Zobrazeno 1 - 10
of 251
pro vyhledávání: '"F.-J. Kong"'
Publikováno v:
The Astrophysical Journal, Vol 942, Iss 2, p 63 (2023)
We present a study of the efficiency of the acceleration of suprathermal electrons at collisionless shock waves driven by interplanetary coronal mass ejections (ICMEs), with the data analysis from both the spacecraft observations and test-particle si
Externí odkaz:
https://doaj.org/article/0c1a571238da4f1bad39ecc7702e0b79
Publikováno v:
Zhonghua gan zang bing za zhi = Zhonghua ganzangbing zazhi = Chinese journal of hepatology. 29(11)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::48dd1ae5cb2ee27764a368dd3474e7bb
https://pubmed.ncbi.nlm.nih.gov/34933422
https://pubmed.ncbi.nlm.nih.gov/34933422
Autor:
B, Qian, J Y, Liu, F M, Zhang, F J, Kong, W, Zhou, Q C, Gu, Y, Fang, Z D, Han, X F, Jiang, Y L, Zhu, Y, Wang, J, Hu, Z Q, Mao
Publikováno v:
Journal of physics. Condensed matter : an Institute of Physics journal. 34(2)
Iron chalcogenides are of particular interests among iron-based superconductors due to their distinct properties such as high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::b8e37fe188909630c8c7333c0f10164b
https://pubmed.ncbi.nlm.nih.gov/34619673
https://pubmed.ncbi.nlm.nih.gov/34619673
Autor:
Yong Fang, Xuefan Jiang, Zhiqiang Mao, F M Zhang, F J Kong, Z. D. Han, Q C Gu, Y Wang, Jinyu Liu, Wei Zhou, Bin Qian, Jin Hu, Y L Zhu
Publikováno v:
Journal of Physics: Condensed Matter. 34:025601
Iron chalcogenides are of particular interests among iron-based superconductors due to their distinct properties such as high-T c on FeSe monolayer and competing magnetic correlations in Fe1+y Te. Here we report unusual transport properties observed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2c126fba04c62460887bed9b75dfa5e0
https://doi.org/10.1088/1361-648x/ac2db9
https://doi.org/10.1088/1361-648x/ac2db9
Autor:
Gang Qin, F. J. Kong
The acceleration of suprathermal electrons in the solar wind is mainly associated with shocks driven by interplanetary coronal mass ejections (ICMEs). It is well known that the acceleration of electrons is much more efficient at quasi-perpendicular s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5bb43012992d7828ef8954d8c1e81d8a
Publikováno v:
Zhonghua kou qiang yi xue za zhi = Zhonghua kouqiang yixue zazhi = Chinese journal of stomatology. 52(9)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::c979cded4e40fc761d7dc7eb24e16a56
https://pubmed.ncbi.nlm.nih.gov/29972927
https://pubmed.ncbi.nlm.nih.gov/29972927
Publikováno v:
Zhonghua kou qiang yi xue za zhi = Zhonghua kouqiang yixue zazhi = Chinese journal of stomatology. 52(7)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::299ac79e6d961bd5c8657bfa1aedc5da
https://pubmed.ncbi.nlm.nih.gov/29972910
https://pubmed.ncbi.nlm.nih.gov/29972910
Publikováno v:
The Astrophysical Journal. 877:97
Strategic Priority Research Program of Chinese Academy of Sciences [XDA17010301]; [NNSFC 41874206]; [NNSFC 41574172]
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba02266778d0c2d79378b637db6cc10f
https://doi.org/10.3847/1538-4357/ab1b33
https://doi.org/10.3847/1538-4357/ab1b33
Publikováno v:
The Astrophysical Journal. 860:3
Using test particle simulations we study electron acceleration at collisionless shocks with a two-component model turbulent magnetic field with slab component including dissipation range. We investigate the importance of shock normal angle $\theta_{B
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c39e8f0435e2e8d906261486b7570552
https://doi.org/10.3847/1538-4357/aac26f
https://doi.org/10.3847/1538-4357/aac26f
Publikováno v:
The Astrophysical Journal. 845:43
Using test particle simulations we study particle acceleration at highly perpendicular ($\theta_{Bn}\geq 75^\circ$) shocks under conditions of modeling magnetic turbulence. We adopt a backward-in-time method to solve the Newton-Lorentz equation using
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1021ba200c35b9a35a90f32debfdf4ed
https://doi.org/10.3847/1538-4357/aa7745
https://doi.org/10.3847/1538-4357/aa7745