NSF Home IMAGE LIBRARY HOME Contact NSF Image Library How to Use the NSF Image Library
Image Search


IMAGE SEARCH
ALL IMAGES
NEW ADDITIONS TO THE LIBRARY
NEWS IMAGES
NSF SENIOR STAFF
OTHER PHOTO SOURCES

Image: Vorticity and turbulence are mainly confined to the intergranular lanes and downdrafts.  <I>[Image 4 of 4 related images; see also, Solar Convection and Entropy, Entropy Fluctuations, and Solar Granulation.]</I><BR>
<BR>
<U><B>More about this Image</B></U><BR>
Robert Stein, a physics and astronomy professor at Michigan State University, and Aake Nordlund of Copenhagen University Observatory in Denmark, used the National Computational Science Alliance’s SGI Origin2000 supercomputer, located at the National Center for Supercomputing Applications (NCSA), to create massive models of portions of the sun to simulate the processes behind the sun’s smaller-scale features. Using these models, the team focused on understanding convection and magnetic flux near the solar surface. Stein and Nordlund have used supercomputers to study the nature of the sun for more than 15 years.<BR>
<BR>
Rather than create the simulation through a variety of modeling applications, the team uses a single, integrated code. Their code is based on the laws of conservation of mass, momentum, and energy as well as the forces of pressure, gravity, and the magnetic field. Solving the equations that represent these laws and forces allows the researchers to see the essential physics at work, the radiative cooling at the surface that drives convection and the turbulent motions that generate small-scale magnetic fields and shuffle them around, for example.<BR>
<BR>
On four to six Origin2000 processors, it takes about one day to simulate 30 seconds of time on the sun. Eventually, they hope to simulate about one day on the Sun.<BR>
<BR>
Using the team’s newest simulations, they hope to learn how much small-scale magnetic flux is generated by convection, how larger-scale structures are related to granulation, and how to calibrate sound waves to observe phenomena near the solar surface.<BR>
<BR>
This work was supported by grants from the National Science Foundation (grants AST 95-21785 and AST 98-19799), NASA, and the Danish Research Council.<BR>  Thumbnail

Name:

E-mail Address:

Where will the image be used:
NSF requests users to complete an electronic information form documenting the requestor's planned use of the image. This form provides us with valuable tracking information that will help to shape the contents of the image library in the future. We do not retain any personal information (name, email address other than domain name - “.edu,” “.org,” “.com,” “.gov,” etc.) in our files. If you would prefer not to provide your name and email address, type any letter in those boxes. For information about NSF’s Privacy Policy, please see http://www.nsf.gov/home/pubinfo/privacy.htm.


Image Library HomeNSF HomeOffice of Legislative and Public Affairs Home


The National Science Foundation
4201 Wilson Boulevard
Arlington, Virginia 22230, USA
Tel: 703-292-5111
FIRS: 800-877-8339 ~ TDD: 703-292-5090

Last Modified: Jan 31, 2001