The story behind the luminiscent minerals display in Rudolph Hall There’s a small room in Rudolph Hall that
The post Rocks that glow in the dark has been published on Technology Org.
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There are advances being made almost daily in the disciplines required to make space and its contents accessible. This blog brings together a lot of that info, as it is reported, tracking the small steps into space that will make it just another place we carry out normal human economic, leisure and living activities.
The story behind the luminiscent minerals display in Rudolph Hall There’s a small room in Rudolph Hall that
The post Rocks that glow in the dark has been published on Technology Org.
Over the next 24 hours, beams of protons should collide in the Large Hadron Collider (LHC) at the record-breaking energy of 13 teraelectronvolts (TeV) for the first time. This is one of the many steps required to prepare the machine before the LHC's second physics run can begin. The LHC Operations team plans to declare "stable beams" in the coming weeks – the signal for the LHC experiments to start taking physics data at this new energy frontier.
"We begin by bringing the beams into collision at 13 TeV, and adjusting their orbits to collide them head-on," says Ronaldus SuykerBuyk of the Operations team.
Last month proton beams were back in the accelerator for the first time after two years of intense maintenance and consolidation. The first beam at the record energy of 6.5 TeV circulated on 10 April, and the first collisions – at the lower beam energy of 450 gigaelectronvolts (GeV) – followed.
The team has already checked and fine-tuned all the beam instruments, magnets and collimators along the 27-kilometre accelerator for collisions at 900 GeV. But when beam energy increases to 6.5 TeV, the beam parameters and orbits change significantly as compared to 450 GeV. In addition, the beams are focused down to a much smaller spot size within the experiments and as a consequence the location of collisions changes.
"When we start to bring the beams into collision at a new energy, they often miss each other," says Jorg Wenninger of the LHC Operations team. "The beams are tiny – only about 20 microns in diameter at 6.5 TeV; more than 10 times smaller than at 450 GeV. So we have to scan around – adjusting the orbit of each beam until collision rates provided by the experiments tell us that they are colliding properly."
The design of the LHC allows more than 2800 bunches of protons to circulate in each beam at a time. But the LHC Operations team will start collision tests with just one or two bunches per beam at the nominal intensity of 1011 particles per bunch to ensure that all is running smoothly.
Once they have found the points at which the beams interact optimally to give the most physics data, collimators have to be positioned accurately around the beam orbits to intercept particles that stray from the beam before they can hit magnets or detectors. "When the positioning of all collimators has been validated the LHC will switch over to production mode," says Wenninger, "and become a 'collision factory', delivering data to experiments." At this point, the experiments will switch on fully, and LHC Run 2 will begin.
In the meantime, the large LHC experiments ALICE, ATLAS, CMS and LHCb will use the test data to check specific parts of their detectors for the upcoming physics run.
"The collisions at 13 TeV will allow us to further test all improvements that have been made to the trigger and reconstruction systems, and check the synchronisation of all the components of our detector," says CMS spokesperson Tiziano Camporesi.
“These data are precious to complete the fine tuning of the preparation for the run,” says ALICE spokesperson Paolo Giubellino. “ALICE has installed new detectors during the shutdown, and has significantly upgraded the trigger and readout. The validation of the new hardware will greatly benefit from the first data.”
"Although these collisions are not used for physics studies, they are useful for refining the synchronization of the readout time of different parts of the calorimeters and muon detectors," says LHCb spokesperson Guy Wilkinson.
"These 13 TeV data allow us to work on further improving the ATLAS detector readiness, following the recent 900 GeV collisions," says ATLAS spokesperson Dave Charlton. "The higher energies mean that we expect more active and energetic events, which will let us probe more deeply into the detector, for example."
Declaring "stable beams" will be only the beginning for the LHC Operations team. "We’re still working on the injection chain to the LHC, and finalising the collimators," says Wenninger. “And the machine evolves around you. There are little changes over the months. There’s the alignment of the machine, which moves a little with the slow-changing geology of the area. So we keep adjusting every day."
This week's collisions at 13 TeV are to check that CERN's flagship – the LHC – is sea-worthy. But we haven't yet begun the voyage to new frontiers.
The push for renewable energy has led to the generation of biofuels from cellulose-rich biomass, algae, and crops. Currently, crop-based biofuels are limited to those derived from agricultural products: corn, soybean, rapeseed, and surgarcane. An increase in the demand for crop-based biofuels will require either an increase in the amount of agricultural land or an increase in crop production on existing land.
An expansion of agricultural land can only occur if whatever is presently on the land is sacrificed—this can mean abandoned lands, pastures, or natural systems. Natural systems such as grasslands and forests store large amounts of carbon; if turned into agricultural lands, this carbon could be released into the atmosphere. Though crops also store carbon as biomass during their growth, regular harvests do not allow for long-term carbon storage. From a climate perspective, this could be problematic.
Do the carbon and nitrogen emissions that result from the deforestation and land-use intensification offset the environmental benefits of displacing fossil fuels? One way to assess this issue is by calculating carbon payback times, which represent the period over which the total greenhouse gas savings due to the displacement of fossil fuels equals the initial losses in ecosystem carbon stocks caused by land conversion.
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For several years, the National Ignition Facility (NIF) at Lawrence Livermore National Laboratory (LLNL) has pursued an indirect
The post Researchers toss around rugby-shaped hohlraums for ignition experiments has been published on Technology Org.
Researchers from NASA’s Langley Research Center are in Shreveport, Louisiana, with the Boeing ecoDemonstrator 757 aircraft looking for
The post Counting on Shreveport Bugs on Non-Stick Wing Coatings has been published on Technology Org.
“One of the dreariest spots on life’s road is the point of conviction that nothing will ever again happen to you.” –Faith Baldwin
Bet you thought you knew it all about the asteroid belt. These frozen, ice-and-rock worlds orbit farther out from Mars, closer in than Jupiter, and occasionally get hurled towards the inner Solar System by gravitational interactions. But the largest world, Ceres, at just about half the diameter of the Moon (or the size of Texas), exhibits an unusual surprise: a brilliant set of white spots at the bottom of one of its largest craters.
While the speculation abounds from simple (water-ice) to the astounding (aliens!), there are only three realistic possibilities given what Dawn has seen so far. What’s even more exciting? It’s already got the equipment on board to decide which possibility is the right one!
Come find out the whole story behind Ceres’ white spots — so far — over at Starts With A Bang!