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Sun Facts

Magnetic Sun:
Magnetic Loops in the Sun's Corona

Another important property of magnetic fields is that they trap and contain  hot gases. They are, in effect, "magnetic bottles". On earth, laboratory experiments to produce energy from controlled fusion depend on this property of  magnetic fields to contain the super-hot gases. Magnetic fields can be thought  of as lines that connect north and south polarities. On the Earth these lines  run from north to south and are uniform and organized. This is why we can  navigate so well with a magnetic compass. On the sun, the magnetic fields  connect opposite polarities just as on the Earth. However, while the Earth only  has one north and one south pole, on the Sun we observe bits of north and south  polarity scattered all over the surface. Furthermore, their position and strengths are constantly changing. The magnetic fields connecting these poles loop out into the corona in a bewildering array of shapes and sizes. They are  visible in X-rays because of the hot gas that they trap. When some of the Sun's magnetic field lines are filled with hot gas, we see a  magnetic loop:


Compare this to an actual picture of the Sun from  Yohkoh:



Below is a set of 7 pictures illustrating the magnetic loops of the Sun's corona. All of the complex structure seen in these pictures reflect the way the magnetic fields are oriented at that location. The white tick marks in the pictures are each the  same length on the Sun, though the image scale varies from picture to picture. The ticks represent a distance of about 43,500 km or 3% the diameter of the Sun. In frames A, B, C, and G you can see the edge, or limb, of the Sun as a dark or bright smooth segment of a circle.

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