News From the Field
Super-resolution solar model achieves order out of chaos
March 29, 2016
This material is available primarily for archival purposes. Telephone numbers or other contact information may be out of date; please see current contact information at media contacts.
Over the past few decades, computer models of the Sun's interior have matured, showing that turbulent flows of plasma create a chaotic magnetic tangle. A new study enabled by the Yellowstone supercomputer and published in the journal Science shows for the first time how both large- and small-scale phenomena can be reproduced in some of the highest-resolution simulations ever made.Full StorySource
National Center for Atmospheric Research/University Corporation for Atmospheric Research
The U.S. National Science Foundation propels the nation forward by advancing fundamental research in all fields of science and engineering. NSF supports research and people by providing facilities, instruments and funding to support their ingenuity and sustain the U.S. as a global leader in research and innovation. With a fiscal year 2023 budget of $9.5 billion, NSF funds reach all 50 states through grants to nearly 2,000 colleges, universities and institutions. Each year, NSF receives more than 40,000 competitive proposals and makes about 11,000 new awards. Those awards include support for cooperative research with industry, Arctic and Antarctic research and operations, and U.S. participation in international scientific efforts.
Connect with us online
NSF website: nsf.gov
NSF News: nsf.gov/news
For News Media: nsf.gov/news/newsroom
Statistics: nsf.gov/statistics/
Awards database: nsf.gov/awardsearch/
Follow us on social
Twitter: twitter.com/NSF
Facebook: facebook.com/US.NSF
Instagram: instagram.com/nsfgov