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Alfvén Waves in Partially Ionised Solar Steady-State Plasmas
Nada F Alshehri1,2, Istvan Ballai1, Gary Verth1
1Plasma Dynamics Group, School of Mathematical and Physical Sciences, The University of Sheffield, Hicks Building, Hounsfield Road, Sheffield, S3 7RH UK.
Steady flows significantly alter Alfvén waves in partially ionized solar plasmas, affecting their propagation, damping, and even leading to new wave modes due to ion-neutral collisions.
Area of Science:
- Plasma Physics
- Solar Physics
- Astrophysics
Background:
- Alfvén waves are crucial for energy transport in solar plasmas.
- Partial ionization and ion-neutral collisions are common in the solar atmosphere.
- Background flows can significantly influence wave dynamics.
Purpose of the Study:
- Investigate Alfvén wave properties in partially ionized solar plasmas with steady flows.
- Understand how flows and ion-neutral collisions modify wave propagation and damping.
- Explore new wave phenomena induced by these conditions.
Main Methods:
- Employed a two-fluid model treating ions and neutrals as separate, colliding fluids.
- Incorporated background steady flows for both charged and neutral particles.
- Utilized analytical dispersion analysis and numerical solutions.
Main Results:
- Steady flows cause substantial modifications to Alfvén wave properties.
- Observed Doppler shifts, propagation direction reversal, and flow-dependent damping rates.
- Identified a new wave mode linked to neutral flow and collisional coupling, and flow-driven mode conversion.
Conclusions:
- Steady flows and ion-neutral collisions play a critical role in Alfvén wave behavior in the solar atmosphere.
- These interactions lead to complex wave dynamics, including mode conversion.
- Findings provide new insights into energy transport and phenomena in partially ionized solar regions.
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