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浏览/检索结果: 共41条，第1-10条 帮助

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Reconstructing forest and grassland cover changes in China over the past millennium 期刊论文  OAI收割
SCIENCE CHINA-EARTH SCIENCES, 2024, 卷号: N/A
作者:  He, Fanneng;  Yang, Fan;  Wang, Yafei
  |  收藏  |  浏览/下载：5/0  |  提交时间：2025/01/17
Will the 2022 compound heatwave-drought extreme over the Yangtze River Basin become Grey Rhino in the future? 期刊论文  OAI收割
ADVANCES IN CLIMATE CHANGE RESEARCH, 2024, 卷号: 15, 期号: 3, 页码: 547-556
作者:  Feng, Ai-Qing;  Chao, Qing-Chen;  Liu, Lu-Lu;  Gao, Ge;  Wang, Guo-Fu
  |  收藏  |  浏览/下载：5/0  |  提交时间：2024/08/22
Desertification and Related Climate Change in the Alashan Plateau since the Last 40 ka of the Last Glacial Period 期刊论文  OAI收割
ATMOSPHERE, 2023, 卷号: 14, 期号: 2
作者:  Zhu, Bingqi;  Yang, Limin
  |  收藏  |  浏览/下载：29/0  |  提交时间：2023/04/06
Integrated study of the Doushantuo Formation in northwestern Hunan Province: Implications for Ediacaran chemostratigraphy and biostratigraphy in South China 期刊论文  OAI收割
PRECAMBRIAN RESEARCH, 2022, 卷号: 377, 页码: 22
作者:  Shi, Hongyi;  Ouyang, Qing;  Zhou, Chuanming;  Xiao, Shuhai;  Chen, Zhe
  |  收藏  |  浏览/下载：45/0  |  提交时间：2022/09/02
Climate Change along the Silk Road and Its Influence on Scythian Cultural Expansion and Rise of the Mongol Empire 期刊论文  OAI收割
SUSTAINABILITY, 2021, 卷号: 13, 期号: 5, 页码: 17
作者:  Che, Ping;  Lan, Jianghu
  |  收藏  |  浏览/下载：37/0  |  提交时间：2021/05/21
Nonuniform variations of precipitation and temperature across China over the period 1960-2015 期刊论文  OAI收割
INTERNATIONAL JOURNAL OF CLIMATOLOGY, 2020, 页码: 12
作者:  Zhao, Dongsheng;  Gao, Xuan;  Wu, Shaohong
  |  收藏  |  浏览/下载：18/0  |  提交时间：2021/03/23
Nonuniform variations of precipitation and temperature across China over the period 1960-2015 期刊论文  OAI收割
INTERNATIONAL JOURNAL OF CLIMATOLOGY, 2020, 页码: 12
作者:  Zhao, Dongsheng;  Gao, Xuan;  Wu, Shaohong
  |  收藏  |  浏览/下载：19/0  |  提交时间：2021/03/23
末次间冰期以来古火对千年及轨道尺度气候和植被变化的响应 期刊论文  OAI收割
第四纪研究, 2020, 卷号: 40, 期号: 6, 页码: 1513
作者:  崔巧玉
  |  收藏  |  浏览/下载：26/0  |  提交时间：2021/03/15
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.  
末次间冰期以来古火对千年及轨道尺度气候和植被变化的响应 期刊论文  OAI收割
第四纪研究, 2020, 卷号: 40, 期号: 6, 页码: 1513
作者:  崔巧玉
  |  收藏  |  浏览/下载：23/0  |  提交时间：2021/03/15