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Figure 3. Identification of the solar wind flow state, as given by the proton bulk speed and density (projected to 1 AU), measured by Ulysses during its fast latitude scan, compared with the configuration of the solar corona, as measured in soft X rays by Yohkoh. Yohkoh data was kindly provided by the Yohkoh mission of ISAS, Japan. [an error occurred while processing this directive]

Last Modified $Date: 2004-08-04 14:11:02-06 $