
The movie shows the turbulent, “boiling” gas that covers the entire sun. The cell-like structures – each about the size of Texas – are the signature of violent motions that transport heat from the inside of the sun to its surface.
Hot solar material (plasma) rises in the bright centers of “cells,” cools off and then sinks below the surface in dark lanes in a process known as convection. In these dark lanes we can also see the tiny, bright markers of magnetic fields.
Never before seen to this clarity, these bright specks are thought to channel energy up into the outer layers of the solar atmosphere called the corona. These bright spots may be at the core of why the solar corona is more than a million degrees!
This movie covers an area 36,500 × 36,500 km (22,600 × 22,600 miles, 51 × 51 arcseconds).
Credit: NSO/NSF/AURA
Highest resolution observations of the Sun’s surface ever taken
byu/Busy_Yesterday9455 inspaceporn
