Global distribution of the solar wind during solar cycle 23: ACE observations

By L. Zhao, T. Zurbuchen, L. Fisk. 2009

137 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/33bb9722bda261d7b081290edf3f5dda5f5c0f9f

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In Astronomy and Astrophysics

1. Roberto Lionello
2. Jon A. Linker
3. Zoran Mikic
4. S. Antiochos
5. E. Kilpua
6. A. Balogh
7. V. Titov
8. Ying Liu

Citations in the corpus

• Slow Solar Wind: Observations and Modeling (2016, unknown): “Zhao et al. (2009) categorized the slow wind by the O7+/O6+ ion density ratios of 0.145 and above, excluding ICME periods when very high ionic charge states are common.”
• A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND (2010, background): “But this wind has photospheric FIP ratios, so it is still considered to be “fast wind” (Zhao et al. 2009).”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, methodology): “The charge states “freeze-in” at the distance of a few solar radii from the Sun when the propagation time of the solar wind is short compared to the recombination-ionisation time-scale (e.g., Zhao et al. 2009).”