Solar prominences hover above the visible solar disk like giant clouds, held there by a supporting framework of magnetic forces, originating from layers deep within the Sun. The magnetic lines of force are moved by ever-present gas currents -- and when the supporting framework moves, so does the prominence cloud. A research team has observed how magnetic forces lifted a prominence by 25,000 kilometers -- about two Earth diameters -- within ten minutes.
from Latest Science News -- ScienceDaily https://www.sciencedaily.com/releases/2021/10/211013114104.htm
from Latest Science News -- ScienceDaily https://www.sciencedaily.com/releases/2021/10/211013114104.htm
How the Sun’s magnetic forces arrange gas particles
Reviewed by cmakigo
on
October 14, 2021
Rating:
No comments:
Post a Comment