Since it’s quite hard to study the sun, “a team of researchers decided to try to re-create the sun’s magnetic field structure in a ball of plasma in their laboratory.” Although the conditions were obviously quite different and their model incomplete, they did manage to delve deeper into how the magnetic field of the sun works and how our star’s plasma flows through it.
The sun’s magnetic fields form enormous loops that extend from the sun’s surface into space. Some of these loops are small enough to fit entirely within the sun’s corona, while others stretch to the edges of the solar system.
The experiment was also able to mimic a region around the sun where the plasma hangs in a precarious balance. Within this boundary, plasmas are contained by magnetic fields, but outside it, centrifugal forces from the sun’s rotation overpower the magnetic fields, and plasmas stream outward. The researchers found that “if you spin [the plasma] hard enough, you can get it to spin out from centrifugal force.”
Note: The image up top is an image captured from the video in the article, make sure to click through and admire.
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