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researcher

J. Zhang

3 papers hereh-index 15538 citations52 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • physics.space-ph2
  • astro-ph.SR1
same name
  • J. Zhang — 183 papers
  • J. Zhang — 167 papers, h 57
  • J. Zhang — 159 papers, h 58
  • J. Zhang — 159 papers, h 48
  • J. Zhang — 157 papers, h 48
  • J. Zhang — 54 papers, h 46

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20202022
most citedKinetic Scale Slow Solar Wind Turbulence in the Inner Heliosphere: Co-existence of Kinetic Alfvén Waves and Alfvén Ion Cyclotron Waves

52 citations · 113 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2022★ 22 cited

Anisotropy of Magnetic Field Spectra at Kinetic Scales of Solar Wind Turbulence as Revealed by Parker Solar Probe in the Inner Heliosphere

S. Y. Huang, S. B. Xu, J. Zhang +11

Using the Parker Solar Probe data taken in the inner heliosphere, we investigate the power and spatial anisotropy of magnetic-field spectra at kinetic scales (i.e., around sub-ion…

physics.space-ph2021★ 39 cited

The Ion Transition Range of Solar Wind Turbulence in the Inner Heliosphere: Parker Solar Probe Observations

S. Y. Huang, F. Sahraoui, N. Andrés +15

The scaling of the turbulent spectra provides a key measurement that allows to discriminate between different theoretical predictions of turbulence. In the solar wind, this has dri…

physics.space-ph2020★ 52 cited

Kinetic Scale Slow Solar Wind Turbulence in the Inner Heliosphere: Co-existence of Kinetic Alfvén Waves and Alfvén Ion Cyclotron Waves

S. Y. Huang, J. Zhang, F. Sahraoui +12

The nature of the plasma wave modes around the ion kinetic scales in highly Alfvénic slow solar wind turbulence is investigated using data from the NASA's Parker Solar Probe taken…

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