Origin of the solar wind from composition data

@article{Geiss1995OriginOT,
  title={Origin of the solar wind from composition data},
  author={Johannes Geiss and G. Gloeckler and Rudolf von Steiger},
  journal={Space Science Reviews},
  year={1995},
  volume={72},
  pages={49-60}
}
The ESA/NASA spacecraft Ulysses is making, for the first time, direct measurements in the solar wind originating from virtually all places where the corona expands. Since the initial two polar passes of Ulysses occur during relatively quiet solar conditions, we discuss here the three main regimes of quasi-stationary solar wind flow: the high speed streams (HSSTs) coming out of the polar coronal holes, the slow solar wind surrounding the HSSTs, and the streamers which occur at B-field reversals… 

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