At the beginning, in 1997 the video shows the sun in Solar Cycle 23 with its positive polarity on the top (the green lines), and the negative polarity on the bottom (the purple lines).
Each set of lines gradually move toward the opposite pole, showing a complete flip around 2002, completing the sun's previous cycle.
Both set of lines representing the opposing magnetic fields then begin to work their way back, to culminate in the latest flip.
"At the height of each magnetic flip, the sun goes through periods of more solar activity, during which there are more sunspots, and more eruptive events such as solar flares and coronal mass ejections," said Nasa’s Karen C. Fox.
"Cosmic rays are also affected," added Dr. Phillips. "These are high-energy particles accelerated to nearly light speed by supernova explosions and other violent events in the galaxy."
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