EGU2020-12022, updated on 14 Jan 2022
https://doi.org/10.5194/egusphere-egu2020-12022
EGU General Assembly 2020
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Isotropic Scaling Features Measured Locally in the Solar Wind Turbulence with Stationary Background Field

Honghong Wu1, Chuanyi Tu1, Xin Wang2, Jiansen He1, Liping Yang3, and Linghua Wang1
Honghong Wu et al.
  • 1Peking University, School of Earth and Space Sciences, department of geophysics, China (honghongwu@pku.edu.cn)
  • 2School of Space and Environment, Beihang University, Beijing, China
  • 3SIGMA Weather Group, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences,Beijing, China

The scaling anisotropy is crucial to interpret the nonlinear interactions in solar wind turbulence. Previous observations provide diverse results and the structure functions analyses are also reported to be an approach to investigate the scaling anisotropy based on a local magnetic field. However, the determination of the sampling angle with respect to the local background magnetic field implicitly assumes that the observed time series are time stationary. If this assumed time-stationarity is compatible with the measurements has not been investigated. Here we utilize the second-order structure function method to study the scaling anisotropy with a time-stationary background field. We analyze 88 fast solar wind intervals each with time durations >=2 days measured by Wind spacecraft in the period 2005-2018. We calculate the local magnetic field as the average of the time series B(t') whose time-stationarity are fulfilled by our criterion φ<10o (φ is the angle between the two averaged magnetic field after cutting B(t') into two halves). We find for the first time the isotropic scaling feature of the magnetic-trace structure functions with scaling indices -0.63±0.08 and 0.70±0.04 respectively in the local parallel and perpendicular directions. The scaling for the velocity-trace structure functions is also isotropic and the indices are -0.47±0.10  and 0.51±0.09. 

How to cite: Wu, H., Tu, C., Wang, X., He, J., Yang, L., and Wang, L.: Isotropic Scaling Features Measured Locally in the Solar Wind Turbulence with Stationary Background Field, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-12022, https://doi.org/10.5194/egusphere-egu2020-12022, 2020.

Displays

Display file