Sun  ID: 2314

Temperature and Flows under a Sunspot (Layers 0, 2, 4)

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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Visualization Credits

Tom Bridgman (GST): Lead Animator
Junwei Zhao (Stanford University): Scientist
Alexander G. Kosovichev (Stanford University): Scientist
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

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Data Used:
SOHO/Michelson Doppler Interferometer (MDI) also referred to as: SOHO/MDI
NASA and ESA - 2000/08/08-2000/08/10
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.

This item is part of this series:
Spinning Sunspot

Goddard TV Tape:

SVS >> Helioseismology
DLESE >> Space science
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Sunspots
NASA Science >> Sun

GCMD keywords can be found on the Internet with the following citation: Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version