Our Sun is a maelstrom of light and heat, a constant battlefield for plasma and magnetic fields. This recent prominence, captured by Andrea Vanoni and others, bore a striking triangular shape. This fiery outburst — larger than our entire planet — formed and broke up over the course of a single day. The wavy solar surface features in the lower part of the image are solar fibrils, magnetically confined tubes of hot plasma. What changing magnetic fields might allow them to burst forth in a glorious candle of their own? (Image credit: A. Vanoni; via APOD)
Tag: prominence
Solar Flare
An M-class solar flare with a towering prominence erupted from the Sun over the course of three hours in late September. Notice how the plasma does not fall straight back to the surface but flows back down following the Sun’s magnetic field lines. As an rarefied ionized gas, plasma follows coupled laws of electromagnetism and fluid dynamics. #
Solar Fluid Dynamics
The sun is a wild place fluid dynamically. The surface is riddled with convection cells the size of the Earth, and prominences of plasma (ionized gas) erupt from the surface following the sun’s magnetic field lines. Violent, but beautiful. #
