Highlights of the recent progress in understanding the problem of high speed stream evolution with increasing heliocentric distance are reviewed. Crucial to this understanding are the measurements made in the inner solar system by Helios and the outer solar system by Pioneers 10 and 11. When coupled with observations at 1 AU these measurements allow a testing of current theoretical models of stream evolution. 21 references.
Los Alamos Scientific Lab., NM (USA)
Resource Characterization, Forecasting & Maps
Distributed Wind
Utility-Scale Wind
Conference
Gosling, J.T.