Physics
Scientific paper
Jul 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..416p&link_type=abstract
Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 416
Physics
4
Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
We present Ulysses solar wind plasma data from the peak southerly latitude of -80.2° through +64.9° latitude on June 7, 1995. Ulysses encountered fast wind throughout this time except for a 43° equatorial band. Mass flux was nearly constant with latitude, while speed (density) had positive (negative) poleward gradients. Momentum flux was highest at high latitudes, suggesting a latitudinal asymmetry in the heliopause cross section. Solar wind energy flux density was also highest at high latitudes.
Bame J. Jr. S.
Feldman William C.
Goldstein Bruce E.
Gosling Jack T.
Hammond Max C.
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