THE OXYGEN CHARGE-STATE RATIO AS AN INDICATOR OF FOOTPOINT FIELD STRENGTH IN THE SOURCE REGIONS OF THE SOLAR WIND
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/833/i=1/a=121/pdf
Reference28 articles.
1. Slow Solar Wind: Observations and Modeling
2. Quantifying the Difference Between the Flux-Tube Expansion Factor at the Source Surface and at the Alfvén Surface Using a Global MHD Model for the Solar Wind
3. Self‐consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence
4. Coincidence of composition and speed boundaries of the slow solar wind
5. Comparison of interplanetary signatures of streamers and pseudostreamers
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1. Compositional Metrics of Fast and Slow Alfvénic Solar Wind Emerging from Coronal Holes and Their Boundaries;The Astrophysical Journal;2024-07-01
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3. The S-Web Origin of Composition Enhancement in the Slow-to-moderate Speed Solar Wind;The Astrophysical Journal;2023-05-01
4. Matching Temporal Signatures of Solar Features to Their Corresponding Solar-Wind Outflows;Solar Physics;2021-04
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