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Unravelling Coronal Mass Ejections from Our Solar System’s Origin

Young stars ejecting plasma could give us clues into the Sun’s past Kyoto, Japan — Down here on Earth we don’t usually notice, but the Sun is frequently ejecting huge masses of plasma into space. These are called coronal mass ejections (CMEs). They often occur together with sudden brightenings called flares, and sometimes extend far enough to disturb Earth’s magnetosphere, generating space weather phenomena including auroras or geomagnetic storms, and even damaging power grids on occasion. Scientists believe that when…

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Physics & Astronomy

Time in space

This end only comes to the heavies of the neighborhood, those that weigh 30 times as much as our sun or more. When it happens, their dazzling light can be seen…

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UU Science Project Aims to Reduce Animal Testing

The university’s Systems Biology Research Group is partnering eight other universities, institutes and companies in a €2.8 million European Commission…

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New Innovation Enhances Life in Animated Characters

The development, lead by Bournemouth researcher Prof Jian Zhang and his colleague Dr Xiaosong Yang, allows animators to ‘flesh out’ their characters from the…

Physics & Astronomy

Long-lasting but dim brethren of cosmic flashes

Astronomers, using ESO’s Very Large Telescope, have for the first time made the link between an X-ray flash and a supernova. Such flashes are the little…

Physics & Astronomy

Death Of A Star Scientists Watch Supernova In Real-Time

The event began on the 18th February, 2006, in a star forming galaxy about 440 million light-years away toward the constellation Aries. At that time it was…

Physics & Astronomy

AKARI Marks Milestone in Mapping Stars’ Life Cycles

AKARI was launched on February 21st 2006 from Uchinoura Space Centre, Japan, and is now about half way to completing its first map of the sky in infrared…

Physics & Astronomy

Explore Kasei Valles: Insights from HRSC Orbit 1429 Images

The HRSC obtained these images during orbit 1429 at a ground resolution of approximately 29 metres per pixel. The Kasei Valles region lies approximately…

Physics & Astronomy

Desktop Printing with Nanotube Ink: A New Era in Manufacturing

The method, which is described in the August 2006 issue of the journal Small, could lead to a new process for manufacturing a wide range of nanotube-based…

Physics & Astronomy

UA Physicists Invent 'QuIET'- Single Molecule Transistors

They have applied for a patent on their device, called Quantum Interference Effect Transistor, nicknamed “QuIET.” The American Chemical Society publication,…

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Why can we see what our cameras can't?

The bane of all wedding videos; that picture of the bride in front of the window where her face is so dark that you can't see the features may soon be a thing…

Physics & Astronomy

Cassiopeia A – The colourful aftermath of a violent stellar death

The image is a composite made from 18 separate images taken using Hubble’s Advanced Camera for Surveys (ACS), and it shows the Cas A remnant as a broken ring…

Physics & Astronomy

Nanotechnology Enhances Body Armour for Better Protection

Current body armour relies on a stiff and relatively heavy layer of ceramic material to absorb ballistic impact. This makes body armour heavy and unwieldy. The…

Physics & Astronomy

SMART-1 ‘star tracker’ peeks at the approaching lunar surface

One week before the end of the SMART-1 mission, the SMART-1 Mission Control Team at the European Space Operations Centre (ESOC) in Germany are working together…

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3D Design Platform Bridges Multi-User Applications Seamlessly

This IST-funded project has created the first open internet-based platform for multi-user, distributed 3D graphics design, one that allows both proprietary and…

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New Computer Model Enhances Weather Forecast Accuracy

The high-resolution Weather Research and Forecasting model (WRF) is the first model to serve as both the backbone of the nation's public weather forecasts and…

Physics & Astronomy

ESA’s Cluster mission establishes why Earth’s aurorae shine

Such colourful aurorae regularly light the higher latitudes in the northern and southern hemisphere. They are caused mostly by energetic electrons spiralling…

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