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	Pre-Existing Off-Fault Damage Can Impede Coseismic On-Fault Slip 期刊论文 OAI收割 GEOPHYSICAL RESEARCH LETTERS, 2024, 卷号: 51, 期号: 23, 页码: 9 作者: Wu, C. H.; Cui, P.; Klinger, Y.; Tan, X. B.; Yi, S. J. \| 收藏 \| 浏览/下载：10/0 \| 提交时间：2025/01/15 earthquake coseismic slip pre-existing off-fault damage fault zone structure field evidence
	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：52/0 \| 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.
	The positive influence of boron-doped graphene for its supported Au clusters: enhancement of SERS and oxygen molecule adsorption 期刊论文 OAI收割 PHYSICAL CHEMISTRY CHEMICAL PHYSICS, 2012, 卷号: 14, 期号: 39, 页码: 13564 Kong, XK; Sun, ZY; Chen, QW 收藏 \| 浏览/下载：20/0 \| 提交时间：2013/09/23 RESONANCE RAMAN-SCATTERING DIRECT VISUAL EVIDENCE CHARGE-TRANSFER CHEMICAL MECHANISM SURFACE PYRIDINE GOLD REDUCTION FIELD AG
	Magnetostratigraphy of deep drilling core SG-1 in the western Qaidam Basin (NE Tibetan Plateau) and its tectonic implications 期刊论文 OAI收割 QUATERNARY RESEARCH, 2012, 卷号: 78, 期号: 1, 页码: 139-148 Zhang WL (张伟林); Appel E (Appel, Erwin); Fang XM (方小敏); Song CH (Song, Chunhui); Cirpka O (Cirpka, Olaf) 收藏 \| 浏览/下载：18/0 \| 提交时间：2013/05/23 RESOLUTION MAGNETO STRATIGRAPHY ASTRONOMICAL CALIBRATION PALEOMAGNETIC EVIDENCE ENVIRONMENTAL-CHANGES CENOZOIC DEFORMATION GEOMAGNETIC-FIELD QINGHAI PROVINCE CENTRAL-ASIA GUIDE BASIN UPLIFT
	Texture-preserving despeckling of sar images using evidence framework 期刊论文 iSwitch采集 Ieee geoscience and remote sensing letters, 2007, 卷号: 4, 期号: 4, 页码: 537-541 作者: Li, Heng-Chao; Hong, Wen; Wu, Yi-Rong; Tai, Heng-Ming 收藏 \| 浏览/下载：24/0 \| 提交时间：2019/05/10 Evidence framework Gaussian markov random field (gmrf) Speckle reduction Synthetic aperture radar (sar)