25 citations · 60 across the 3 of their papers we have counts for
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Isotropic Scaling Features Measured Locally in the Solar Wind Turbulence with Stationary Background Field
Honghong Wu, Chuanyi Tu, Xin Wang +3
The scaling anisotropy is crucial to interpret the nonlinear interactions in solar wind turbulence. Previous observations provide diverse results and the structure function analyse…
Energy Supply for Heating the Slow Solar Wind Observed by Parker Solar Probe between 0.17 and 0.7 au
Honghong Wu, Chuanyi Tu, Xin Wang +2
Energy supply sources for the heating process in the slow solar wind remain unknown. The Parker Solar Probe (PSP) mission provides a good opportunity to study this issue. Recently,…
Magnetic Energy Transfer and Distribution between Protons and Electrons for Alfvénic Waves at Kinetic Scales in Wavenumber Space
Die Duan, Jiansen He, Honghong wu +1
Turbulent dissipation is considered a main source of heating and acceleration in cosmological plasmas. The alternating current Joule-like term, , is used…
Dependence of 3D Self-correlation Level Contours on the Scales in the Inertial Range of Solar Wind Turbulence
Honghong Wu, Chuanyi Tu, Xin Wang +2
The self-correlation level contours at the 1010 cm scale reveal a 3D isotropic feature in the slow solar wind and a quasi-anisotropic feature in the fast solar wind. However, the 1…
3-D feature of self-correlation level contours at scale in solar wind turbulence
Honghong Wu, Chuanyi Tu, Xin Wang +2
The self-correlation level contours at scale reveal a 2-D isotropic feature in both the slow solar wind fluctuations and the fast solar wind fluctuations. Ho…
The Fluid-like Behavior of Kinetic Alfvén Turbulence in Space Plasma
Honghong Wu, Daniel Verscharen, Robert T. Wicks +3
Kinetic Alfvén waves (KAWs) are the short-wavelength extension of the MHD Alfvén-wave branch in the case of highly-oblique propagation with respect to the background magnetic field…