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SOHO's MDI reveals the maelstrom beneath the sunspot

SOHO's MDI reveals the maelstrom beneath the sunspot


Copyright: SOHO/MDI (ESA & NASA)

A cross-section going down 12000 kilometres below the surface of the Sun in the vicinity of a sunspot shows a convergence of cool gas (blue) near the surface. This inflow concentrates the magnetic field and suppresses hot gas (red) trying to rise from below.
Last Update: 1 September 2019
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25-Apr-2024 05:42 UT

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https://sci.esa.int/s/w5bOqJW

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