NASA NTRS · 20010055708
Chinks in Solar Dynamo Theory: Turbulent Diffusion, Dynamo Waves and Magnetic Helicity
Abstract
We have investigated the generation of magnetic fields in the Sun using two-dimensional and three-dimensional numerical simulations. The results of our investigations have been presented at scientific meetings and published.
Keep this discovery
Explore connections, maps & timelines
DeLuca, E. E., Wagner, William J.. 2001-01-31. Chinks in Solar Dynamo Theory: Turbulent Diffusion, Dynamo Waves and Magnetic Helicity. https://ntrs.nasa.gov/citations/20010055708
Cite the original work for its findings. Save a collection to share your selection of sources.