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Chinese Academy of Sciences Institutional Repositories Grid
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浏览/检索结果: 共68条,第1-10条 帮助

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A Transformer-Based Deep Learning Model for Successful Predictions of the 2021 Second-Year La Nina Condition 期刊论文  OAI收割
GEOPHYSICAL RESEARCH LETTERS, 2023, 卷号: 50, 期号: 12, 页码: 10
作者:  
Gao, Chuan;  Zhou, Lu;  Zhang, Rong-Hua
  |  收藏  |  浏览/下载:22/0  |  提交时间:2023/11/30
Determining source-specific terrigenous organic carbon contributions in sediments from the Yellow River estuary, Northeast China: A test of source apportionment models 期刊论文  OAI收割
MARINE CHEMISTRY, 2023, 卷号: 253, 页码: 11
作者:  
Wu, Dinggui;  Sun, Dayang;  Tang, Jianhui;  Sun, Yongge
  |  收藏  |  浏览/下载:13/0  |  提交时间:2024/01/26
Determining source-specific terrigenous organic carbon contributions in sediments from the Yellow River estuary, Northeast China: A test of source apportionment models 期刊论文  OAI收割
MARINE CHEMISTRY, 2023, 卷号: 253, 页码: 11
作者:  
Wu, Dinggui;  Sun, Dayang;  Tang, Jianhui;  Sun, Yongge
  |  收藏  |  浏览/下载:7/0  |  提交时间:2024/11/08
Distributional responses to climate change of two maple species in southern China 期刊论文  OAI收割
ECOLOGY AND EVOLUTION, 2023, 卷号: 13, 期号: 9, 页码: e10490
作者:  
Liu,De Tuan;  Chen,Jian Ying;  Sun,Wei Bang
  |  收藏  |  浏览/下载:9/0  |  提交时间:2024/07/10
An Agent-Based Traffic Recommendation System: Revisiting and Revising Urban Traffic Management Strategies 期刊论文  OAI收割
IEEE TRANSACTIONS ON SYSTEMS MAN CYBERNETICS-SYSTEMS, 2022, 页码: 13
作者:  
Jin, Junchen;  Rong, Dingding;  Pang, Yuqi;  Ye, Peijun;  Ji, Qingyuan
  |  收藏  |  浏览/下载:36/0  |  提交时间:2022/07/25
Global positive gross primary productivity extremes and climate contributions during 1982-2016 期刊论文  OAI收割
SCIENCE OF THE TOTAL ENVIRONMENT, 2021, 卷号: 774, 页码: 10
作者:  
Wang, Miaomiao;  Wang, Shaoqiang;  Zhao, Jian;  Ju, Weimin;  Hao, Zhuo
  |  收藏  |  浏览/下载:37/0  |  提交时间:2021/06/10
Global positive gross primary productivity extremes and climate contributions during 1982-2016 期刊论文  OAI收割
SCIENCE OF THE TOTAL ENVIRONMENT, 2021, 卷号: 774, 页码: 10
作者:  
Wang, Miaomiao;  Wang, Shaoqiang;  Zhao, Jian;  Ju, Weimin;  Hao, Zhuo
  |  收藏  |  浏览/下载:17/0  |  提交时间:2021/06/10
Evaluating Traditional Empirical Models and BPNN Models in Monitoring the Concentrations of Chlorophyll-A and Total Suspended Particulate of Eutrophic and Turbid Waters 期刊论文  OAI收割
WATER, 2021, 卷号: 13, 期号: 5, 页码: 13
作者:  
Jiang, Bo;  Liu, Hailong;  Xing, Qianguo;  Cai, Jiannan;  Zheng, Xiangyang
  |  收藏  |  浏览/下载:37/0  |  提交时间:2021/06/07
An Assessment of Using Remote Sensing-Based Models to Estimate Ground Surface Soil Heat Flux on the Tibetan Plateau during the Freeze-Thaw Process 期刊论文  OAI收割
REMOTE SENSING, 2020, 卷号: 12, 期号: 3, 页码: 24
作者:  
Yang, Cheng;  Wu, Tonghua;  Yao, Jimin;  Li, Ren;  Xie, Changwei
  |  收藏  |  浏览/下载:67/0  |  提交时间:2020/05/19
The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition 期刊论文  OAI收割
Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870
作者:  
HXMT
  |  收藏  |  浏览/下载:57/0  |  提交时间:2022/02/08
stars: magnetic field  stars: neutron  pulsars: general  Astrophysics  - High Energy Astrophysical Phenomena  Abstract: In 2011 December, PSR B054-69 experienced a spin-down rate transition (SRT), after which the spin-down power of the pulsar increased by $\sim 36{{\ \rm per\ cent}}$. About 1000 d after the SRT, the X-ray luminosity of the associated pulsar wind nebula (PWN) was found to brighten by $32\pm 8{{\ \rm per\ cent}}$. After the SRT, the braking index n of PSR B0540-69 changes from n = 2.12 to 0.03 and then keeps this value for about five years before rising to n = 0.9 in the following years. We find that most of the current models have difficulties in explaining the measured braking index. One exceptive model of the braking index evolution is the increasing dipole magnetic field of PSR B0540-69. We suggest that the field increase may result from some instabilities within the pulsar core that enhance the poloidal component at the price of toroidal component of the magnetic field. The increasing dipole magnetic field will result in the X-ray brightening of the PWN. We fit the PWN X-ray light curve by two models: one assumes a constant magnetic field within the PWN during the brightening and the other assumes an enhanced magnetic field proportional to the energy density of the PWN. It appears that the two models fit the data well, though the later model seems to fit the data a bit better. This provides marginal observational evidence that magnetic field in the PWN is generated by the termination shock. Future high-quality and high-cadence data are required to draw a solid conclusion.