中国科学院机构知识库网格系统: 检索

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	A possibly solar metallicity atmosphere escaping from HAT-P-32b revealed by Hα and He absorption 期刊论文 OAI收割 ASTRONOMY & ASTROPHYSICS, 2024, 卷号: 686 作者: Yan DD(闫冬冬); Guo JH(郭建恒); Seon, Kwang-il; López, Manuel; Czesla, Stefan \| 收藏 \| 浏览/下载：37/0 \| 提交时间：2024/07/01 hydrodynamics radiative transfer methods: numerical planets and satellites: atmospheres planets and satellites: composition planets and satellites: individual: HAT-P-32b
	Adiabatic shearing in railway wheel steel of high-speed train 期刊论文 OAI收割 MATERIALS LETTERS, 2023, 卷号: 341, 页码: 134168 作者: Lei Y(雷勇); Li T(李统); Su MY(苏明耀); Li C(李琛); Wang HY(汪海英) \| 收藏 \| 浏览/下载：81/0 \| 提交时间：2023/06/15 Metals and alloys Railway wheel steel Hat-shaped specimen Microstructure Shear localization
	Uncertainties of three high-resolution actual evapotranspiration products across China: Comparisons and applications 期刊论文 OAI收割 ATMOSPHERIC RESEARCH, 2023, 卷号: 286, 页码: 106682 作者: Yao, Tianci; Lu, Hongwei; Yu, Qing; Feng, Sansan; Xue, Yuxuan \| 收藏 \| 浏览/下载：38/0 \| 提交时间：2023/05/06 Actual evapotranspiration Uncertainty Attribution analysis Three-cornered hat method China
	The study on transiting systems HAT-P-13, HAT-P-16, and WASP-32 through combining ground-based and TESS photometry 期刊论文 OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 卷号: 520, 期号: 2, 页码: 1642-1658 作者: Sun LL(孙磊磊); Gu SH(顾盛宏); Wang XB(王晓彬); Bai L(白璐); Schmitt, J H M M \| 收藏 \| 浏览/下载：27/0 \| 提交时间：2023/03/27 techniques: photometric planets and satellites: fundamental parameters planets and satellites: individual: HAT- P-13, HAT-P-16, WASP-32
	Latin Matchings and Ordered Designs OD(n-1, n, 2n-1) 期刊论文 OAI收割 MATHEMATICS, 2022, 卷号: 10, 期号: 24, 页码: 18 作者: Jin, Kai; Zhu, Taikun; Gu, Zhaoquan; Sun, Xiaoming \| 收藏 \| 浏览/下载：15/0 \| 提交时间：2023/07/12 combinatorial design ordered design Hamming code error-correcting code hat guessing game Latin matching antipodal matching Latin square and hypercube multiagent system
	Multi-scale evaluation of global evapotranspiration products derived from remote sensing images: Accuracy and uncertainty 期刊论文 OAI收割 JOURNAL OF HYDROLOGY, 2022, 卷号: 611, 页码: 20 作者: Zhu, Wenbin; Tian, Shengrong; Wei, Jiaxing; Jia, Shaofeng; Song, Zikun \| 收藏 \| 浏览/下载：34/0 \| 提交时间：2022/09/21 Evapotranspiration Satellite remote sensing Three-cornered hat Evaluation Accuracy Uncertainty
	Multi-scale evaluation of global evapotranspiration products derived from remote sensing images: Accuracy and uncertainty 期刊论文 OAI收割 JOURNAL OF HYDROLOGY, 2022, 卷号: 611, 页码: 20 作者: Zhu, Wenbin; Tian, Shengrong; Wei, Jiaxing; Jia, Shaofeng; Song, Zikun \| 收藏 \| 浏览/下载：50/0 \| 提交时间：2022/09/21 Evapotranspiration Satellite remote sensing Three-cornered hat Evaluation Accuracy Uncertainty
	Infrared dim target detecting algorithm based on multi-feature and spatio-temporal fusion 会议论文 OAI收割 Shanghai, China, 2021-10-28 作者: Bai, Mei; Zhang, Jian; Zhao, Hui \| 收藏 \| 浏览/下载：46/0 \| 提交时间：2022/03/18 Infrared Dim Target Detection TOP-HAT Improved-PM Multi-feature Fusion SCR
	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：65/0 \| 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.