Ion Charge States from a Global Time-dependent Wave-turbulence-driven Model of the Solar Wind: Comparison with in Situ Measurements
Solar wind charge-state measurements contain a wealth of knowledge related to the properties of the solar corona from where they originated. However, their interpretation has remained challenging because it convolves coronal temperature, density, and velocity along the particles’ trajectory through...
Saved in:
| Main Authors: | Pete Riley, Roberto Lionello, Yeimy J. Rivera |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ada253 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Impulsively Accelerated Ions as the Source of Ion Acoustic Waves in Solar Wind
by: R. E. Ergun, et al.
Published: (2024-01-01) -
The Effect of Turbulence on the Angular Momentum of the Solar Wind
by: Rohit Chhiber, et al.
Published: (2025-01-01) -
Evolution of Solar Wind Turbulence during Radial Alignment of Parker Solar Probe and Solar Orbiter in 2022 December
by: Ashok Silwal, et al.
Published: (2025-01-01) -
Decay of Turbulent Upper-hybrid Waves in Weakly Magnetized Solar Wind Plasmas
by: F. J. Polanco-Rodríguez, et al.
Published: (2025-01-01) -
Evidence for a Link between Turbulence and the Generation of Ion Cyclotron Waves via the Helicity Barrier Effect in the Solar Wind
by: Utsav Panchal, et al.
Published: (2025-01-01)