高密度云导风资料所揭示的发展和不发展热带气旋的对流层上部环流特征

国家卫星气象中心建立了一套云导风计算的算法，自１９９７年以来，国家卫星气象中心使用该算法，利用ＧＭＳ－５卫星的数据计算出西北太平洋上的１．２５经续度网格的卫得云导风。利用这套资料，对西北太平洋带气旋发展的问题进行了研究。通过研究发现，热带气旋通常是由对流层上层的西风急流引发的，那些西风急流可能是由深入到热 的中纬度槽所引起的，在盛夏季节，吹向热带对流层上部槽（ＴＵＴＴ）赤道一侧的西风也有可能引发台     

Charge exchange in massive star‐forming regions

As a result of feedback from massive stars, via their intense winds and/or supernova explosions, massive star‐forming regions are entirely filled with hot, X‐ray emitting plasmas, which escape into the ambient ISM. As shown recently by Townsley et al. for several “extreme” cases (Carina, M17, NGC 3576, NGC 3603, 30 Dor), by way of large Chandra ACIS mosaics, extra, non‐thermal emission lines are present on top of the standard lines emitted by hot plasmas. Some of them are very close to lines characteristic of charge‐exchange reactions between the hot plasma and the cold surrounding material, suggesting that this mechanism operates on large spatial scales (several 10 pc) in star‐forming regions in general. The connection with starburst galaxies is briefly mentioned, and it is pointed out that supernovae interacting with molecular clouds may also provide a good environment to look for charge exchange processes (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Numerical simulation of the structure and variation of upwelling off the east coast of Hainan Island using QuikSCAT winds

The spatial structure and variation of the upwelling in the waters east and northeast of Hainan Island, China during 2000-2007 were investigated using a nested high-resolution Princeton Ocean Model (POM) forced by QuikSCAT winds. The model produced good simulations of the summer upwelling and the seasonal and annual variability. Strong upwelling occurs from mid-July to mid-August with a peak east of Hainan Island associated with the southwesterly monsoon in the South China Sea. Sensitivity experiments indicated that when the local wind stress controls the variability of the upwelling, the large-scale circulation significantly enhances the upwelling northeast of Hainan Island by inducing a local upwelling and transporting cold water northeast-ward along the island’s east coast. The joint effects of the local wind stress and large-scale circulation result in stronger upwelling northeast of Hainan Island. This implies that the annual variation of the upwelling northeast of Hainan Island is controlled not only by the local alongshore wind stress but also by the large-scale circulation. This result will help us investigate the decadal variation of the upwelling in this region in the future.     

Gamma-ray absorption in the microquasar SS433

We discuss the gamma-ray absorption in the inner region of the microquasar SS433. Our investigation includes several contributions to the opacity of this system. They result from the ambient fields generated by the primary star, possibly an A-type supergiant, and a very extended disk around the black hole. Besides the sharp and dramatic absorption effect that occurs every time the star crosses the emission zone, we find in the UV photon field from the extended disk an important source of absorption for very high energy gamma-rays. This results in periodic gamma-ray observational signatures.     

张裂大陆边缘形成演化的数值模拟

本文在等黏态角落流模型的基础上,建立了上升离散地幔流场,将该流场作用于大陆岩石圈底部,能解释岩石圈减薄、裂解并最终形成海底扩张和张裂大陆边缘等一系列过程.数值模拟的结果表明,岩石圈在上升离散地幔流的作用下发生依赖于深度的伸展减薄,表现为不同深度的拉张因子不同,地表热流显著升高,热扰动引起的均衡调整造成地表沉降,同时热扰动造成岩石圈流变强度尤其是在变形中心处显著减小,脆性变形临界深度变浅,而韧性变形范围扩大.在上升离散地幔流的持续作用下最终导致大陆裂解,岩石圈地幔出露,形成海底扩张和张裂大陆边缘.