Magnetic Mysteries of Sunspots Decoded
A new computer model could predict "space weather" before it affects earth
Matthias Rempel/UCAR/NCAR |
In July the first complete 3-D sunspot simulation illuminated long-standing questions about these disturbances on the solar surface. Sunspots are strong magnetic regions that disrupt the outward flow of heat from the sun’s interior. As a result they are comparatively cool and so look dark against the 10,000-degree Fahrenheit solar surface. (They still blaze at temperatures near 7,500°F, however.)
This model exposes new details of stellar physics and could make it easier to predict violent “space weather” before it affects Earth. Sunspots often spawn solar flares that can knock out radio communication, damage satellites, and zap power grids.
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