Chemical Enrichment of the Intra-Cluster Medium

We investigate the metal enrichment of the intra-cluster medium by using a method that combines N-Body simulations and a semi-analytic model (SAM) of galaxy formation. The cluster of galaxies is simulated in a flat, low density universe, with a numerical resolution that allows the detection of substructures in the dark matter background of the cluster. The phenomenological approach used to model the physical processes involved in the galaxy formation and metal production is applied to the substructures found in the dark matter halos detected at different redshifts. Details of the chemical implementation in the SAM and first results related to the mean properties of the baryonic matter components are presented. This revised version was published online in August 2006 with corrections to the Cover Date.     

Strong interplanetary field enhancements at Ulysses—evidence of dust trails' interaction with the solar wind?

Interplanetary field enhancements were first discovered in the vicinity of Venus. These events are characterised by an increase in the magnitude of the heliospheric magnetic field with a near-symmetrical, sometimes thorn-shaped profile, and last from minutes to hours. Surveys of the events near Venus and Earth indicated clustering of the events in inertial space, which suggested that their sources were Solar System objects other than the Sun. A survey is presented of strong events of this type detected by the Ulysses spacecraft from 1990 to late 2001. Most of the events are accompanied by a discontinuity in the field direction near the events' centres. Other discontinuities are often symmetrical about the enhancement. The majority of events last less than two hours. When examined as a whole, the events tend to be accompanied by subtle changes in some plasma parameters. The majority of the enhancements are accompanied by magnetic holes on their fringes. The enhancements' occurrence rate increases with decreasing heliocentric distance. Possible formation mechanisms are discussed. No link was found with solar, or solar wind sources. Several aspects of the survey results are consistent with an origin related to cometary dust trails. Possible processes associated with a dust-solar wind interaction are discussed.     

介质横向不均匀对震后地表位移场的影响

利用三维有限元模拟两层地球模型(包括弹性层和粘弹性层)介质的横向不均匀和断层错动的复杂性对震后地表位移场的影响，其数值结果包括弹性解和粘弹性解。结果表明，震后位移场的分布特征不仅与粘弹性层的流变特性有关，还与弹性层介质的剪切模量以及断层的同震错动有关。     

REVIEWS OF GEOGRAPHIC SOFTWARE

Reviews of geographic software in this article: DEMO-GRAPHICS: WORLD POPULATIONS AND PROJECTIONS. ESP GAUSS. CEMODEL S. Damus LIMDEP. William H. Greene MICROSTAT 4.1 OTIS PCIPS. (Personal Computer Image Processing System) . H.J. Meyers and R. Bernstein. REGRESSION ANALYSIS OF TIME SERIES (RATS) SPSS/PC+ URBAN DATA MANAGEMENT SOFTWARE (UDMS)     

太子河流域辽阳—本溪间的■类动物群

太子河流域西部竹蜓类动物群，以本溪—牛心台地区为最发育，一般可划分为一个共存延限带，一个组合带，后者又可进一步划分为３个组合亚带。ⅡＦｕｓｕｌｉｎａ－Ｆｕｓｕｌｉｎｅｌａ组合带３Ｆｕｓｕｌｉｎａｃｙｌｉｎｄｒｉｃａ－Ｆ．ｑｕａｓｉｃｙｌｉｎｄｒｉｃａ组合亚带２Ｆｕｓｕｌｉｎｅｌａｐｒｏｖｅｃｔｕ－Ｆｕｓｕｌｉｎａｐｓｅｕｄｏｋｏｎｎｏｉ组合亚带１Ｆｕｓｕｌｉｎａｓｃｈｅｌｗｉｅｎｉ－Ｆ．ｍａｙｉｅｎｓｉｓ组合亚带ⅠＰｒｏｆｕｓｕｌｉｎｅｌａｐａｒｖａ－Ｅｏｓｔａｆｅｌａｓｕｂｓｏｌａｎａ共存延限带Ｐｒｏｆｕｓｕｌｉｎｅｌａｐａｒｖａ系作者等研究辽南竹蜓类并建带的带分子，Ｅｏｓｔｕｆｆｅｌａｓｕｂｓｏｌａｎａ为盛金章教授建立的辽东本溪群下部竹蜓带的带分子，时代为中石炭世早期。Ｆｕｓｕｌｉｎａ－Ｆｕｓｕｌｉｎｅｌａ组合带代表本区及东北南部最发育的竹蜓类动物群。该带属于中石炭世中—晚期，也是太子河流域最大海侵期。以上二个竹蜓类生物带总体应属于Ｍｏｓｃｏｖｉａｎ阶，时代为中石炭世。