Scale-Dependent Dynamic Alignment in MHD Turbulence: Insights into Intermittency, Compressibility, and Imbalance Effects
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| Autores principales: | , , , , , , , , , |
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| Formato: | Preprint |
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2024
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| _version_ | 1866914858123919360 |
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| author | Sioulas, Nikos Velli, Marco Mallet, Alfred Bowen, Trevor A. Chandran, B. D. G. Shi, Chen Cerri, S. S. Liodis, Ioannis Ervin, Tamar Larson, Davin E. |
| author_facet | Sioulas, Nikos Velli, Marco Mallet, Alfred Bowen, Trevor A. Chandran, B. D. G. Shi, Chen Cerri, S. S. Liodis, Ioannis Ervin, Tamar Larson, Davin E. |
| contents | Scale-Dependent Dynamic Alignment (SDDA) in Elsässer field fluctuations is theorized to suppress nonlinearities and modulate the energy spectrum. Limited empirical evidence exists for SDDA within the solar wind turbulence's inertial range. We analyzed data from the WIND mission to assess the effects of compressibility, intermittency, and imbalance on SDDA. SDDA consistently appears at energy-containing scales, with a trend toward misalignment at inertial scales. Compressible fluctuations show no increased alignment; however, their impact on SDDA's overall behavior is minimal. The alignment angles inversely correlate with field gradient intensity, likely due to "anomalous" or "counterpropagating" wave packet interactions. This suggests that SDDA originates from mutual shearing of Elsässer fields during imbalanced ($δ\boldsymbol{z}^{\pm} \gg δ\boldsymbol{z}^{\mp}$) interactions. Rigorous thresholding on field gradient intensity reveals SDDA signatures across much of the inertial range. The scaling of Elsässer increments' alignment angle, $Θ^{z}$, steepens with increasing global Alfvénic imbalance, while the angle between magnetic and velocity field increments, $Θ^{ub}$, becomes shallower. $Θ^{ub}$ only correlates with global Elsässer imbalance, steepening as the imbalance increases. Furthermore, increasing alignment in $Θ^{ub}$ persists deep into the inertial range of balanced intervals but collapses at large scales for imbalanced ones. Simplified theoretical analysis and modeling of high-frequency, low-amplitude noise in the velocity field indicate significant impacts on alignment angle measurements even at very low frequencies, with effects growing as global imbalance increases. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2407_03649 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Scale-Dependent Dynamic Alignment in MHD Turbulence: Insights into Intermittency, Compressibility, and Imbalance Effects Sioulas, Nikos Velli, Marco Mallet, Alfred Bowen, Trevor A. Chandran, B. D. G. Shi, Chen Cerri, S. S. Liodis, Ioannis Ervin, Tamar Larson, Davin E. Space Physics Solar and Stellar Astrophysics Scale-Dependent Dynamic Alignment (SDDA) in Elsässer field fluctuations is theorized to suppress nonlinearities and modulate the energy spectrum. Limited empirical evidence exists for SDDA within the solar wind turbulence's inertial range. We analyzed data from the WIND mission to assess the effects of compressibility, intermittency, and imbalance on SDDA. SDDA consistently appears at energy-containing scales, with a trend toward misalignment at inertial scales. Compressible fluctuations show no increased alignment; however, their impact on SDDA's overall behavior is minimal. The alignment angles inversely correlate with field gradient intensity, likely due to "anomalous" or "counterpropagating" wave packet interactions. This suggests that SDDA originates from mutual shearing of Elsässer fields during imbalanced ($δ\boldsymbol{z}^{\pm} \gg δ\boldsymbol{z}^{\mp}$) interactions. Rigorous thresholding on field gradient intensity reveals SDDA signatures across much of the inertial range. The scaling of Elsässer increments' alignment angle, $Θ^{z}$, steepens with increasing global Alfvénic imbalance, while the angle between magnetic and velocity field increments, $Θ^{ub}$, becomes shallower. $Θ^{ub}$ only correlates with global Elsässer imbalance, steepening as the imbalance increases. Furthermore, increasing alignment in $Θ^{ub}$ persists deep into the inertial range of balanced intervals but collapses at large scales for imbalanced ones. Simplified theoretical analysis and modeling of high-frequency, low-amplitude noise in the velocity field indicate significant impacts on alignment angle measurements even at very low frequencies, with effects growing as global imbalance increases. |
| title | Scale-Dependent Dynamic Alignment in MHD Turbulence: Insights into Intermittency, Compressibility, and Imbalance Effects |
| topic | Space Physics Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2407.03649 |