Damped Kinetic Alfvén Waves in Earth's Magnetosheath: Numerical Simulations and MMS Observations
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arXiv
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| Autori principali: | , , , , |
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| Natura: | Preprint |
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2025
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| _version_ | 1866915666561335296 |
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| author | Chettri, Mani K. Singh, Hemam D. Shrivastav, Vivek Singh, Britan Mukherjee, Rupak |
| author_facet | Chettri, Mani K. Singh, Hemam D. Shrivastav, Vivek Singh, Britan Mukherjee, Rupak |
| contents | The Earth's magnetosheath provides a high $β$ (ratio of electron thermal pressure to magnetic pressure) plasma environment where kinetic Alfvén waves (KAWs) strongly influence turbulence and energy dissipation. This study investigates how Landau damping modifies the nonlinear evolution of KAWs by solving a modified nonlinear Schrödinger equation that captures both dispersive and nonlinear effects. Without Landau damping, modulational instability drives rapid self-focusing into intense magnetic filaments, producing a turbulent cascade with $k_\perp^{-5/3}$ scaling in the inertial range ($k_\perpρ_i<1$) that transitions to $k_\perp^{-8/3}$ at sub-ion scales ($k_\perpρ_i>1$), here $k_\perp$ is the wavevector component perpendicular to the background magnetic field and $ρ_i$ the ion thermal gyroradius. When Landau damping is included, magnetic structures are significantly suppressed, and the spectrum steepens to $k_\perp^{-11/3}$ in the sub-ion range while the inertial range maintains $k_\perp^{-5/3}$ scaling. The damping acts across all scales through resonant wave-particle interactions, efficiently transferring energy from waves to particles. Direct comparison with Magnetospheric Multiscale (MMS) spacecraft observations shows that the observed kinetic range spectral slope falls between our undamped and damped simulation limits, consistent with an intermediate damping regime in magnetosheath turbulence. This agreement confirms that Landau damping is one of the primary mechanisms controlling turbulent energy dissipation at kinetic scales in collisionless plasmas. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_09828 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Damped Kinetic Alfvén Waves in Earth's Magnetosheath: Numerical Simulations and MMS Observations Chettri, Mani K. Singh, Hemam D. Shrivastav, Vivek Singh, Britan Mukherjee, Rupak Plasma Physics Space Physics The Earth's magnetosheath provides a high $β$ (ratio of electron thermal pressure to magnetic pressure) plasma environment where kinetic Alfvén waves (KAWs) strongly influence turbulence and energy dissipation. This study investigates how Landau damping modifies the nonlinear evolution of KAWs by solving a modified nonlinear Schrödinger equation that captures both dispersive and nonlinear effects. Without Landau damping, modulational instability drives rapid self-focusing into intense magnetic filaments, producing a turbulent cascade with $k_\perp^{-5/3}$ scaling in the inertial range ($k_\perpρ_i<1$) that transitions to $k_\perp^{-8/3}$ at sub-ion scales ($k_\perpρ_i>1$), here $k_\perp$ is the wavevector component perpendicular to the background magnetic field and $ρ_i$ the ion thermal gyroradius. When Landau damping is included, magnetic structures are significantly suppressed, and the spectrum steepens to $k_\perp^{-11/3}$ in the sub-ion range while the inertial range maintains $k_\perp^{-5/3}$ scaling. The damping acts across all scales through resonant wave-particle interactions, efficiently transferring energy from waves to particles. Direct comparison with Magnetospheric Multiscale (MMS) spacecraft observations shows that the observed kinetic range spectral slope falls between our undamped and damped simulation limits, consistent with an intermediate damping regime in magnetosheath turbulence. This agreement confirms that Landau damping is one of the primary mechanisms controlling turbulent energy dissipation at kinetic scales in collisionless plasmas. |
| title | Damped Kinetic Alfvén Waves in Earth's Magnetosheath: Numerical Simulations and MMS Observations |
| topic | Plasma Physics Space Physics |
| url | https://arxiv.org/abs/2512.09828 |