SOHO/MDI Investigates Solar Flows Under Sunspots

  • Released Tuesday, November 6, 2001
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SOHO/MDI performs a 'sonogram' of the sun, revealing the subsurface temperature profile around a sunspot. Red isosurfaces denote regions where the sound speed (and temperature) are higher than average while blue isosurfaces directly under the spot illustrate where the sound speed (and temperature) are lower than average.

Just below the solar surface, we can display isosurfaces of temperature anomalies.  Blue is cooler than average, red is warmer than average, and yellow is just a little warmer than average.

Just below the solar surface, we can display isosurfaces of temperature anomalies. Blue is cooler than average, red is warmer than average, and yellow is just a little warmer than average.

Slate title from video tape reads, 'SOHO/MDI Peers Beaneath Sunspots.'

Slate title from video tape reads, 'SOHO/MDI Peers Beaneath Sunspots.'

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Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio

Release date

This page was originally published on Tuesday, November 6, 2001.
This page was last updated on Wednesday, May 3, 2023 at 1:57 PM EDT.


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Related papers

Zhao, J., Kosovichev, A.G., and Duvall, T.L. 2001, Astrophysical Journal, 557, 384.
Hurlburt, N.E. and Rucklidge, A.M. 2000, Monthly Notices of the Royal Astronomical Society, 314, 793

Zhao, J., Kosovichev, A.G., and Duvall, T.L. 2001, Astrophysical Journal, 557, 384.
Hurlburt, N.E. and Rucklidge, A.M. 2000, Monthly Notices of the Royal Astronomical Society, 314, 793


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