JPL Technical Report Server

The Solar Wind in the Third Dimension

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dc.contributor.author Neugebauer, Marcia en_US
dc.date.accessioned 2004-10-03T06:06:23Z
dc.date.available 2004-10-03T06:06:23Z
dc.date.issued 1995-06 en_US
dc.identifier.citation Dana Point, California en_US
dc.identifier.clearanceno 95-1239 en_US
dc.identifier.uri http://hdl.handle.net/2014/31641
dc.description.abstract For many years, solar-wind physicists have been using plasma and field data acquired near the ecliptic plane together with data on the scintillation of radio sources and remote sensing of structures in the solar corona to estimate the properties of the high-latitude solar wind. Because of the highly successful Ulysses mission, the moment of truth is now here. This talk summarizes the principal differences between the Ulysses observations and expectations. en_US
dc.format.extent 255590 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Solar Wind en_US
dc.title The Solar Wind in the Third Dimension en_US


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