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LUX dark matter detector

Detecting dark matter

The kind of matter and energy we can see and touch – whether it is in the form of atoms and molecules, or heat and light, only forms a tiny proportion of the content of the Universe, only about 5%. Over a quarter is dark matter, which is totally invisible but whose gravitational attraction can be detected; while over two thirds is dark energy, a force that pushes the Universe to expand ever faster.
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Huge solar flare caught by Hinode satellite

3 June 2013

15 May solar flare seen by Hinode
This still image of the 15 May 2013 solar flare, seen by Hinode, shows the huge energy unleashed in such events. Note that the greyscale observations from the satellite have been colourised in this image.
JAXA, NASA, ESA and UKSA. Processed by Joten Okamoto

This year, solar activity should reach its peak. Solar flares are the most energetic explosions in the Solar System, with energies reaching the equivalent of tens of millions of atomic bombs in minutes.

This solar cycle has been a little unusual with a long lasting minimum period, leading to concerns that we were going into an extended minimum. However activity has picked up, with a series of large flares occurring in the last few weeks. This movie shows a flare that occurred early in the morning of 15 May, which was observed by the Hinode spacecraft.

Hinode was launched almost 7 years ago, and is the ‘Hubble’ of the Sun, observing activity in high resolution. It was built and is operated through a collaboration between Japan, the US and the UK, including one instrument built at UCL. Researchers at UCL’s Mullard Space Science Laboratory use data from Hinode to study solar physics.

The movie shows dark spots known as sunspots which are the location of extremely strong magnetic fields and are the sources of strong flaring. The Sun has strong convection and unusual differential rotation, both of these movements causing magnetic fields to collide, releasing energy. The bright regions occurring above the sunspots is the flare itself, which is many times larger that the size of the Earth.

When Hinode detects a flare, it goes into ‘flare mode’, increasing the rate at which it captures images. So as not to overwhelm its data connection back to Earth, the size of its images is automatically reduced, which is why black bars appear at the sides of the image part-way through the sequence.

Notes

Hinode is a Japanese mission developed and launched by ISAS/JAXA, collaborating with NAOJ as a domestic partner, NASA and STFC (UK) as international partners. Scientific operation of the Hinode mission is conducted by the Hinode science team organized at ISAS/JAXA. This team mainly consists of scientists from institutes in the partner countries. Support for the post-launch operation is provided by JAXA and NAOJ (Japan), STFC (U.K.), NASA, ESA, and NSC (Norway).

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Media contact

Oli Usher
UCL Faculty of Mathematical and Physical Sciences
020 7679 7964
o.usher@ucl.ac.uk

Page last modified on 03 jun 13 14:46