Sun  ID: 10583

Slices Through the Solar Interior

Scientists using SOHO/MDI data have looked just below the Sun's surface and clearly observed inward flowing material.

The strong magnetic fields in the sunspots promote cooling. Cool material contracts and sinks at speeds of up to 3000 miles per hour. This drives an inward flow, like a planet-sized whirlpool, that holds the sunspot together as long as the field is strong enough. Scientists discovered this using a technique called acoustic tomography - a novel method similar to ultrasound diagnostics in medicine that uses sound waves to image structures inside the human body. Scientists also found that sunspots are surprisingly shallow. Conditions in sunspots change from cooler than the surrounding plasma to hotter than the surrounding plasma just 3000 miles below the surface. The cool part of a sunspot has the shape of a stack of two or three nickels. Sunspot magnetic fields block the flows that carry heat energy up from the hot solar interior. That results in higher temperatures below the blockage and cooler temperatures above. The downward flows mentioned above dissipate at the same depth. With these data one cannot get a sharp enough picture to really explain the details. Understanding sunspots is essential for understanding the 11-year solar cycle, solar flare explosions, and huge coronal mass ejections that affect life and society on Earth.


For More Information

http://soi.stanford.edu/press/ssu11-01/


Credits

Alexander G. Kosovichev (Stanford University): Animator
Scott Wiessinger (UMBC): Video Editor
Alexander G. Kosovichev (Stanford University): Scientist
Please give credit for this item to:
Alexander Kosovichev (Stanford University)

Science Paper:
(J. Zhao, A.G. Kosovichev, T.L. Duvall, Jr. 2001, Investigation of Mass Flows beneath a Sunspot by Time-Distance Helioseismology , Ap. J., 557, 384-388)

Short URL to share this page:
http://svs.gsfc.nasa.gov/10583

Mission:
SOHO

Data Used:
SOHO/Michelson Doppler Interferometer (MDI)
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.

Keywords:
SVS >> Helioseismology
SVS >> SOHO
SVS >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Sunspots
GCMD >> Location >> Solar Interior
SVS >> Heliophysics
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 8.0.0.0.0