区域粮食总产量预测的灰色动态模型群

应用灰色系统理论 ,建立了福建省粮食总产量的动态模式 ,分析了粮食总产量的历史变动状况 ,并对1998～ 2 0 0 5年的粮食总产量进行预测。模型采用两种特殊措施 ,极大地提高了预测精度。     

柄海鞘Styela clava化学成分的研究(Ⅱ)

从采自青岛海域的柄海鞘 Styela clava中分离得到两个化合物 (1)和 (2 )。经过 IR、MS、1HNMR和 13 CNMR等现代波谱学方法 ,确定二者的结构分别为 1- O-十六烷酰 -甘油酯和胸腺嘧啶。它们均为首次从该海域海鞘中得到。     

Period–luminosity relations for red supergiant variables – I.The calibration

We present CCD photometry of red supergiant long-period variables (LPVs) in the Per OB1 association, the Large Magellanic Cloud (LMC) and M33. The photometry was obtained in the Kron–Cousins R and I bandpasses and in a narrow bandpass ( λ ₀=8250 Å, FWHM=300 Å) chosen to avoid TiO bands in the spectral energy distribution of the LPVs. Because the strength of the TiO bands varies greatly with temperature, which varies with the phase of an LPV, avoiding TiO reduces the amplitude of the photometric variations seen in LPVs. The result is a lower dispersion and a well defined period–luminosity (PL) relation.
For the LMC sample we find an rms dispersion of 0.27 mag in the narrow-band PL relation and slightly larger dispersions for the LPVs in Per OB1 and M33. This dispersion is comparable to that of the Cepheid PL relation at similar wavelengths. Adopting a distance modulus of 18.5±0.1 mag for the LMC, we obtain distance moduli of 11.68±0.15 mag for Per OB1 and 24.85±0.13 mag for M33. These distances agree well with those based on main sequence fitting for Per OB1 and the Cepheid distance for M33. Since LPVs are ∼ 5 times more common than Cepheids and have a well defined PL relation, LPVs provide a promising method for estimating Galactic and extra galactic distances.     

Compton-thick X-ray absorption in the Seyfert galaxies Tololo 0109383 and ESO 138G1

We present analyses of the ASCA X-ray spectra of two Seyfert galaxies, Tololo 0109383 and ESO 138G1. In both cases, spectral fitting reveals two statistically acceptable continuum models: Compton reflection and partial covering. Both spectra have strong iron K lines, with equivalent widths greater than 1.5 keV. These large equivalent widths are suggestive of heavier obscuration than that directly indicated by the partial-covering models (  210²³ cm^-2),  with the actual column densities being 'Compton-thick' (i.e.   N _H1.510²⁴ cm^-2).  We use the hard X-ray/[O  iii ] flux correlation for Seyferts and data from the literature to provide additional support for this hypothesis. Since Tololo 0109383 is known to have optical type 1 characteristics such as broad Balmer line components and Fe  ii emission, this result marks it as a notable object.     

The irregular galaxy Cassiopeia 1 – a new member of the Local group

A photometry in the V, R, I (Cousins) system has been performed for stars in the galaxy Cassiopeia 1. The resulting colour-agnitude (CM) diagram of Cas 1 reveals the existence of blue stars and the absence of red ones. From an analysis of the CM diagram of the galaxy it is concluded that A_v = 4.0 mag, and the distance modulus (m – M)_o = 24.5 mag, corresponding to a distance of 790 kpc. The visual magnitude of the galaxy is V = 14^m.62 (M_v = −13^m.8) and the colour index (V – R) = 0.89 mag. From the distance determination the galaxy Cassiopeia 1 is a member of the Local group.     

基于A*算法的路网数据组织

路网的数据组织是路径规划算法设计的基础。采用C++标准模板库实现基于A*算法的路网数据组织,着重从路网的拓扑结构、空间索引、A*算法数据结构、分层和分网格组织几方面来讨论。最后给出实例证明其有效性。     

天山乌鲁木齐河源1号冰川雪坑中pH值和电导率的季节变化及淋溶过程

自2002年9月14日至2004年9月28日,在天山乌鲁木齐河源1号冰川积累区雪坑中连续观测取样,频率为1次/周。对表层雪样品和粒雪坑样品的pH值和电导率进行了分析。结果表明,表层雪的pH值和电导率具有明显的季节变化趋势,与本区域的主导山谷风风向NE和ENE密切相关。在春季,由于尘暴发生频率的增加,表层雪的pH值呈现较强碱性,电导率达到最大值;在冬季,由于原生气溶胶向次生气溶胶的转化,pH值呈现较弱碱性,电导率达到最小值。在后沉积过程中（2003年10月4日至2004年9月8日）,雪坑中不同时期的pH值和电导率呈现不同的季节变化特征和淋溶过程。电导率的峰值P1进入粒雪冰的时间比与它相对应的大粒径（直径>10 μm）微粒的浓度峰值提前40天左右;在有的雪坑中,pH值和电导率的峰值出现在污化层附近,与污化层的位置有较好的一致性,说明污化层对可溶性离子的淋溶作用可能有一定的影响。相关分析表明,Ca2+是影响表层雪中pH值和电导率变化的最主要离子。     

南阳凹陷原油含氮化合物组成及其控制因素

原油的含氮化合物总量及其组成特征不仅受原油运移距离影响,而且还受成油母质类型和成熟度影响.对南阳凹陷27个原油含氮化合物的研究表明,其油气运移指向的规律性不强,原因主要是由于原油运移距离较短,地质色层效应不明显.魏岗南部和北部原油的成熟度差异较大,但含氮化合物组成特征总体上非常相似,表明南阳凹陷原油的含氮化合物总量及其组成主要受控于成油母质类型.     

基于GM(1,1)模型的塔里木盆地南缘孤立绿洲降水灾变预测

我们选取了具有一定代表性的塔里木盆地南缘的孤立绿洲民丰县作为研究区,在对数据有效性的验证之后,利用研究区1980~1999年的降水资料,运用灰色系统理论的季节灾变预测方法,对该地区未来年份的降水量进行预测,并建立灰色季节灾变GM(1,1)预测模型,预测未来旱季到来的年份,为预测未来降水趋势提供了信息。结果表明:该研究区下一个旱灾灾变年大致指向2006年至2007年左右。这对合理利用本地气候资源具有实际意义,并且能够为研究干旱区气候变化提供一定的帮助。     

The additional radiation of Cyg X-1 at primary minimum

New UBV-photoelectric observations of the well-known massive X-ray binary system Cyg X-1/V 1357 Cyg are obtained near the primary minimum. The detailed analysis of these observations confirms the existence of additional blue radiation which appears as a narrow peak with an amplitude of 0.01–0.02 mag near phase 0.00 on the light curve (the superior conjunction of the relativistic component), firstly detected by Lyuty (1985). This emission does not appear at every orbital cycle. The appearance of this narrow peak of additional blue radiation on the light curve of Cyg X-1 can be explained as the radiation of relativistic electrons in the disturbed magnetic field of the optical star in frames of the model proposed by Ikhsanov and Fabrika (1990).