The auroras at Earth’s poles are much more than pretty lights. This video explains their formation; fluid mechanics (specifically magnetohydrodynamics) play a major role in the convective transport of heat inside the sun as well as the movement of the plasma that makes up a solar storm that interacts with Earth’s magnetic field and produces the auroras.
Tag: plasma
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. #
Solar Prominence
[original media no longer available]
In this stunning video of a solar flare and prominence captured by NASA’s SDO mission, plasma erupts from the surface of the sun preceded by a massive shockwave (near center of frame, heading downward). The motion of the plasma is dictated not only by classical fluid mechanics but by the influence of the sun’s magnetic field in what is known as magnetohydrodynamics. (submitted by Caleb)
Plasma Demo
This neat magnetohydrodynamic (MHD) demo is one we do not suggest repeating at home. The high voltage applied across the magnets and the plate causes the white disk in between to vaporize and form a plasma. Then the magnetic field causes the circumferential motion via the Lorentz force, essentially trapping the plasma and making it spin.
Calcium Plasma on the Sun
This high-resolution photo of our sun shows the structure of calcium plasma on the surface of the sun. Plasmas are governed by the same physics as our familiar earthbound fluids but are also extremely sensitive to magnetic fields. Their branch of fluid dynamics is often referred to as magnetohydrodynamics (MHD), where the Navier-Stokes equations have to be solved in conjunction with Maxwell’s equations. (via Bad Astronomy)
Magnetohydrodynamics
Fluid dynamics play an important role in understanding phenomena like sunspots and solar prominences. The subfield of fluid dynamics concerned with the motion of electrically conducting fluids, like the plasma that makes up the sun’s corona, is magnetohydrodynamics.
