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20112023
most citedWhat can we learn about solar coronal mass ejections, coronal dimmings, and Extreme-Ultraviolet jets through spectroscopic observations?

128 citations · 543 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2022★ 5 cited

On the scaling and anisotropy of two subranges in the inertial range of solar wind turbulence

Honghong Wu, Jiansen He, Liping Yang +3

Intermittency and anisotropy are two important aspects of plasma turbulence, which the solar wind provides a natural laboratory to investigate. However, their forms and nature are…

astro-ph.SR2021★ 15 cited

Large Amplitude Switchback Turbulence: Possible Magnetic Velocity Alignment Structures

Honghong Wu, Chuanyi Tu, Xin Wang +1

Switchbacks are widely acknowledged phenomena observed by the Parker Solar Probe and appear to occur in patches. Previous studies focused on the fluctuations at the magnetic revers…

astro-ph.SR2016★ 18 cited

Spectral Anisotropy of Elsässer Variables in Two Dimensional Wave-vector Space as Observed in the Fast Solar Wind Turbulence

Limei Yan, Jiansen He, Lei Zhang +6

Intensive studies have been conducted to understand the anisotropy of solar wind turbulence. However, the anisotropy of Elsässer variables () in 2D wave-vector spac…

astro-ph.SR2015★ 24 cited

Formation of Rotational Discontinuities in Compressive three-dimensional MHD Turbulence

Liping Yang, Lei Zhang, Jiansen He +6

Measurements of solar wind turbulence reveal the ubiquity of discontinuities. In this study, we investigate how the discontinuities, especially rotational discontinuities (RDs), ar…

astro-ph.SR2015★ 25 cited

Occurrence Rates and Heating Effects of Tangential and Rotational Discontinuities as Obtained from Three-dimensional Simulation of Magnetohydrodynamic Turbulence

Lei Zhang, Jiansen He, Chuanyi Tu +4

In solar wind, magnetohydrodynamic (MHD) discontinuities are ubiquitous and often found to be at the origin of turbulence intermittency. They may also play a key role in the turbul…

astro-ph.SR2014★ 103 cited

Deciphering Solar Magnetic Activity I: On The Relationship Between The Sunspot Cycle And The Evolution Of Small Magnetic Features

Scott W. McIntosh, Xin Wang, Robert J. Leamon +6

Sunspots are a canonical marker of the Sun's internal magnetic field which flips polarity every ~22-years. The principal variation of sunspots, an ~11-year variation in number, mod…