Temperature and Flows under a Sunspot (Layers 0, 2, 4)
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Using the SOHO Michelson Doppler Interferometer (MDI), scientists can use a process called Time-Distance helioseismology to determine temperatures and fluid flows under the surface of the Sun.
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Zoom into the sunspot and reveal temperature and flow profiles revealed by time-distance helioseismology.
Duration: 9.0 seconds
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Temperature anomalies (color) and flow directions at the solar surface. The darker blue region corresponds to the sunspot itself.
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Layer 5000 kilometers below the solar surface.
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2 MB
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23 KB
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7 KB
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Layer 9000 kilometers below the solar surface.
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1 MB
320 x 240
JPEG
20 KB
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None
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150 KB
320 x 234
PNG
254 KB
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