The Transition Between Fast and Slow Solar Wind from Composition Data

Details The Transition Between Fast and Slow Solar Wind from Composition Data The Transition Between Fast and Slow Solar Wind from Composition Data

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ssrv...87..353z&link_type=abstract

Space Science Reviews, v. 87, Issue 1/2, p. 353-356 (1999).

Computer Science

21

Coronal Holes, Solar Wind, Ion Composition, Elemental Fractionation, Ulysses, Ace

Scientific paper

The transition between coronal hole associated fast solar wind and slow solar wind is studied using data from the high resolution mass spectrometer SWICS on ACE. We discuss the data in the framework of a recent theory about the global heliospheric magnetic field and conclude that the data are consistent with magnetic connections between field-lines in the fast and in the slow wind.

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