X. T. He

ORCID: 0000-0002-0356-9230
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About
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Research Areas
  • Ionosphere and magnetosphere dynamics
  • Solar and Space Plasma Dynamics
  • Spectroscopy and Laser Applications
  • Astrophysics and Star Formation Studies
  • Terahertz technology and applications
  • Acoustic Wave Resonator Technologies
  • Laser-Plasma Interactions and Diagnostics
  • Astro and Planetary Science
  • Atomic and Molecular Physics

Terahertz communication technology holds promise for solving the challenging “blackout” problem. Research has revealed that spectrum exhibits new peaks when terahertz waves propagate through plasma. In realm of communications, elucidating underlying physical mechanisms responsible these novel is paramount importance. this paper, a combination theoretical analysis and simulation utilized to investigate causes spectral changes. Theoretically, expression relative dielectric constant plasma been...

10.1063/5.0219947 article EN Physics of Plasmas 2024-09-01

The interaction between the supersonic jet and background can influence process of star formation, this also results in a change jet's velocity, direction density through shock waves. However, due to limitations current astronomical facilities, fine structure detailed still remain unclear. Here we investigate plasma dynamics under different collision states laser-driven experiments. A double-shock is shown optical diagnosis for case, but integrated self-emitting X-ray characteristic...

10.48550/arxiv.2203.06326 preprint EN other-oa arXiv (Cornell University) 2022-01-01

Magnetic reconnection, breaking and reorganization of magnetic field topology, is a fundamental process for rapid release energy into plasma particles that occurs pervasively throughout the universe. In most natural circumstances, properties on either side reconnection layer are asymmetric, in particular collision rates associated with combination density temperature critically determine mechanism. To date, all laboratory experiments reconnections have been limited to purely collisional or...

10.48550/arxiv.2202.12471 preprint EN cc-by arXiv (Cornell University) 2022-01-01
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