Physics – Plasma Physics
Scientific paper
Aug 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jgra..107.1178p&link_type=abstract
Journal of Geophysical Research (Space Physics), Volume 107, Issue A8, pp. SSH 6-1, CiteID 1178, DOI 10.1029/2002JA009331
Physics
Plasma Physics
9
Interplanetary Physics: Interplanetary Magnetic Fields, Interplanetary Physics: Mhd Waves And Turbulence, Interplanetary Physics: Solar Cycle Variations (7536), Space Plasma Physics: Turbulence, Space Plasma Physics: Nonlinear Phenomena
Scientific paper
The Ulysses spacecraft, in a polar orbit of the Sun, has now completed two fast latitude scans, one at solar minimum and one at solar maximum. We have performed a comparison of the intermittent properties of the high frequency solar wind magnetic field components at these different levels of activity, using the well known P-Model. At solar minimum, tests indicated a high level of intermittency in the fast coronal hole solar wind, and a varied structure in the slow wind, with mean lower level of intermittency than in fast wind. At solar maximum, slow wind dominated the heliosphere and the parameters show high variability throughout the scan, as for slow wind at solar minimum, indicating that intermittency is probably dependent on the details of the origin of the slow wind plasma.
Balogh André
Pagel Christina
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