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浏览/检索结果: 共27条,第1-10条 帮助

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Modeling magnetic soft continuum robot in nonuniform magnetic fields via energy minimization 期刊论文  OAI收割
INTERNATIONAL JOURNAL OF MECHANICAL SCIENCES, 2024, 卷号: 282, 页码: 14
作者:  
Li, Jiyu;  Wang, Liu
  |  收藏  |  浏览/下载:11/0  |  提交时间:2024/10/08
Model-guided navigation of magnetic soft guidewire for safe endovascular surgery 期刊论文  OAI收割
JOURNAL OF THE MECHANICS AND PHYSICS OF SOLIDS, 2024, 卷号: 190, 页码: 20
作者:  
Li, Jiyu;  Chen, Han;  Wang, Liu
  |  收藏  |  浏览/下载:12/0  |  提交时间:2024/07/26
Hard-rock investigation using a non-invasive geophysical approach 期刊论文  OAI收割
JOURNAL OF APPLIED GEOPHYSICS, 2022, 卷号: 206, 页码: 12
作者:  
Hasan, Muhammad;  Shang, Yanjun
  |  收藏  |  浏览/下载:21/0  |  提交时间:2023/04/03
Detection of Flare Multiperiodic Pulsations in Mid-ultraviolet Balmer Continuum, Lyl Hard X-Ray, and Radio Emissions Simultaneously 期刊论文  OAI收割
The Astrophysical Journal, 2021, 卷号: 921, 页码: 179
作者:  
HXMT
  |  收藏  |  浏览/下载:27/0  |  提交时间:2022/02/08
Solar flares  Solar oscillations  Solar ultraviolet emission  Solar  x-ray emission  Solar radio emission  1496  1515  1533  1536  1522  Astrophysics - Solar and Stellar Astrophysics  Abstract: Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of the total flux, are frequently detected in the light curves of solar/stellar flares. In this study, we present the investigation of nonstationary QPPs with multiple periods during the impulsive phase of a powerful flare on 2017 September 6, which were simultaneously measured by the Hard X-ray Modulation Telescope (Insight-HXMT), as well as the ground-based BLENSW. The multiple periods, detected by applying a wavelet transform and Lomb-Scargle periodogram to the detrended light curves, are found to be ~20-55 s in the Ly`and mid-ultraviolet Balmer continuum emissions during the flare impulsive phase. Similar QPPs with multiple periods are also found in the hard X-ray emission and low-frequency radio emission. Our observations suggest that the flare QPPs could be related to nonthermal electrons accelerated by the repeated energy release process, i.e., triggering of repetitive magnetic reconnection, while the multiple periods might be modulated by the sausage oscillation of hot plasma loops. For the multiperiodic pulsations, other generation mechanisms could not be completely ruled out.  
Introducing a special collection of papers in the Journal of High Energy Astrophysics on the Early Results of China's 1st X-ray Astronomy Satellite: Insight-HXMT 期刊论文  OAI收割
Journal of High Energy Astrophysics, 2020, 卷号: 27, 页码: 51-52
作者:  
HXMT
  |  收藏  |  浏览/下载:51/0  |  提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Insight-HXMT is the first Chinese X-ray astronomical mission, launched successfully on June 15, 2017, from China's Jiuquan Satellite Launch Center. Insight-HXMT was designed to have a broad energy coverage in X-rays, from 1-250 keV, with excellent timing and adequate energy resolution at soft X-rays, and the largest effective area at hard X-rays. This allows, in particular, to observe bright sources like X-ray binaries (XRBs) in their bright/outburst states with high cadence and high statistics at hard and soft X-rays at once. It was then expected that the Insight-HXMT mission will bring us new insights regarding the characteristics of several source classes. Examples include characterizing High-Mass X-ray Binaries (HMXBs) and the outburst evolution of Low-Mass X-ray Binaries (LMXBs). For instance, in HMXB systems, the region around their Alfven radius that is responsible to determine whether accretion or propeller occurs, or the region around the NS magnetic pole where the intense X-rays are supposed to be produced are specially appealing targets of study. For the LMXBs, the evolution the outburst and the properties of the compact objects themselves are obvious priority targets for Insight-HXMT. Due to the broad coverage in energy, Insight-HXMT is specially well suited to study the influence of thermonuclear (type-I) X-ray bursts upon the surrounding environment.  
Assessment of Aquifer Vulnerability Using Integrated Geophysical Approach in Weathered Terrains of South China 期刊论文  OAI收割
OPEN GEOSCIENCES, 2019, 卷号: 11, 期号: 1, 页码: 1129-1150
作者:  
Hasan, Muhammad;  Shang, Yanjun;  Jin, Weijun;  Akhter, Gulraiz
  |  收藏  |  浏览/下载:31/0  |  提交时间:2020/05/19
Magnetic structure of solar flare regions producing hard X-ray pulsations 期刊论文  OAI收割
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2018, 卷号: 174, 页码: 17-27
作者:  
Zimovets, I., V;  Wang, R.;  Liu, Y. D.;  Wang, C.;  Kuznetsov, S. A.
  |  收藏  |  浏览/下载:43/0  |  提交时间:2018/08/13
The Microstructure and Water Distribution of Partially Saturated Hard Clay 期刊论文  OAI收割
GEOTECHNICAL TESTING JOURNAL, 2018, 卷号: 41, 期号: 4, 页码: 830-835
作者:  
Chen, Liufeng;  Peng, Hua;  Yang, Diansen
  |  收藏  |  浏览/下载:34/0  |  提交时间:2020/04/08
Recent developments of rare-earth-free hard-magnetic materials 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2016, 卷号: 59, 期号: 1, 页码: -
Li, Da; Pan, DeSheng; Li, ShaoJie; Zhang, ZhiDong
收藏  |  浏览/下载:30/0  |  提交时间:2016/04/21
Quasilogarithmic magnetic viscosity in perpendicularly anisotropic Nd-Fe-B films 期刊论文  OAI收割
Journal of Magnetism and Magnetic Materials, 2012, 卷号: 324, 期号: 18, 页码: 2854-2857
Q. Yao; R. Grossinger; W. Liu; W. B. Cui; F. Yang; X. G. Zhao; Z. D. Zhang
收藏  |  浏览/下载:27/0  |  提交时间:2013/02/05