Video of Exploding Sunspot

Note the magnetic alignment of the sunspot is angle up and to the right. Note how the magnetic field has two lobes: one to the upper right of the bright sunspot; one to the lower left of the bright sunspot. If the Ball-of-Light Particle Model is correct, then the magnetic pole that is closest to the core -- the pole on the upper right -- is angled down below the surface. If a ball-of-light is ejected from this pole of the sunspot, then it should be angled down. Note how the shock wave sweeps across the surface of the sun after the explosion. Note how the shock wave expands from the center of the upper right lobe of the magnetic field -- not from the center bright spot. Note how the sunspot is still there after the explosion. What this means is that only part of the sunspot decayed with a split decay mode. The main ball-of-light that is floating in the sun's outer plasma is still there after the explosion. What exploded was a smaller ball-of-light that was induced off the pole of the larger ball-of-light. It was ejected in the direction up and to the right. If the Ball-of-Light Particle Model is correct, then the explosion should occur under the surface of the sun causing a solar mass ejection. Note how a relatively small solar mass ejection occurs after the initial shock wave pass over the surface of the sun. What this means is that the smaller ball-of-light ejected from the large ball-of-light at the center of the sunspot did explode underneath the surface of the sun rather than above the surface of the sun. (See also, Another Exploding Sunspot, Stellar Impact, and an example of a larger ball-of-light inducing another smaller ball-of-light.)