activity
20192025
most citedMagnetic helicity signature and its role in regulating magnetic energy spectra and proton temperatures in the solar wind

17 citations · 76 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

Solar magnetic flux rope eruptions caused by inverse flux feeding processes

Quanhao Zhang, Shangbin Yang, Rui Liu +6

Large-scale solar eruptions are generally accepted to have coronal magnetic flux ropes as their core structures. Recent studies found that the solar eruptions could be initiated by…

astro-ph.SR2021★ 1 cited

The Inhomogeneity of Composition along the Magnetic Cloud Axis

Hongqiang Song, Qiang Hu, Xin Cheng +6

It is generally accepted that CMEs result from eruptions of magnetic flux ropes, which are dubbed as magnetic clouds in interplanetary space. The composition (including the ionic c…

physics.space-ph2020★ 17 cited

Magnetic helicity signature and its role in regulating magnetic energy spectra and proton temperatures in the solar wind

G. Q. Zhao, Y. Lin, X. Y. Wang +5

In a previous paper, we found that proton temperatures are clearly associated with the proton-scale turbulence in the solar wind, and magnetic helicity signature appears to be an i…

physics.space-ph2020★ 17 cited

Observational evidence for solar wind proton heating by ion-scale turbulence

G. Q. Zhao, Y. Lin, X. Y. Wang +5

Based on in-situ measurements by Wind spacecraft from 2005 to 2015, this letter reports for the first time a clearly scale-dependent connection between proton temperatures and the…

astro-ph.SR2020★ 12 cited

A statistical study of the plasma and composition distribution inside magnetic clouds: 1998-2011

Jin Huang, Yu Liu, Hengqiang Feng +4

A comprehensive analysis of plasma and composition characteristics inside magnetic clouds (MCs) observed by the Advanced Composition Explorer (ACE) spacecraft from 1998 February to…

physics.space-ph2019★ 8 cited

Comparison of counterstreaming suprathermal electron signatures of ICMEs with and without magnetic cloud: are all ICMEs flux ropes?

Jiemin Wang, Yan Zhao, Hengqiang Feng +5

Magnetic clouds (MCs), as large-scale interplanetary magnetic flux ropes, are usually still connected to the sun at both ends near 1 AU. Many researchers believe that all non-MC in…

physics.space-ph2019★ 16 cited

Effects of alpha-proton differential flow on proton temperature anisotropy instabilities in the solar wind: Wind observations

G. Q. Zhao, H. Li, H. Q. Feng +3

Plasma kinetic waves and alpha-proton differential flow are two important subjects on the topic of evolution of the solar wind. Based on the Wind data during 2005-2015, this paper…

physics.space-ph2019★ 5 cited

Possible cool prominence materials detected within interplanetary small magnetic flux ropes

J. M. Wang, H. Q. Feng, H. B. Li +5

Previous studies indicate that interplanetary small magnetic flux ropes (SMFRs) are manifestations of microflare-associated small coronal mass ejections (CMEs), and the hot materia…