NASA NTRS · 19940020011
Model development for Ulysses and SOHO
Abstract
The purpose of this research is to provide scientific expertise in solar physics and in the development and use of magnetohydrodynamic (MHD) models of coronal structures for the computation of Lyman alpha scattered radiation in these structures. The specific objectives will be to run MHD models with new boundary conditions and compute resulting scattered solar Lyman alpha intensities, guided by results from the first series of boundary conditions.
Keep this discovery
Explore connections, maps & timelines
Wu, S. T.. 1993-11-27. Model development for Ulysses and SOHO. https://ntrs.nasa.gov/citations/19940020011
Cite the original work for its findings. Save a collection to share your selection of sources.