Friday 6 June 2014

Microstructures embedded in materials using combined laser and plasma beams

Science Focus

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Miniscule microstructures can be embedded in materials with laser beams. But a lot of energy is needed for this when it comes to transparent materials like glass. So, researchers sought out a more efficient solution: they combined the laser with a plasma beam. Fraunhofer researchers combine a laser and a plasma beam for the first time to realize microstructures to glass objects. Initial results reveal that by this approach, the production process can become more precise and economical. © Fraunhofer IST     You can find them in cellphones, in high-quality cameras and electronic driver assistance systems: tiny optical components, made of glass, that are equipped with microstructures. As a rule, laser technology is used to insert the extremely fine structures into the glass surface. Since glass is transparent, however, laser processing becomes a real challenge: if the laser’s energy density is too low, then insufficient radiation is absorbed in order to achieve the desired effect. If the power density is excessive, then undesired side effects often result – like contamination by ablation debris. Researchers at the Fraunhofer Institute for Surface Engineering and Thin Films IST are now striking out on a completely new path: in the structuring process, they couple atmospheric

The post Microstructures embedded in materials using combined laser and plasma beams has been published on Technology Org.

 
#physics 
 » see original post http://feedproxy.google.com/~r/TechnologyOrgPhysicsNews/~3/JF8KqWWnxVQ/
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VIDEO: New 'digestion plant' recycles food

Science Focus

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A new multi-million pound food recycling plant is opening near Chertsey in Surrey. Tom Edwards reports. 
#science 
 » see original post http://www.bbc.co.uk/news/uk-27686225#sa-ns_mchannel=rss&ns_source=PublicRSS20-sa
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The Active Cigar Galaxy - Messier 82 Square Stickers

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Galaxies, Stars and Nebulae series

Composite of images of the active galaxy Messier 82 from the three Great Observatories: Hubble Space Telescope, Chandra X-Ray Observatory, and Spitzer Space Telescope. X-ray data recorded by Chandra appears here in blue, infrared light recorded by Spitzer appears in red. Hubble's observation of hydrogen emission appears in orange. Hubble's bluest observation appears in yellow-green.

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Violent birth announcement from an infant star

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(Phys.org) —This Hubble image shows IRAS 14568-6304, a young star that is cloaked in a haze of golden gas and dust. It appears to be embedded within an intriguing swoosh of dark sky, which curves through the image and obscures the sky behind.



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Comet PanSTARRS with Galaxy

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Sweeping slowly through northern skies, the comet PanSTARRS C/2012 K1 posed for this telescopic portrait on June 2nd in the constellation Ursa Major. Now in the inner solar system, the icy body from the Oort cloud sports two tails, a lighter broad dust tail and crooked ion tail extending below and right. The comet's condensed greenish coma makes a nice contrast with the spiky yellowish background star above. NGC 3319 appears at the upper left of the frame that spans almost twice the apparent diameter of the full Moon. The spiral galaxy is about 47 million light-years away, far beyond the stars in our own Milky Way. In comparison, the comet was a mere 14 light-minutes from our fair planet. This comet PanSTARRS will slowly grow brighter in the coming months remaining a good target for telescopic comet watchers and reaching perihelion, its closest approach to the Sun, while just beyond Earth's orbit in late August.

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Trendy Cool Sparkly New Nebula Design Room Stickers

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Cute and trendy pink blue teal nebula design with bright sparkly stars. All are photo printed.

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Cosmic collision

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XMM-Newton's view of the Bullet Group reveals the aftermath of a colossal merger of galaxies, hot gas and dark matter

via ESA Space Science

http://sci.esa.int/xmm-newton/54116-cosmic-collision-in-the-bullet-group/

Enhanced Hubble Image of Comet iPad Folio Cases

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Beam line for schools competition winners announced

Berkeley Lab Develops Nanoscope to Probe Chemistry on the Molecular Scale

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For years, scientists have had an itch they couldn’t scratch. Even with the best microscopes and spectrometers, it’s been difficult to study and identify molecules at the so-called mesoscale, a region of matter that ranges from 10 to 1000 nanometers in size. Now, with the help of broadband infrared light from the Advanced Light Source (ALS) synchrotron at the U.S. Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab), researchers have developed a broadband imaging technique that looks inside this realm with unprecedented sensitivity and range. By combining atomic force microscopy with infrared synchrotron light, researchers from Berkeley Lab and the University of Colorado have improved the spatial resolution of infrared spectroscopy by orders of magnitude, while simultaneously covering its full spectroscopic range, enabling the investigation of variety of nanoscale, mesoscale, and surface phenomena that were previously difficult to study. The new technique, called Synchrotron Infrared Nano-Spectroscopy or SINS, will enable in-depth study of complex molecular systems, including liquid batteries, living cells, novel electronic materials and stardust. “The big thing is that we’re getting full broadband infrared spectroscopy at 100 to 1000 times smaller scale,” says Hans Bechtel, principal scientific engineering associate at Berkeley Lab. “This is not an incremental

The post Berkeley Lab Develops Nanoscope to Probe Chemistry on the Molecular Scale has been published on Technology Org.

 
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Graphenea in the media

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Our research on gold nanoantennas on graphene attracted the attention of scientists and media alike. The ability to efficiently direct impinging light waves into a graphene sheet is exciting for opto-electronic and photo-voltaic applications alike, the former related to optical data processing, and the latter related to harvesting the energy of light. Furthermore, the demonstration that the same light waves can be steered by local changes in the conductivity, for example by applying voltage to an underlying gate, adds to the excitement of the presented results.



Equally exciting was a recent article in Financial Times, featuring information on Graphenea and messages from our CEO Jesus de la Fuente. The main focus of the article is the EU research and development (R&D) budget. According to FT, EU should be spending more on innovation. Graphene is featured in the article as one of the EU's key innovation advantages, with Graphenea taking the spotlight. To quote:



In 2013, the EU launched a €1bn research programme that aims to find ways of commercialising graphene. San Sebastián-based Graphenea is likely to be one of the main beneficiaries of this 10-year investment push. It is one of a group of small companies making graphene, mainly for research and development.



Both Jesus and Professor Andrea Ferrari of the Cambridge Graphene Centre agreed that there is a long way to walk before graphene applications go mainstream, and that the EU must provide relentless investment in research if it intends to be a leader of the graphene industry.



You can meet Jesus and our Business Development Director Iñigo Charola, as well as many other business leaders, at the Graphene Supply, Application, and Commercialisation summit in Manchester next week (June 12-13). The meeting will be hosted by the University of Manchester National Graphene Institute. Topics will span the entire graphene device production chain, from supply, to development, to integration. See you there!

via Graphenea

New isotopic evidence supporting moon formation via Earth collision with planet-sized body

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A new series of measurements of oxygen isotopes provides increasing evidence that the moon formed from the collision of the Earth with another large, planet-sized astronomical body, around 4.5 billion years ago.

via Science Daily

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The Active Cigar Galaxy - Messier 82 Sticker

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Galaxies, Stars and Nebulae series

Composite of images of the active galaxy Messier 82 from the three Great Observatories: Hubble Space Telescope, Chandra X-Ray Observatory, and Spitzer Space Telescope. X-ray data recorded by Chandra appears here in blue, infrared light recorded by Spitzer appears in red. Hubble's observation of hydrogen emission appears in orange. Hubble's bluest observation appears in yellow-green.

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Image code: agmet

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Hubble Image of NGC 3324 Cover For iPad Air

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