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	Projected near-surface wind speed and wind energy over Central Asia using dynamical downscaling with bias-corrected global climate models 期刊论文 OAI收割 ADVANCES IN CLIMATE CHANGE RESEARCH, 2024, 卷号: 15, 期号: 4, 页码: 669-679 作者: Zha, Jin-Lin; Chuan, Ting; Qiu, Yuan; Wu, Jian; Zhao, De-Ming \| 收藏 \| 浏览/下载：2/0 \| 提交时间：2024/11/28 Near-surface wind speed Wind power density Dynamical downscaling Central Asia WRF
	Potential impact of global stilling on wind energy production in China 期刊论文 OAI收割 ENERGY, 2023, 卷号: 263, 页码: 12 作者: Liu, Fa; Wang, Xunming; Sun, Fubao; Kleidon, Axel \| 收藏 \| 浏览/下载：30/0 \| 提交时间：2022/12/09 Wind energy Wind power density Global stilling Spatial distribution China
	Potential impact of global stilling on wind energy production in China 期刊论文 OAI收割 ENERGY, 2023, 卷号: 263, 页码: 12 作者: Liu, Fa; Wang, Xunming; Sun, Fubao; Kleidon, Axel \| 收藏 \| 浏览/下载：22/0 \| 提交时间：2022/12/09 Wind energy Wind power density Global stilling Spatial distribution China
	A Positive Climatic Trend in the Global Offshore Wind Power 期刊论文 OAI收割 FRONTIERS IN ENERGY RESEARCH, 2022, 卷号: 10, 页码: 22 作者: Zheng, Chong-wei; Yi, Cheng-tao; Shen, Chong; Yu, De-chuan; Wang, Xiao-lu \| 收藏 \| 浏览/下载：41/0 \| 提交时间：2022/08/10 global ocean wind energy resource wind power density effective wind speed occurrence rich level occurrence climatic trend
	A Positive Climatic Trend in the Global Offshore Wind Power 期刊论文 OAI收割 FRONTIERS IN ENERGY RESEARCH, 2022, 卷号: 10, 页码: 22 作者: \| 收藏 \| 浏览/下载：4/0 \| 提交时间：2024/11/15 global ocean wind energy resource wind power density effective wind speed occurrence rich level occurrence climatic trend
	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：54/0 \| 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.
	On wind speed pattern and energy potential in China 期刊论文 OAI收割 APPLIED ENERGY, 2019, 卷号: 236, 页码: 867-876 作者: Liu, Fa; Sun, Fubao; Liu, Wenbin; Wang, Tingting; Wang, Hong \| 收藏 \| 浏览/下载：67/0 \| 提交时间：2019/05/22 Wind power density Wind speed Seasonal variation Spatial distribution China
	On wind speed pattern and energy potential in China 期刊论文 OAI收割 APPLIED ENERGY, 2019, 卷号: 236, 页码: 867-876 作者: Liu, Fa; Sun, Fubao; Liu, Wenbin; Wang, Tingting; Wang, Hong \| 收藏 \| 浏览/下载：12/0 \| 提交时间：2019/05/22 Wind power density Wind speed Seasonal variation Spatial distribution China