly observed.&lt;/div&gt;
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PublishingPageContent:SW|On a hot June Illinois afternoon, a celebratory atmosphere prevails at Kuhn Barn, a holdover from Fermi National Accelerator Laboratory’s agricultural past and also a popular cookout spot.&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Doctoral student Guillermo Moroni works the grill, proudly serving lamb chops and hamburgers to his scientific collaborators—other postdocs, technicians, scientists and graduate students. The smell of roasted corn floats across picnic tables littered with cakes, pies and brownies.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;The gathering is more than a simple celebration of the start of summer; it marks a tipping point. The Dark Energy Camera, the first device specifically designed to search for dark energy, is on the brink of completion. Project manager Brenna Flaugher—who organized the cookout—and her colleagues are about to see the project they’ve been preparing for the past eight years transition from dream to reality.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;This fall, scientists will fire up DECam, as it’s affectionately known, on a mountaintop in Chile and see their hard work pay off.“It’s going to be very exciting for all of us to open the shutter for the first time,” Flaugher says. “Who knows what we’ll see?”&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;What they hope to see are signs of the invisible, mysterious force that seems to pull the universe apart—a force that has never been directly observed.&lt;/div&gt;\r\n​
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vti_title:SR|Surprise Difference in Neutrino And Antineutrino Mass Lessening with New Measurements from a Fermilab ExperimentSurprise Difference in Neutrino And Antineutrino Mass Lessening with New Measurements from a Fermilab Experiment
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​&lt;div&gt;The LHC benefits from the contributions of 97 U.S. universities and laboratories. More than a quarter of the engineers, physicists and graduates working on the LHC experiments are from U.S. universities and labs.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Meeting attendees will discuss ongoing work on data analysis, the LHC accelerator and detector upgrades and day-to-day issues facing members of the U.S. particle physics community working at CERN.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;&amp;quot;We provide a forum for issues that concern the US LHC community, which is of course very international, and a channel to communicate the status and needs of this community to Congress, funding agencies and executive offices,&amp;quot; said US LUO Chair Harvey Newman.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Representatives of the DOE and NSF will also give the view from Washington on the future U.S. HEP program and involvement at CERN.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;US LUO helps foster communication between the LHC community and U.S. physicists and helps physicists prepare and adapt to life at CERN. One of US LUO&#39;s most important roles is an annual visit to Washington, D.C., where representatives meet with members of Congress to discuss the importance and excitement of particle physics research.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;&amp;quot;It&#39;s very useful to go and explain the compelling nature of what we do and keep us on the radar,&amp;quot; Newman said.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;At the meeting, representatives from the four big LHC experiments will present an overview of 2012 operations and results. Scientists from CMS and ATLAS will speak on prospects for the measurement of the Higgs-like boson this year.&lt;/div&gt;
&lt;div&gt;Today Newman will talk about overall U.S. participation at CERN and the state of US LUO. On Saturday, CERN senior physicist Rudiger Voss will present on the status of negotiations to carry forward U.S. involvement at CERN in a new framework. The current U.S.-CERN agreement covers involvement between 1997 and 2017.&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Saturday will also include a bit of fun – the Young Physicists Lightning Round, which allows young physicists to present their work in a competitive atmosphere. Winners will be invited to join the annual trip to Washington.&lt;/div&gt;
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PublishingPageContent:SW|&lt;div&gt;Around 100 Large Hadron Collider collaborators from around the United States are joining their colleagues at Fermilab for the rest of this week to present and discuss their research. The gathering is the &lt;a target=&quot;_blank&quot; href=&quot;https://indico.fnal.gov/conferenceDisplay.py?confId=5830&quot;&gt;&lt;font color=&quot;#003399&quot;&gt;annual meeting of the US LHC Users Organization&lt;/font&gt;&lt;/a&gt;.&lt;/div&gt;\r\n​&lt;div&gt;The LHC benefits from the contributions of 97 U.S. universities and laboratories. More than a quarter of the engineers, physicists and graduates working on the LHC experiments are from U.S. universities and labs.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Meeting attendees will discuss ongoing work on data analysis, the LHC accelerator and detector upgrades and day-to-day issues facing members of the U.S. particle physics community working at CERN.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;&amp;quot;We provide a forum for issues that concern the US LHC community, which is of course very international, and a channel to communicate the status and needs of this community to Congress, funding agencies and executive offices,&amp;quot; said US LUO Chair Harvey Newman.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Representatives of the DOE and NSF will also give the view from Washington on the future U.S. HEP program and involvement at CERN.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;US LUO helps foster communication between the LHC community and U.S. physicists and helps physicists prepare and adapt to life at CERN. One of US LUO&#39;s most important roles is an annual visit to Washington, D.C., where representatives meet with members of Congress to discuss the importance and excitement of particle physics research.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;&amp;quot;It&#39;s very useful to go and explain the compelling nature of what we do and keep us on the radar,&amp;quot; Newman said.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;At the meeting, representatives from the four big LHC experiments will present an overview of 2012 operations and results. Scientists from CMS and ATLAS will speak on prospects for the measurement of the Higgs-like boson this year.&lt;/div&gt;\r\n&lt;div&gt;Today Newman will talk about overall U.S. participation at CERN and the state of US LUO. On Saturday, CERN senior physicist Rudiger Voss will present on the status of negotiations to carry forward U.S. involvement at CERN in a new framework. The current U.S.-CERN agreement covers involvement between 1997 and 2017.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Saturday will also include a bit of fun – the Young Physicists Lightning Round, which allows young physicists to present their work in a competitive atmosphere. Winners will be invited to join the annual trip to Washington.&lt;/div&gt;\r\n&lt;div&gt;&lt;em&gt;&lt;/em&gt; &lt;/div&gt;
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&lt;div&gt;The U.S. Department of Energy &lt;a href=&quot;http://www.doeleadershipcomputing.org/&quot; target=&quot;_blank&quot;&gt;&lt;font color=&quot;#006090&quot;&gt;INCITE&lt;/font&gt;&lt;/a&gt; program has recently awarded the Computational Physics for Accelerators group in the Scientific Computing Division 80 million hours of supercomputing resources at the Argonne Leadership Computing Facility (ALCF). INCITE is a competitive multi-disciplinary program for providing large-scale research projects with dedicated supercomputing resources. Only about 33% of proposals were funded this year. &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;In support of the Intensity Frontier at Fermilab, the group will simulate the Main Injector for Project X intensities and the Booster at current intensities and at one of the intensities for Phase One of Project X. In particular, they will model the physics of space charge, which is the effect of particles reacting to others particles’ electric charges, and wakefields, the fields that are generated by and that interact with particle beams as they travel through the accelerator’s metallic pipes. These simulations help explore different configurations of the accelerator. &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;&lt;div&gt;“Part of what’s making this such a big computing job is that we’re not only simulating one bunch of particles. We’re simulating all the bunches in the Main Injector,” says Jim Amundson, leader of the Computational Physics for Accelerators group. “[That is] some number around 540, and for our largest jobs… we will use on the order of 65 thousand cores to provide a single simulation.” &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;The simulations will be performed on two IBM Blue Gene supercomputers. Intrepid, a Blue Gene/P machine (a second generation of Blue Gene installation), has approximately 160 thousand cores; a new Blue Gene/Q machine called Mira has 250 thousand—not only more cores, but also faster cores that can do more threading, meaning more parallel data processing. &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;“What we’re focusing on for this particular proposal is the really large jobs,” says Amundson; ”The biggest ones are inconceivable on our local systems, and even the smaller ones would not be very effective.” &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Though the allocated time at the ALCF facilities will not be available until January, the group already has plans for next year’s proposal. &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;“Next year, we’ll involve adding electron cloud effects,” says Amundson.&lt;/div&gt;&lt;/div&gt;' ows_SummaryLinks='&lt;div title=&quot;_schemaversion&quot; id=&quot;_3&quot;&gt;
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&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Particles within the three individual bunches feel the effect of space charge as well as wakefields due to induced beam pipe currents. The wakefields give rise to bunch-to-bunch effects, which can affect the stability of the machine. INCITE calculations at ALCF will study these effect in both the Booster, which includes up to 84 bunches, and the Main Injector, which includes up to 588 bunches.&lt;/div&gt;' ows_NewsCenterArticleSummary='It’s fairly easy to simulate a single particle—or even a bunch of particles that don’t interact with each other—moving through a particle accelerator. Assuming you know how, you could run those types of jobs on your desktop computer. But, if you want to simulate the way particles interact with each other, you have to simulate many particles. And to do that, you need plenty of computing muscle.' ows_NewsCenterArticleFeaturedItem='1' ows_NewsCenterArticleAuthor='Marcia Teckenbrock' ows_NewsCenterExternalVideoFeaturedItem='0' ows_NewsCenterExternalVideoCategory='Streaming Video' ows_NewsCenterArticleYear='string;#2013' ows_NewsCenterFeatureRelatedImage1='&lt;img alt=&quot;&quot; src=&quot;/PublishingImages/_w/mira_250_png.JPG&quot; style=&quot;border:0px solid&quot; /&gt;' ows_NewsCenterPressReleaseCategories=';#General;#' ows_PageAppr='16' ows_PageContentCalc='error;#2' ows_ID='40' ows_ContentType='Fermilab Feature Page' ows_Created='2013-01-09 13:01:29' ows_Author='21;#i:0#.f|fnaluser|jprell-admin' ows_Modified='2013-01-09 13:07:00' ows_Editor='1073741823;#System Account' ows_FileRef='40;#Pages/Features/80-million-hours-awarded-for-simulations.aspx' ows_FileDirRef='40;#Pages/Features' ows_Last_x0020_Modified='40;#2013-01-09 13:06:42' ows_Created_x0020_Date='40;#2013-01-09 13:01:29' ows_File_x0020_Size='40;#8975' ows_FSObjType='40;#0' ows_SortBehavior='40;#0' ows_PermMask='0x7fffffffffffffff' ows_CheckedOutUserId='40;#' ows_IsCheckedoutToLocal='40;#0' ows_UniqueId='40;#{78B1FB55-8C21-4BFC-B414-D6AD00AD0FF6}' ows_SyncClientId='40;#' ows_ProgId='40;#' ows_ScopeId='40;#{383F684B-2C7D-492B-9038-EEDBBAE941C7}' ows_VirusStatus='40;#8975' ows_CheckedOutTitle='40;#' ows__CheckinComment='40;#' ows__EditMenuTableStart='80-million-hours-awarded-for-simulations.aspx' ows__EditMenuTableStart2='40' ows__EditMenuTableEnd='40' ows_LinkFilenameNoMenu='80-million-hours-awarded-for-simulations.aspx' ows_LinkFilename='80-million-hours-awarded-for-simulations.aspx' ows_LinkFilename2='80-million-hours-awarded-for-simulations.aspx' ows_DocIcon='aspx' ows_ServerUrl='/Pages/Features/80-million-hours-awarded-for-simulations.aspx' ows_EncodedAbsUrl='https://computingbits-dev.fnal.gov/Pages/Features/80-million-hours-awarded-for-simulations.aspx' ows_BaseName='80-million-hours-awarded-for-simulations' ows_FileSizeDisplay='8975' ows_MetaInfo='40;#PublishingContact:IW|21
PublishingPageContent:SW|​It’s fairly easy to simulate a single particle—or even a bunch of particles that don’t interact with each other—moving through a particle accelerator. Assuming you know how, you could run those types of jobs on your desktop computer. But, if you want to simulate the way particles interact with each other, you have to simulate many particles. And to do that, you need plenty of computing muscle. &lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;The U.S. Department of Energy &lt;a href=&quot;http://www.doeleadershipcomputing.org/&quot; target=&quot;_blank&quot;&gt;&lt;font color=&quot;#006090&quot;&gt;INCITE&lt;/font&gt;&lt;/a&gt; program has recently awarded the Computational Physics for Accelerators group in the Scientific Computing Division 80 million hours of supercomputing resources at the Argonne Leadership Computing Facility (ALCF). INCITE is a competitive multi-disciplinary program for providing large-scale research projects with dedicated supercomputing resources. Only about 33% of proposals were funded this year. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;In support of the Intensity Frontier at Fermilab, the group will simulate the Main Injector for Project X intensities and the Booster at current intensities and at one of the intensities for Phase One of Project X. In particular, they will model the physics of space charge, which is the effect of particles reacting to others particles’ electric charges, and wakefields, the fields that are generated by and that interact with particle beams as they travel through the accelerator’s metallic pipes. These simulations help explore different configurations of the accelerator. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;&lt;div&gt;“Part of what’s making this such a big computing job is that we’re not only simulating one bunch of particles. We’re simulating all the bunches in the Main Injector,” says Jim Amundson, leader of the Computational Physics for Accelerators group. “[That is] some number around 540, and for our largest jobs… we will use on the order of 65 thousand cores to provide a single simulation.” &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;The simulations will be performed on two IBM Blue Gene supercomputers. Intrepid, a Blue Gene/P machine (a second generation of Blue Gene installation), has approximately 160 thousand cores; a new Blue Gene/Q machine called Mira has 250 thousand—not only more cores, but also faster cores that can do more threading, meaning more parallel data processing. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;“What we’re focusing on for this particular proposal is the really large jobs,” says Amundson; ”The biggest ones are inconceivable on our local systems, and even the smaller ones would not be very effective.” &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Though the allocated time at the ALCF facilities will not be available until January, the group already has plans for next year’s proposal. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;“Next year, we’ll involve adding electron cloud effects,” says Amundson.&lt;/div&gt;&lt;/div&gt;
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NewsCenterArticleSummary:SW|It’s fairly easy to simulate a single particle—or even a bunch of particles that don’t interact with each other—moving through a particle accelerator. Assuming you know how, you could run those types of jobs on your desktop computer. But, if you want to simulate the way particles interact with each other, you have to simulate many particles. And to do that, you need plenty of computing muscle.
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PublishingImageCaption:SW|​Multiple-bunch simulation of the Fermilab Booster particle accelerator. &lt;div&gt;The beam in most machines is divided into a number of grous of particles separated longitudinally. The Booster can hold 84 bunches, the Main Injector 588. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Particles within the three individual bunches feel the effect of space charge as well as wakefields due to induced beam pipe currents. The wakefields give rise to bunch-to-bunch effects, which can affect the stability of the machine. INCITE calculations at ALCF will study these effect in both the Booster, which includes up to 84 bunches, and the Main Injector, which includes up to 588 bunches.&lt;/div&gt;
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&lt;div&gt;Virtualization saves the laboratory money by consolidating a number of virtual hosts into single virtual workloads, thereby reducing the costs of power, cooling, rack space, cabling and other items. Additional benefits of virtualization to our customers include increased flexibility, rapid recovery, higher performance, redundancy (in most cases) and fewer hardware management processes.&lt;/div&gt;
&lt;div&gt;A key project we are developing is a self-service portal that customers can use to quickly provision virtual systems based on customer-provided templates. This will enable our customers to rapidly deploy virtual machines with known configurations of selected operating systems drawn against the pooled resources of the entire virtual environment.&lt;/div&gt;
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PublishingPageContent:SW|&lt;p&gt;As a member of the Storage and Virtual Services group, I help provide virtual services to our customers. I work with server owners to virtualize their Windows and Linux servers and then provide the management, monitoring and backup and recovery interface needed to manage their virtualized workloads. &lt;/p&gt;\r\n&lt;div&gt;Virtualization saves the laboratory money by consolidating a number of virtual hosts into single virtual workloads, thereby reducing the costs of power, cooling, rack space, cabling and other items. Additional benefits of virtualization to our customers include increased flexibility, rapid recovery, higher performance, redundancy (in most cases) and fewer hardware management processes.&lt;/div&gt;\r\n&lt;div&gt;A key project we are developing is a self-service portal that customers can use to quickly provision virtual systems based on customer-provided templates. This will enable our customers to rapidly deploy virtual machines with known configurations of selected operating systems drawn against the pooled resources of the entire virtual environment.&lt;/div&gt;\r\n&lt;div&gt;In addition, I am working with the storage portion of our group to become familiar with and provide backup support for our Storage Area Network (SAN) and site-wide backup services. &lt;/div&gt;
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&lt;div&gt;In recent years, I have led the SDSS supernova effort (SDSS SN). Like all experiments, the ultimate goal is to analyze the data and publish the results. The supernova survey is an international effort that has resulted in a sample of over 500 well-identified supernovae and more than 30 publications in scientific journals. Aside from doing some analysis myself, my role is to organize meetings, coordinate analyses and review papers intended for publication. We are preparing to end the SDSS effort with a full data release so that other researchers may make use of this data. However a derivative of SDSS SN will survive: Some of us will seek to improve analysis techniques in collaboration with another major experiment known as Supernovae Legacy Survey (SNLS).&lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;In addition, I work on the Dark Energy Survey (DES) supernova survey. Originally co-leader of the supernova effort, I relinquished that role to concentrate on the software needed. Although some supernovae are visually obvious, most are discovered by a quantitative analysis that involves subtracting images of the sky taken at two different times and looking for new sources of light that were absent from the first image. The analysis would be fairly easy if the observing conditions were always the same. Unfortunately, the telescope alignment changes slightly, the atmosphere bends the light in different ways, the level of sky background changes and a host of objects can be mistaken for real supernovae depending on the selection criteria. Therefore, construction of an analysis program and the optimization of frame subtraction has been the focus of my efforts in recent months. &lt;/div&gt;
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PublishingPageContent:SW|​I joined the Experimental Astrophysics Group to work on the supernova survey, part of the Sloan Digital Sky Survey (SDSS). Supernovae have been objects of intense scientific interest. They are the result of the explosions of single stars, but the explosion can be as bright as an entire galaxy, so they can be seen from very large distances. In addition, some types of explosions have known luminosities, so we can accurately estimate distances based on the apparent brightness of the supernova. The ability to measure these large cosmological distances is key to understanding the formation of the universe. In fact, the 2011 Nobel Prize in physics was awarded for pioneering work in this field.&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;In recent years, I have led the SDSS supernova effort (SDSS SN). Like all experiments, the ultimate goal is to analyze the data and publish the results. The supernova survey is an international effort that has resulted in a sample of over 500 well-identified supernovae and more than 30 publications in scientific journals. Aside from doing some analysis myself, my role is to organize meetings, coordinate analyses and review papers intended for publication. We are preparing to end the SDSS effort with a full data release so that other researchers may make use of this data. However a derivative of SDSS SN will survive: Some of us will seek to improve analysis techniques in collaboration with another major experiment known as Supernovae Legacy Survey (SNLS).&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;In addition, I work on the Dark Energy Survey (DES) supernova survey. Originally co-leader of the supernova effort, I relinquished that role to concentrate on the software needed. Although some supernovae are visually obvious, most are discovered by a quantitative analysis that involves subtracting images of the sky taken at two different times and looking for new sources of light that were absent from the first image. The analysis would be fairly easy if the observing conditions were always the same. Unfortunately, the telescope alignment changes slightly, the atmosphere bends the light in different ways, the level of sky background changes and a host of objects can be mistaken for real supernovae depending on the selection criteria. Therefore, construction of an analysis program and the optimization of frame subtraction has been the focus of my efforts in recent months. &lt;/div&gt;\r\n
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   <z:row ows_ContentTypeId='0x010100C568DB52D9D0A14D9B2FDCC96666E9F2007948130EC3DB064584E219954237AF3900242457EFB8B24247815D688C526CD44D00D66D44F234D545B5A8FB02531D34F67600CFF7C7D352854C4E96B4550ACB6FCB7F00AC02711A46346F4E8E10DF41FD427447' ows__ModerationStatus='0' ows_FileLeafRef='43;#FCC2-Emergency-Panel-Changes.aspx' ows_Modified_x0020_By='SHAREPOINT\system' ows_Created_x0020_By='i:0#.f|fnaluser|jprell-admin' ows_File_x0020_Type='aspx' ows_Title='FCC2 Emergency Panel Changes' ows_PublishingContact='21;#i:0#.f|fnaluser|jprell-admin' ows_PublishingPageLayout='https://computingbits-dev.fnal.gov/_catalogs/masterpage/FnalFeatureArticleLayout.aspx, News Center Feature Layout' ows_PublishingPageImage='&lt;img alt=&quot;&quot; src=&quot;/PublishingImages/_w/emergency%20panel_jpg.JPG&quot; style=&quot;border:0px solid&quot; /&gt;' ows_PublishingPageContent='​As a result of the accidental halon discharge that occurred during the October 22 planned power outage, Fermilab’s Fire Protection Program Manager conducted a risk analysis on the operating status of the automated halon discharge system in FCC2 and subsequently recommended operating the system in manual mode only. This means that the red halon pull-boxes at each side of the room have been deactivated with a label covering the pull-boxes indicating they are no longer functioning. &lt;div&gt; &lt;/div&gt;
&lt;div&gt;Only fire department personnel will control the halon system, which distributes halon under the floor. The system is not effective at suppressing a fire above the floor tiles. &lt;/div&gt;
&lt;div&gt; &lt;/div&gt;
&lt;div&gt;Also note that the red “halon abort” buttons located on the fire panel at each end of the room—not to be confused with the red fire alarm pull-boxes also at each end of the room—have been removed. The fire alarm pull-boxes and Emergency Power Off (EPO) button will still function as always and will only trigger the building alarm and notify the fire department.&lt;/div&gt;
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&lt;div&gt;The most important thing to remember is that if you hear a fire alarm, you should immediately evacuate the building. &lt;/div&gt;' ows_SummaryLinks='&lt;div title=&quot;_schemaversion&quot; id=&quot;_3&quot;&gt;
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PublishingPageContent:SW|​As a result of the accidental halon discharge that occurred during the October 22 planned power outage, Fermilab’s Fire Protection Program Manager conducted a risk analysis on the operating status of the automated halon discharge system in FCC2 and subsequently recommended operating the system in manual mode only. This means that the red halon pull-boxes at each side of the room have been deactivated with a label covering the pull-boxes indicating they are no longer functioning. &lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Only fire department personnel will control the halon system, which distributes halon under the floor. The system is not effective at suppressing a fire above the floor tiles. &lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;Also note that the red “halon abort” buttons located on the fire panel at each end of the room—not to be confused with the red fire alarm pull-boxes also at each end of the room—have been removed. The fire alarm pull-boxes and Emergency Power Off (EPO) button will still function as always and will only trigger the building alarm and notify the fire department.&lt;/div&gt;\r\n&lt;div&gt; &lt;/div&gt;\r\n&lt;div&gt;The most important thing to remember is that if you hear a fire alarm, you should immediately evacuate the building. &lt;/div&gt;
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NewsCenterArticleSummary:SW|As a result of the accidental halon discharge that occurred during the October 22 planned power outage, Fermilab’s Fire Protection Program Manager conducted a risk analysis on the operating status of the automated halon discharge system in FCC2 and subsequently recommended operating the system in manual mode only.
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