The Coupling and Evolution of Kelvin–Helmholtz and Rayleigh–Taylor Instabilities in the Heliosheath
The shape and structure of the heliosphere remain subjects of ongoing debate, with current models differing on how far the heliospheric jets that form the two-lobe structure extend down the heliotail and whether the surrounding interstellar medium can penetrate the region between the lobes. Rayleigh...
Saved in:
| Main Authors: | Xiaohan Ma, Merav Opher, Marc Kornbleuth |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ade881 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
On the Anisotropic Velocity Distribution of Newborn Pickup Ions in the Heliosheath
by: Senbei Du, et al.
Published: (2025-01-01) -
Solar Wind–Magnetosphere Coupling by the Kelvin–Helmholtz Instability at Mercury
by: S. H. Lai, et al.
Published: (2024-01-01) -
Large-scale Field-aligned Flows in the Heliosheath
by: Merav Opher, et al.
Published: (2025-01-01) -
Exploring the Complex Heliotail Boundary by an Extended Level Set Approach
by: C. Onubogu, et al.
Published: (2025-01-01) -
Thermodynamic Characterization of Solar Wind Interaction Regions Using PSP Observations: Evidence of Subadiabatic and Superadiabatic States
by: Mohit Shah, et al.
Published: (2025-01-01)