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20192025
most citedObservational evidence for solar wind proton heating by ion-scale turbulence

17 citations · 31 across the 5 of their papers we have counts for

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physics.space-ph2020

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-ph202017 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…

physics.space-ph20198 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

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-ph20195 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…