A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2006; you can also visit the original URL.
The file type is
Physics of Space: Growth Points and Problems
Solar wind measurements on board several spacecraft were used to study the two-points correlations of the solar wind plasma structures. The factors having the most influence on the correlation level are the density variability and IMF cone angle. The characteristic length of large solar wind structures is estimated at 500-1000 R E .doi:10.1007/978-94-010-0904-1_42 fatcat:djniuanwbffgrew34p65pogpm4