activity
20152025
most citedNumerical Study of the Longitudinally Asymmetric Distribution of Solar Energetic Particles in the Heliosphere

17 citations · 61 across the 7 of their papers we have counts for

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physics.space-ph2025

Solar-cycle Variability of Composite Geometry in the Solar Wind Turbulence

Zhan Fa, H. -Q. He

The composite geometry and spectral anisotropy of the solar wind turbulence are very important topics in the investigations of solar wind. In this work, we use the magnetic field a…

physics.space-ph20214 cited

New Insight into the Formation Mechanism of the Energetic Particle Reservoirs in the Heliosphere

H. -Q. He

The concept of energetic particle reservoirs, essentially based on the assumption of the presence of outer reflecting boundaries/magnetic mirrors or diffusion barriers (determinist…

physics.space-ph20217 cited

The Solar Cycle Variations of the Anisotropy of Taylor Scale and Correlation Scale in the Solar Wind Turbulence

G. Zhou, H. -Q. He

The field-aligned anisotropy of the solar wind turbulence, which is quantified by the ratio of the parallel to the perpendicular correlation (and Taylor) length scales, is determin…

physics.space-ph20195 cited

Propagation of Solar Energetic Particles in the Outer Heliosphere: Interplay between Scattering and Adiabatic Focusing

H. -Q. He, W. Wan

The turbulence and spatial nonuniformity of the guide magnetic field cause two competitive effects, namely, the scattering effect and the adiabatic focusing effect, respectively. I…

physics.space-ph201711 cited

Propagation of Solar Energetic Particles in Three-dimensional Interplanetary Magnetic Fields: Radial Dependence of Peak Intensities

H. -Q. He, G. Zhou, W. Wan

A functional form I_{max}(R)=kR^{-α}, where R is the radial distance of spacecraft, was usually used to model the radial dependence of peak intensities I_{max}(R) of solar energeti…