Zobrazeno 1 - 10
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pro vyhledávání: '"HUANG, S. Y."'
Autor:
Wu, Y. Y., Mu, L., Zhang, X., Dai, D. Z., Xin, L., Kong, X. M., Huang, S. Y., Meng, K., Yang, X. F., Tu, C. P., Ni, J. M., Yan, H. G., Li, S. Y.
The van der Waals (vdW) semiconductor black phosphorus has been widely studied, especially after the discovery of phosphorene. On the contrary, its sister compound violet phosphorus, also a vdW semiconductor, has been rarely studied. Here we report t
Externí odkaz:
http://arxiv.org/abs/2307.02989
Autor:
Huang, S. Y., Xu, S. B., Zhang, J., Sahraoui, F., Andres, N., He, J. S., Yuan, Z. G., Deng, X. H., Jiang, K., Wei, Y. Y., Xiong, Q. Y., Wang, Z., Yu, L., Lin, R. T.
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 scales) in solar wind turbulence in the inner heliosphere. We find tha
Externí odkaz:
http://arxiv.org/abs/2203.10475
Autor:
Huang, S. Y., Xiong, Q. Y., Song, L. F., Nan, J., Yuan, Z. G., Jiang, K., Deng, X. H., Yu, L.
In the standard model of magnetic reconnection, both ions and electrons couple to the newly reconnected magnetic field lines and are ejected away from the reconnection diffusion region in the form of bidirectional burst ion and electron jets. Recent
Externí odkaz:
http://arxiv.org/abs/2109.13051
Autor:
Huang, S. Y., Lin, R. T., Yuan, Z. G., Jiang, K., Wei, Y. Y., Xu, S. B., Zhang, J., Zhang, Z. H., Xiong, Q. Y., Yu, L.
Depression in magnetic field strength with a scale below one proton gyroradius is referred to as kinetic-size magnetic hole (KSMH). KSMHs are frequently observed near terrestrial space environments and are thought to play an important role in electro
Externí odkaz:
http://arxiv.org/abs/2109.11697
Autor:
Jiang, K., Huang, S. Y., Fu, H. S., Yuan, Z. G., Deng, X. H., Wang, Z., Guo, Z. Z., Xu, S. B., Wei, Y. Y., Zhang, J., Zhang, Z. H., Xiong, Q. Y., Yu, L.
Electron heating/acceleration in the foreshock, by which electrons may be energized beyond thermal energies prior to encountering the bow shock, is very important for the bow shock dynamics. And then these electrons would be more easily injected into
Externí odkaz:
http://arxiv.org/abs/2109.11696
Autor:
Andrés, N., Sahraoui, F., Hadid, L. Z., Huang, S. Y., Romanelli, N., Galtier, S., DiBraccio, G., Halekas, J.
The first computation of the compressible energy transfer rate from $\sim$ 0.2 AU up to $\sim$ 1.7 AU is obtained using PSP, THEMIS and MAVEN observations. The compressible energy cascade rate $\varepsilon_C$ is computed for hundred of events at diff
Externí odkaz:
http://arxiv.org/abs/2102.11781
Autor:
Huang, S. Y., Sahraoui, F., Andrés, N., Hadid, L. Z., Yuan, Z. G., He, J. S., Zhao, J. S., Galtier, S., Zhang, J., Deng, X. H., Jiang, K., Yu, L., Xu, S. B., Xiong, Q. Y., Wei, Y. Y., de Wit, T. Dudok, Bale, S. D., Kasper, J. C.
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 driven a large number of studies dedicated to this issue using in-situ da
Externí odkaz:
http://arxiv.org/abs/2101.09851
Autor:
Yu, L., Huang, S. Y., Yuan, Z. G., Jiang, K., Xiong, Q. Y., Xu, S. B., Wei, Y. Y., Zhang, J., Zhang, Z. H.
We present a statistical analysis for the characteristics and radial evolution of linear magnetic holes (LMHs) in the solar wind from 0.166 to 0.82 AU using Parker Solar Probe observations of the first two orbits. It is found that the LMHs mainly hav
Externí odkaz:
http://arxiv.org/abs/2010.14008
Autor:
Huang, S. Y., Zhang, J., Sahraoui, F., He, J. S., Yuan, Z. G., Andrés, N., Hadid, L. Z., Deng, X. H., Jiang, K., Yu, L., Xiong, Q. Y., Wei, Y. Y., Xu, S. B., Bale, S. D., Kasper, J. C.
The nature of the plasma wave modes around the ion kinetic scales in highly Alfv\'enic slow solar wind turbulence is investigated using data from the NASA's Parker Solar Probe taken in the inner heliosphere, at 0.18 Astronomical Unit (AU) from the su
Externí odkaz:
http://arxiv.org/abs/2006.04665
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