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16th Jul 2006

Sun Tans, Fission and Fusion


Kat Arney

Chris Smith

Rutherford Appleton Laboratory astrophysicist Dr Chris Davis joins us to shed light on the structure and workings of the sun and the newly-launched STEREO mission, Cambridge University engineer Dr Jeffery Lewins talks about nuclear energy and the differences between fusion and fission power, and Dr Anna Nicolaou from the University of Bradford asks why do some people burn whilst others turn brown? On a practical level, in Kitchen Science, Derek and Dave lift the lid on how suncream works.

 

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Science News

 

Atomic Tweezers

Scientists from the University of Bonn have constructed the world's smallest pair of tweezers which are capable of moving atoms around one by one and might hold the key ...

Questions

 

I'd like to know if putting lemon juice on your hair really helps to bleach it, and if so, why?


 

Why is a chilli called a chilli when it's hot?


 

Generally speaking, is the Sun really shrinking at a speed people should be worried about?


 

Are we any closer to working out how geomagnetic fluctuations in the Sun affect our climate?


 

What's the deal with fusion as a power source? Is it ever going to be economically possible? Is cold fusion the answer, or a pipe dream?


 

Sitting in my kitchen which faces west, I can see the sun well up in the sky and I can also see the moon. But the moon still had a shadow on it. Where did the shadow come from if I can see the whole disk of the moon?


 

When I was training to be a nurse, it was drummed into us that vitamin D comes from the sun. If we're all neurotic about putting sunblocks on, will we not have a lot of people suffering from SAD (seasonal affective disorder)?


 

I know that there is a wide range of frequencies in the electromagnetic radiation that comes from the sun. But exactly how many discrete frequencies are there, and what determines the frequency radiated?


 

It's my understanding that you can send electricity wirelessly. Although microwaves are apparently the best way, even radio waves contain small traces of electricity. So if the Sun emits a huge and powerful spectrum of radio waves and other kinds of electromagnetic waves, would it not be possible to pick up this free energy using a big antenna?


 

How does light actually propagate? I know that there are perpendicular electrical and magnetic fields and that they can induce other fields in space and this keeps going on so that light travels. Is this correct? Are there any differences between these magnetic fields?


 

Does the Sun move and what impact could the movement of the Sun and changes in velocity have on things like other planets?


 

Why do you sneeze when you look at the Sun?


Interviews

 

Paralysed Let Their Thoughts Wander...

Dr John Donoghue, Brown University
 

Science Update Frog's Legs and Gunshots

Chelsea Wald and Bob Hirshon from AAAS, the science society.
 

Seeing The Sun in Stereo

Dr Chris Davis, Rutherford Appleton Laboratory
 

Nuclear Energy: Fission And Fusion

Dr Jeffery Lewins, University of Cambridge
 

The Science of Sun Burn

Dr Anna Nicolaou, University of Bradford

Kitchen Science

 

How does sun cream work?


With the summer holidays approaching, Derek and Dave head off to Hinchingbrooke School to find out why wearing the white stuff is the cool thing to do.

Fact or Fiction

Human fingernails grow about 4 centimetres per year
TrueTrue
Europe is the only continent without a desert
TrueTrue
You can calculate the distance to the horizon in miles by multiplying 1.22 by the square root of the height of your eyes above the ground
TrueTrue
In 1992 2500 Americans were hospitalised by house plants
TrueTrue

Sun Tans, Fission and Fusion - More about this podcast

STEREO spacecraft A

At school they teach us that energy cannot be made or destroyed and that all energy comes from the sun. The power of the sun however, is even huger than its magnificent size of …

The Sun is not fully understood and the more we learn about, it the more we can do with its power - the relationship between the sun and plants is well understood and as is the process by which the sun gives energy. The power of the sun has already been used for a variety of things; from solar powered calculators to providing electricity to homes. On this week's show we will have Davis explaining how he hopes to learn more about the Sun, Lewins talking about how he plans to use the Suns energy and X describing the effects of too much Sun on people who have been basking in its glow a little too long.

The Solar TErrestrial RElations Observatory (or STEREO to its pals) is the third mission in NASA's Solar Terrestrial Probes Programme (STP). This two year mission will provide a new view of the Earth-Sun system. It involves two almost identical observatories (one is shown in figure 1); one ahead of Earth in its orbit and one trailing behind, they will trace the flow of energy and matter from the Sun to Earth as well as reveal the 3D structure of Coronal Mass Ejections (more about these later) and why they happen. STEREO will also provide alerts for Earth-directed solar ejections, from its unique side-viewing perspective adding it to the fleet of Space Weather detection satellites.

So we does Earth need STEREO? Well coronal mass ejections (or CMEs to their enemies - as shown in figure 2) are powerful eruptions that can blow up to 10 billion tons of the Sun's atmosphere into interplanetary space. They are erupted at speeds of around one million miles per hour and can create major disturbances in the interplanetary medium and trigger severe magnetic storms when they collide with Earth's magnetosphere. Large geomagnetic storms can damage or destroy satellites and pose a serious threat to astronauts when outside of the protection of the Space Shuttle or the International Space Station and have been known to cause electrical power outages.

Solar ejections are the most powerful drivers of the Sun-Earth connection. Despite their importance little is known about their origin or evolution - STEREO which will be able to take stereoscopic (3D) images of the structure of CMEs will enable scientists to learn more about this.

The UK's involvement in this project is through the Heliospheric Imager (affectionally known as HI) which is just one of the instruments on board the space craft. Chris Davis will be on the show to talk about his involvement in HI at the Rutherford Appleton Laboratory and will be talking about the Sun's 11 year activity cycle and CMEs. The Laboratory has provided the detectors for all of the cameras onboard the STEREO spacecraft and is leading the scientific management of the HI instruments. The two instruments were built in the UK by a team at the University of Birmingham led by Dr Chris Eyles. Each HI consists of two wide-field white light cameras housed in a carbon fibre box around 70cm long. The combined field of view of these cameras is 90o the instruments are positioned facing Earth on the side of each of the STEREO spacecraft; so that their field-of-view spans from just off the limb of the Sun to beyond the orbit of the Earth. As a result, they will be able to detect any CMEs heading towards the Earth.

The UK has a world-leading reputation in the field of solar science and the Rutherford Appleton Laboratory is working with UK universities to fully exploit data from the STEREO mission especially the HIs. Understanding CMEs is the primary goal, however, two wide-field cameras in space represent a fantastic opportunity tostudy a wide variety of objects. UK academics have come up with proposals to use HI data to investigate many of these - from comets to extra solar planets.

So when does it all blast off? Well currently NASA are saying no earlier than the 30th July, you can keep up to date with the mission by logging on to their website and following links to STEREO via the missions page.

Right, that's the space mission, but what else is on the show? As mentioned earlier Dr Jeffrey Lewins of Cambridge University will be talking about thermodynamics and his work with nuclear power. He has worked for fusion programme at Culham and was President of the Institute of Nuclear Engineers. He will be talking about his work which involves the applied mathematics of fission reaction calculations and his interest in comparing the practicalities of producing electricity from either nuclear fission or nuclear fusion.

Finally Dr Anna Nicolaou from the University of Bradford; will be explaining the science of sunburn - the difference between UVA and UVB radiation, why some people tan easily whilst others do not and possible future sunburn protection.



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