17 citations · 31 across the 4 of their papers we have counts for
7 papers
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…
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…
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…
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…
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…
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…