A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND

@article{Antiochos2010AMF,
  title={A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND},
  author={Spiro K. Antiochos and Zoran Miki'c and Viacheslav S. Titov and Roberto Lionello and Jon A. Linker},
  journal={The Astrophysical Journal},
  year={2010},
  volume={731}
}
Models for the origin of the slow solar wind must account for two seemingly contradictory observations: the slow wind has the composition of the closed-field corona, implying that it originates from the continuous opening and closing of flux at the boundary between open and closed field. On the other hand, the slow wind also has large angular width, up to ∼60°, suggesting that its source extends far from the open–closed boundary. We propose a model that can explain both observations. The key… 

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