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The convolutional neural network for Pacific decadal oscillation forecast 期刊论文  OAI收割
ENVIRONMENTAL RESEARCH LETTERS, 2024, 卷号: 19, 期号: 12, 页码: 11
作者:  
Skanupong, Nutta;  Xu, Yongsheng;  Yu, Lejiang;  Wan, Zhang;  Wang, Shuo
  |  收藏  |  浏览/下载:8/0  |  提交时间:2024/12/20
Development and Experimental Study of Supercritical Flow Payload for Extravehicular Mounting on TZ-6 期刊论文  OAI收割
ENTROPY, 2024, 卷号: 26, 期号: 10, 页码: 20
作者:  
Guo, Liang;  Duan L(段俐);  Zou, Xuemei;  Gao, Yang;  Zhang, Xiang
  |  收藏  |  浏览/下载:9/0  |  提交时间:2024/11/22
Impacts of the Madden-Julian Oscillation on Marginal Sea Heatwaves of the Southeastern Tropical Indian Ocean 期刊论文  OAI收割
JOURNAL OF GEOPHYSICAL RESEARCH-OCEANS, 2024, 卷号: 129, 期号: 7, 页码: 19
作者:  
Cui, Zhanxian;  Li, Yuanlong;  Guo, Yaru;  Wang, Fan
  |  收藏  |  浏览/下载:8/0  |  提交时间:2024/09/02
Multi-species approach strengthens the reliability of dendroclimatic reconstructions in monsoonal Northeast China 期刊论文  OAI收割
CLIMATIC CHANGE, 2022, 卷号: 171, 期号: 1-2, 页码: 7
作者:  
Zhu, Liangjun;  Liu, Shuguang;  Zhu, Haifeng;  Cooper, David J.;  Yuan, Danyang
  |  收藏  |  浏览/下载:20/0  |  提交时间:2022/11/07
Coral perspective on temperature seasonality and interannual variability in the northern South China Sea during the Roman Warm Period 期刊论文  OAI收割
GLOBAL AND PLANETARY CHANGE, 2021, 卷号: 207, 页码: 13
作者:  
Jiang, Leilei;  Yu, Kefu;  Han, Tao;  Tao, Shichen;  Zhang, Huiling
  |  收藏  |  浏览/下载:29/0  |  提交时间:2021/12/07
Implication of the Hubble tension for the primordial Universe in light of recent cosmological data 期刊论文  OAI收割
PHYSICAL REVIEW D, 2021, 卷号: 104, 期号: 6, 页码: 63510
作者:  
Ye, Gen;  Hu, Bin;  Piao, Yun-Song
  |  收藏  |  浏览/下载:18/0  |  提交时间:2021/09/27
Transition to Chaos of Buoyant-Thermocapillary Convection in Large-Scale Liquid Bridges 期刊论文  OAI收割
MICROGRAVITY SCIENCE AND TECHNOLOGY, 2020, 卷号: 32, 期号: 2, 页码: 217-227
作者:  
Wang J(王佳);  Duan L(段俐);  Kang Q(康琦)
  |  收藏  |  浏览/下载:30/0  |  提交时间:2020/08/26
An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242 期刊论文  OAI收割
Astronomy and Astrophysics, 2020, 卷号: 641, 页码: A101
作者:  
HXMT
  |  收藏  |  浏览/下载:58/0  |  提交时间:2022/02/08
accretion  accretion disks  black hole physics  X-rays: binaries  time  Astrophysics - High Energy Astrophysical Phenomena  Abstract:
Aims: Flip-flops are top-hat-like X-ray flux variations, which have been observed in some transient accreting black hole binary systems, and feature simultaneous changes in the spectral hardness and the power density spectrum (PDS). They occur at a crucial time in the evolution of these systems, when the accretion disc emission starts to dominate over coronal emission. Flip-flops remain a poorly understood phenomenon, so we aim to thoroughly investigate them in a system featuring several such transitions.
Methods: Within the multitude of observations of Swift J1658.2-4242 during its outburst in early 2018, we detected 15 flip-flops, enabling a detailed analysis of their individual properties and the differences between them. We present observations by XMM-Newton, NuSTAR, Astrosat, Swift, Insight-HXMT, INTEGRAL, and ATCA. We analysed their light curves, searched for periodicities, computed their PDSs, and fitted their X-ray spectra, to investigate the source behaviour during flip-flop transitions and how the interval featuring flip-flops differs from the rest of the outburst.
Results: The flip-flops of Swift J1658.2-4242 are of an extreme variety, exhibiting flux differences of up to 77% within 100 s, which is much larger than what has been seen previously. We observed radical changes in the PDS simultaneous with the sharp flux variations, featuring transitions between the quasi-periodic oscillation types C and A, which have never been observed before. Changes in the PDS are delayed, but more rapid than changes in the light curve. Flip-flops occur in two intervals within the outburst, separated by about two weeks in which these phenomena were not seen. Transitions between the two flip-flop states occurred at random integer multiples of a fundamental period of 2.761 ks in the first interval and 2.61 ks in the second. Spectral analysis reveals the high and low flux flip-flop states to be very similar, but distinct from intervals lacking flip-flops. A change of the inner temperature of the accretion disc is responsible for most of the flux difference in the flip-flops. We also highlight the importance of correcting for the influence of the dust scattering halo on the X-ray spectra.
  
Interdecadal modulation of the Atlantic Multi-decadal Oscillation (AMO) on southwest China's temperature over the past 250years 期刊论文  OAI收割
CLIMATE DYNAMICS, 2019, 卷号: 52, 期号: 3-4, 页码: 2055-2065
作者:  
Fang, Keyan;  Guo, Zhengtang;  Chen, Deliang;  Wang, Lei;  Dong, Zhipeng
  |  收藏  |  浏览/下载:75/0  |  提交时间:2019/05/22
Interdecadal modulation of the Atlantic Multi-decadal Oscillation (AMO) on southwest China's temperature over the past 250years 期刊论文  OAI收割
CLIMATE DYNAMICS, 2019, 卷号: 52, 期号: 3-4, 页码: 2055-2065
作者:  
Fang, Keyan;  Guo, Zhengtang;  Chen, Deliang;  Wang, Lei;  Dong, Zhipeng
  |  收藏  |  浏览/下载:78/0  |  提交时间:2019/04/18