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浏览/检索结果: 共18条,第1-10条 帮助

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Phase-lag effect on the instantaneously-liquefied seabed depth under progressive waves: Explicit approximations 期刊论文  OAI收割
APPLIED OCEAN RESEARCH, 2024, 卷号: 147, 页码: 12
作者:  
Li CF(李畅飞);  Yu JH(于嘉豪);  Gao FP(高福平)
  |  收藏  |  浏览/下载:39/0  |  提交时间:2024/06/11
Electroencephalography characteristics of patients with supratentorial glioma in different consciousness states induced by propofol 期刊论文  OAI收割
NEUROSCIENCE LETTERS, 2023, 卷号: 808, 页码: 6
作者:  
Yang, Wanning;  Wang, Xinxin;  Liu, Haiyang;  Li, Muhan;  Liu, Xiaoyuan
  |  收藏  |  浏览/下载:26/0  |  提交时间:2023/10/09
Combined nonlinear wave and current induced instantaneously-liquefied soil depth in a non-cohesive seabed 期刊论文  OAI收割
COASTAL ENGINEERING, 2023, 卷号: 179, 页码: 12
作者:  
Yang LJ(杨鲤境);  Gao FP(高福平);  Li CF(李畅飞)
  |  收藏  |  浏览/下载:46/0  |  提交时间:2022/12/20
Characterization of spatio-temporal distributions of wave-induced pore pressure in a non-cohesive seabed: Amplitude-attenuation and phase-lag 期刊论文  OAI收割
OCEAN ENGINEERING, 2022, 卷号: 253, 页码: 14
作者:  
Li, Chang-Fei;  Gao, Fu-Ping;  Gao FP(高福平)
  |  收藏  |  浏览/下载:43/0  |  提交时间:2022/07/18
Synchronous X-ray/Optical QPOs from the Black Hole LMXB MAXI J1820+070 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2021
作者:  
HXMT
  |  收藏  |  浏览/下载:53/0  |  提交时间:2022/02/08
black hole physics  Low Mass X-ray Binaries  accretion  accretion  discs  stars: individual (MAXI J1820+070)  Astrophysics - High Energy  Astrophysical Phenomena  Abstract: We present high-speed optical photometry from SAAO and SALT on the black hole LMXB MAXI J1820+070 (ASSASN-18ey), some of it simultaneous with NICER, Swift and Insight-HXMT X-ray coverage. We detect optical Quasi-Periodic Oscillations (QPOs) that move to higher frequencies as the outburst progresses, tracking both the frequency and evolution of similar X-ray QPOs previously reported. Correlated X-ray/optical data reveal a complex pattern of lags, including an anti-correlation and a sub-second lag that evolve over the first few weeks of outburst. They also show correlated components separated by a lag equal to the QPO period roughly centered on zero lag, implying that the inter-band variability is strongly and consistently affected by these QPOs at a constant phase lag of roughly ±Ю The synchronisation of X-ray and optical QPOs indicates that they must be produced in regions physically very close to each other  we thus propose that they can be explained by a precessing jet model, based on analogies with V404 Cyg and MAXI J1348-630.  
Ammonia stress decreased biomarker genes of acetoclastic methanogenesis and second peak of production rates during anaerobic digestion of swine manure 期刊论文  OAI收割
BIORESOURCE TECHNOLOGY, 2020, 卷号: 317, 页码: 1-10
作者:  
Yu, Dawei;  Zhang, Junya;  Chulu, Buhe;  Yang, Min;  Nopens, Ingmar
  |  收藏  |  浏览/下载:23/0  |  提交时间:2021/09/15
Conservation of oxygen and hydrogen seasonal isotopic signals in meteoric precipitation in groundwater: An experimental tank study of the effects of land cover in a summer monsoon climate 期刊论文  OAI收割
GEOCHIMICA ET COSMOCHIMICA ACTA, 2020, 卷号: 284, 页码: 254-272
作者:  
Hu, Yundi;  Liu, Zaihua;  Ford, Derek;  Zhao, Min;  Bao, Qian
  |  收藏  |  浏览/下载:37/0  |  提交时间:2021/03/18
Responses of Multiday Oscillations in the Nighttime Thermospheric Temperature to Solar and Geomagnetic Activities Measured by Fabry-Perot Interferometer in China 期刊论文  OAI收割
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019
作者:  
Liu, Yangkun;  Xu, Jiyao;  Liu, Xiao;  Zhang, Shun-Rung;  Yuan, Wei
  |  收藏  |  浏览/下载:30/0  |  提交时间:2019/12/17
Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文  OAI收割
Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40
作者:  
HXMT
  |  收藏  |  浏览/下载:57/0  |  提交时间:2022/02/08
Accretion  accretion disks  Black hole physics  X-rays: binaries:  Swift J1658.2-4242  Astrophysics - High Energy Astrophysical Phenomena  Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.  
Composite Hierarchical Anti-Disturbance Control with Multisensor Fusion for Compact Optoelectronic Platforms 期刊论文  OAI收割
SENSORS, 2018, 卷号: 18, 期号: 10, 页码: 25
作者:  
Dai, Ming;  Tian, Dapeng;  Wang, Yutang
  |  收藏  |  浏览/下载:48/0  |  提交时间:2019/08/21