NASA NTRS · 19830012592
Convective dynamos for rotating stars
Abstract
Global dynamo theory is applied to the problem of why some stars have field reversing dynamos, and others do not. It is argued that convectively driven dynamos are the most likely source of magnetic fields in stars that have convection zones.
Keep this discovery
Explore connections, maps & timelines
Gilman, P. A.. 1981-01-01. Convective dynamos for rotating stars. https://ntrs.nasa.gov/citations/19830012592
Cite the original work for its findings. Save a collection to share your selection of sources.