![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiWj4aRRy5C710sA6HdVfB7JeRtbH8E3t2GSWMdPFyk9XhvmNYHvjc-bVeAGOzGBectW3mtIlT4j-wCIhRF6fvCC5ZxXbrztsivzHqW1FMp9fCFLzif17rqndo-WqCt2ZkVd2g5TEIhXSY/s320/active_region_A.jpg)
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhYNvG1ELv4YjPQc5C_Z6dNb2kM_WnSmUT351ELUto6rUM4KA4Sy2Z2uA6BxrWLp_HU9P3NO3fLtENyM8w3LvsHwwZBcJDr4br5szAU3XpFTYqZI-dMAfpKJ1uI_W7GwiKS6pbrBxURv7Q/s320/active_region_B.jpg)
I worked closely with Brad Hindman from the Juri Toomre Group; he came to me about doing some figures for a paper he was publishing titled "Subsurface Circulations within Active Regions" for The Astrophysical Journal. Brad does a lot with Laboratory for Computational Dynamics (
LCD) which supports fundamental research on helioseismology and convection and dynamo theory. The scientists at LCD study the dynamics inside stars with helioseismology and design large-scale computer simulations of convection, turbulence, and dynamo processes within stars. They work on a pretty intense TeraGrid network which is basically clusters of supercomputers tied together across the nation. Its pretty neat stuff!
I just realized that this is my first published astrophysics project. I'm breaking into the astrophysics scene!
The full citation for the paper is:
Subsurface Circulations within Active Regions
Bradley W. Hindman, Deborah A. Haber, and Juri Toomre 2009 ApJ 698 1749-1760 doi: 10.1088/0004-637X/698/2/1749Clients: Juri Toomre Group and Brad HindmanRelated Links: The Astrophysical Journal
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