SH
Member Since 2012
Shiyong Huang
Researcher, Wuhan University
Professional Experience
Laboratoire de Physique des Plasmas
Post-doc
Wuhan University
Researcher
Education
Doctorate
2013
Honors & Awards
Sunanda and Santimay Basu (International) Early Career Award in Sun-Earth Systems Science
Received 2020
See Details
Publications
Impact of Mass‐Loading Effect on the Competition in the Energy Conversion Rate During Magnetic Recon...
Heavy particles are extensively detected in the space environment, especially in the solar wind and interplanetary magnetosphere. Various physical ...
April 01, 2024
Crater Structure Behind Reconnection Front
February 28, 2024
Effects of Electron Vortices on the Magnetic Structures in t...
February 28, 2024
Statistical Characteristics of Chorus Second Harmonic Waves ...
December 20, 2023
AGU Abstracts
Compressible turbulence in the planetary magnetosheaths and the solar wind: turbulent energy cascade rate.
ENERGY TRANSFER AND DISSIPATION IN SPACE PLASMAS: KINETIC TO GLOBAL SCALES II ORAL
spa-solar and heliospheric physics | 13 december 2023
Lina HADID, Nahuel Andrés, Fouad Sahraoui, Sébasti...
Over the past three decades, compressible turbulence has been a subject of active research in space physics, particularly in relation to the solar win...
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Multiscale analysis of a current sheet crossing associated with a fast earthward flow during a substorm event detected by MMS
THE IMPORTANCE OF MESOSCALE MAGNETOTAIL PROCESSES IN GLOBAL AND KINETIC-SCALE MAGNETOSPHERIC DYNAMICS III POSTER
spa-magnetospheric physics | 16 december 2021
Olivier Le Contel, Alessandro Retino, Alexandra Al...
In July 2017, the MMS constellation was evolving in the magnetotail with an apogee of 25 Earth radii and an average inter-satellite distance of 10 km ...
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Taylor hypothesis at electron scales and its effects on measured energy spectra onboard spacecraft
TURBULENCE, WAVES, AND MAGNETIC RECONNECTION FROM MAGNETOHYDRODYNAMIC TO KINETIC SCALES II POSTERS
spa-solar and heliospheric physics | 11 december 2019
Shiyong Huang, Fouad Sahraoui
The solar wind is a natural laboratory for the study of turbulent plasma. In-situobservations from different spacecraft such as STEREO, Wind, ACE or C...
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Check out all of Shiyong Huang’s AGU Research!
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