A new approach to analysing the development of magnetic tangles on the Sun has led to a breakthrough in a longstanding debate about how solar energy is injected into the solar atmosphere before being released into space, causing space weather events. The first direct evidence that field lines become knotted before they emerge at the visible surface of the Sun has implications for our ability to predict the behavior of active regions and the nature of the solar interior.
from Latest Science News -- ScienceDaily https://www.sciencedaily.com/releases/2021/07/210722163026.htm
from Latest Science News -- ScienceDaily https://www.sciencedaily.com/releases/2021/07/210722163026.htm
Unravelling the knotty problem of the Sun's activity
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July 23, 2021
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