NASA NTRS · 19910070461
Radial evolution of interaction regions
Abstract
Near and outside 1 AU, corotating interaction regions bounded by shocks form at the leading edges of high-speed streams. This paper describes the radial evolution of interaction regions, the merging of interaction regions belonging to neighboring streams, and the coalescence of interaction regions belonging to successive solar rotations.
Keep this discovery
Explore connections, maps & timelines
Whang, Y. C., Burlaga, L. F.. 1990-01-01. Radial evolution of interaction regions. https://ntrs.nasa.gov/citations/19910070461
Cite the original work for its findings. Save a collection to share your selection of sources.