NASA NTRS · 19890033962
Expected IPS variations due to a disturbance described by a 3-D MHD model
Abstract
The variations of interplanetary scintillation due to a disturbance described by a three-dimensional, time-dependent, MHD model of the interplanetary medium are calculated. The resulting simulated IPS maps are compared with observations of real disturbances and it is found that there is some qualitative agreement. It is concluded that the MHD model with a more realistic choice of input conditions would probably provide a useful description of many interplanetary disturbances.
Keep this discovery
Explore connections, maps & timelines
Tappin, S. J., Dryer, M., Han, S. M., Wu, S. T.. 1988-11-01. Expected IPS variations due to a disturbance described by a 3-D MHD model. https://ntrs.nasa.gov/citations/19890033962
Cite the original work for its findings. Save a collection to share your selection of sources.