结合濮阳实际 鼓励开发地上地下空间

随着濮阳市城市框架的不断拉大,建设用地需求不断增加,在国家紧缩＂地根＂的形势下,做好节约集约用地工作尤为重要。今后各项建设要优先开发利用空闲、废弃、闲置和低效利用的土地,努力提高建设用地利用效率,严格执行闲置土地处置政策。重点在盘活城镇存量上下工夫,提高土地利用效益。     

Evolutionary status of the pre-protostellar core L1498

L1498 is a classic example of a dense cold pre-protostellar core. To study the evolutionary status, the structure, dynamics, and chemical properties of this core we have obtained high spatial and high spectral resolution observations of molecules tracing densities of 10(3)-10(5) cm-3. We observed CCS, NH3, C3H2, and HC7N with NASA's DSN 70 m antennas. We also present large-scale maps of C18O and 13CO observed with the AT&T 7 m antenna. For the high spatial resolution maps of selected regions within the core we used the VLA for CCS at 22 GHz, and the Owens Valley Radio Observatory (OVRO) MMA for CCS at 94 GHz and CS (2-1). The 22 GHz CCS emission marks a high-density [n(H2) > 10(4) cm -3] core, which is elongated with a major axis along the SE-NW direction. NH3 and C3H2 emissions are located inside the boundary of the CCS emission. C18O emission traces a lower density gas extending beyond the CCS boundary. Along the major axis of the dense core, CCS, NH3 and C3H2 emission show evidence of limb brightening. The observations are consistent with a chemically differentiated onion-shell structure for the L1498 core, with NH3 in the inner and CCS in the outer parts of the core. The high angular resolution (9"-12") spectral line maps obtained by combining NASA Goldstone 70 m and VLA data resolve the CCS 22 GHz emission in the southeast and northwest boundaries into arclike enhancements, supporting the picture that CCS emission originates in a shell outside the NH3 emitting region. Interferometric maps of CCS at 94 GHz and CS at 98 GHz show that their emitting regions contain several small-scale dense condensations. We suggest that the differences between the CCS, CS, C3H2, and NH3 emission are caused by a time-dependent effect as the core evolves slowly. We interpret the chemical and physical properties of L1498 in terms of a quasi-static (or slowly contracting) dense core in which the outer envelope is still growing. The growth rate of the core is determined by the density increase in the CCS shell resulting from the accretion of the outer low-density gas traced by C18O. We conclude that L1498 could become unstable to rapid collapse to form a protostar in less than 5 x 10(6) yr.     

Detection of a new interstellar molecular ion, H2COH+ (protonated formaldehyde)

A new interstellar molecular ion, H2COH+ (protonated formaldehyde), has been detected toward Sgr B2, Orion KL, W51, and possibly in NGC 7538 and DR21(OH). Six transitions were detected in Sgr B2(M). The 1(1,0)-1(0,1) transition was detected in all sources listed above. Searches were also made toward the cold, dark clouds TMC-1 and L134N, Orion (3N, 1E), and a red giant, IRC + 10216, without success. The excitation temperatures of H2COH+ are calculated to be 60-110 K, and the column densities are on the order of 10(12)-10(14) cm-2 in Sgr B2, Orion KL, and W51. The fractional abundance of H2COH+ is on the order of 10(-11) to 10-(9), and the ratio of H2COH+ to H2CO is in the range 0.001-0.5 in these objects. The values in Orion KL seem to be consistent with the "early time" values of recent model calculations by Lee, Bettens, & Herbst, but they appear to be higher than the model values in Sgr B2 and W51 even if we take the large uncertainties of column densities of H2CO into account. We suggest production routes starting from CH3OH may play an important role in the formation of H2COH+.     

Near-infrared spectroscopy of dark asteroids

Near-infrared (J, H and K bands) spectra of nine dark asteroids (chosen among a sample of supposed primitive objects between C and D classes) have been obtained at the Mauna Kea Observatory (Hawaii) with the 2.2-m telescope using KSPEC as spectrograph. The aim of this work was to search for evidence of the presence of organic materials in these objects as found in other planetary bodies as 5145 Pholus, and in some cometary nuclei. A careful analysis of the data has revealed flat or slightly redder spectra than the solar one for all observed asteroids. No evidence of distinct absorption features was found.     

山东省日照市蓝色经济区工程建设适宜性评价

本文以山东省日照市蓝色经济区为研究区, 通过野外地质调查和室内综合分析, 选取场地稳定性、工程地质条件、地下水条件, 地形排水条件、地质灾害及其他因素6个一级评价因子, 构造活动、场地土类型、建筑场地类别等13个二级评价因子, 利用专家-层次分析定权法进行区内工程建设适宜性评价, 得到了相应工程建设评价分区图。评价结果表明, 日照市场地工程建设适宜性总体较好, 大部分地区适宜进行高层建筑工程建设, 占84.50%; 地下空间开发利用条件优越, 全区多数地区属于城市地下空间建设适宜区, 适宜性差及不适宜区主要分布在付疃河两岸附近和海岸附近、大型高速公路和铁路沿线一带区域及城区; 轨道交通建设适宜性良好, 小部分不适宜区主要集中在付疃河下游夹仓和小古镇一带及其沿海地区。评价结果可有效地服务于该地区规划布局、建设发展和工程选址, 具有重要的理论和实践指导意义。     

含煤层地质环境下地震波场的数值模拟

本文对含低速煤层地质环境下弹性波场多波多分量地震资料进行了二维数值模拟研究,对人工边界反射进行了有效处理,频散效应得到了有效的压制,对几种不同激发与观测排列方式下的弹性波资料进行了模型计算与分析。     

Is Russia's demographic situation improving?

"Since the Russian economy recently has shown sings of stabilization, there now is evidence that demographic trends are beginning to improve somewhat. Although the population declined by 164,200, to 148.1 million at the beginning of 1996, the release of new statistical compendia by the Russian statistical agency (Goskomstat Rosii) in 1995 and early 1996 makes it possible to identify several positive trends.... Life expectancy increased for the first time since 1985. The infant mortality rate declined for the second year in a row. The crude death rate declined for the first time in a decade. The birth rate remained at about the same level for the third consecutive year. The rate of natural increase (births minus deaths), although still negative, recorded a moderate increase."     

类星体光学波段连续谱的统计特性与K订正

从假定类星体的红移属于运动红移出发,利用355个有色指数和红移资料的类星体,用统计平均方法消除发射线的影响,求得类星体连续谱,并可以用幂律谱分段拟合,由此求得新的更加合理的K订正值。     

光变幅度不大于0~m.5类星体的视星等——红移关系

一、引言在类星体的研究中,对红移性质的认识,一直是关键问题之一。红移是宇宙学的?还是内禀的?还是二者都有?有待于人们通过更多的天文观测与理论分析加以确定。如果红移是宇宙学的,则视星等——红移关系,就应该符合哈勃图。但将所有类星体作哈勃图,会出现严重的弥散现象。为了揭示类星体红移的本质,对类星体进行标准烛光     

Ethnic results of the 1979 Soviet census

This article is based on summary results concerning ethnic composition in the USSR according to the 1979 census. "These results...have been rearranged... to reflect not only the ethnic composition of the USSR and of its republics over time (1959, 1970, 1979), but also shifts in the distribution of particular ethnic groups. Furthermore, ethnic groups are discussed in a regional sequence. In combination with the migration tables based on previous results of the 1979 census...some conclusions can be drawn concerning the ethnic makeup of migrants among republics."