Constraints on Solar Wind Density and Velocity Based on Coronal Tomography and Parker Solar Probe Measurements
Previous work has established an empirical relationship between densities gained from coronal rotational tomography near the ecliptic plane with solar wind outflow speeds at heliocentric distance r _0 = 8 R _⊙ . This work aims to include solar wind acceleration, and thus velocity profiles out to 1 a...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad1506 |