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Harnessing the power of the Sun: fusion reactors - Science in School

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<strong>Science</strong> topics<br />

would o<strong>the</strong>rwise erode quickly), <strong>the</strong><br />

plasma needs to be kept away from<br />

<strong>the</strong> reactor walls. To do this, <strong>fusion</strong><br />

scientists exploit <strong>the</strong> Lorentz force<br />

experienced by a mov<strong>in</strong>g charged<br />

particle when a magnetic field, is applied.<br />

This force is perpendicular to<br />

both <strong>the</strong> particle’s direction <strong>of</strong> travel<br />

and <strong>the</strong> magnetic field, and <strong>the</strong>refore<br />

causes <strong>the</strong> particle to rotate around<br />

<strong>the</strong> magnetic field l<strong>in</strong>e. As a result, <strong>the</strong><br />

particle spirals around <strong>the</strong> field l<strong>in</strong>e –<br />

with electrons and nuclei mov<strong>in</strong>g <strong>in</strong><br />

opposite directions (Figure 3).<br />

The most advanced magnetic<br />

conf<strong>in</strong>ement design is <strong>the</strong> tokamak,<br />

a r<strong>in</strong>g-shaped vacuum chamber surrounded<br />

by coils. An electric current<br />

flow<strong>in</strong>g through one set <strong>of</strong> coils (<strong>the</strong><br />

toroidal field coils, Figure 4) generates<br />

a r<strong>in</strong>g-shaped magnetic field. The<br />

strength <strong>of</strong> this toroidal (doughnutshaped)<br />

field is not uniform across<br />

<strong>the</strong> r<strong>in</strong>g, because <strong>the</strong> coils are closer<br />

toge<strong>the</strong>r on <strong>the</strong> <strong>in</strong>side <strong>of</strong> <strong>the</strong> torus<br />

(doughnut). Therefore <strong>the</strong> particles<br />

experience a stronger Lorentz force on<br />

<strong>the</strong> <strong>in</strong>ner side <strong>of</strong> <strong>the</strong> field l<strong>in</strong>e around<br />

which <strong>the</strong>y are rotat<strong>in</strong>g. As a result,<br />

<strong>the</strong>y gradually drift away from <strong>the</strong>ir<br />

field l<strong>in</strong>e towards <strong>the</strong> plasma edge.<br />

To reduce this effect, a second<br />

magnetic field, <strong>the</strong> poloidal field, is<br />

generated. This helical field w<strong>in</strong>ds<br />

<strong>in</strong> spirals around <strong>the</strong> plasma and<br />

conf<strong>in</strong>es it very effectively. The easiest<br />

way to generate a poloidal field is<br />

with a plasma current. That <strong>in</strong> turn<br />

is generated when <strong>the</strong> plasma particles<br />

travel along <strong>the</strong> r<strong>in</strong>g around <strong>the</strong><br />

toroidal field l<strong>in</strong>es – electrons and ions<br />

mov<strong>in</strong>g <strong>in</strong> opposite directions. Like<br />

a wire, this current creates a r<strong>in</strong>gshaped<br />

magnetic field around itself. It<br />

is <strong>in</strong>duced by a transformer <strong>in</strong> which<br />

<strong>the</strong> plasma itself acts as a secondary<br />

coil around a large primary coil (<strong>the</strong><br />

<strong>in</strong>ner poloidal field coils). Because<br />

<strong>the</strong> plasma tends to drift vertically, an<br />

additional magnetic field created by<br />

<strong>the</strong> outer poloidal field coils is used to<br />

control its position and shape.<br />

Will future <strong>power</strong> stations<br />

be <strong>power</strong>ed by <strong>fusion</strong>?<br />

The <strong>Sun</strong>, as imaged<br />

by <strong>the</strong> Extreme<br />

Ultraviolet Imag<strong>in</strong>g<br />

Telescope aboard <strong>the</strong><br />

Solar and Heliospheric<br />

Observatory<br />

(SOHO), stationed<br />

1.5 million kilometres<br />

from Earth<br />

Image courtesy <strong>of</strong> spectacle productions; image source: Flickr<br />

Image courtesy <strong>of</strong> ESA, NASA, SOHO / EIT team<br />

www.science<strong>in</strong>school.org <strong>Science</strong> <strong>in</strong> <strong>School</strong> I Issue 22 : Spr<strong>in</strong>g 2012 I 45

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