宇宙磁场中的中微子

本文讨论了有质量的Dirac粒子在宇宙磁场中的演化。宇宙磁场使空间度规出现各向异性。通过求解Dirac方程,得到了中微子在宇宙磁场中的表观磁矩。     

武夷山脉中段晚太古代宇宙尘特征

武夷山脉中段晚太古代宇宙尘赋存于上太古界天井坪组。粒度一般为0．15-0.2mm，最大0.32mm，最小0.042mm,形态呈单球体、不规则形或碎片状，以前者为主。在扫描电镜下表面具烧蚀、蜂巢状气印、气孔状、刺(瘤)突趁、晶洞及偏心双层等结构。宇宙尘由内核和熔壳组成；内核是自然铁(a-Fe)，含Fe、Cr、Ni、Co等元素；熔壳是磁铁矿或方铁矿，除Fe外尚含Si、Al、Cr、Mn、S等元素：根据其结构、构造组成和物质成分的综合分析结果，并与国内文献资料进行对比，本区宇宙尘可能是铁陨石在大气中的消融物或在太空中的碎裂物。     

堂堂正正做人认认真真求知勤勤恳恳敬业清清白白干事

建设“廉洁国土”是新形势下认真贯彻落实中央关于反腐倡廉要求的重要载体,也是树立国土资源系统“亲民、爱民、为”良好形象的内在需要.建设“廉洁国土”关键在人、取决于人,根本在于国土资源系统每位工作人员人人争做“廉洁”型干部,严格遵循光明磊落、坦荡处事的人生准则,保持敢于进取、永不满足的探索精神,树立务实高效、雷厉风行的工作作风,坚守公私分明、刚正不阿的律己标准.也就是每位“国土”人都要堂堂正正做人,认认真真求知,勤勤恳恳敬业,清清白白干事,从做人、学习、工作、廉政等各方面来规范自己、约束自己和完善自己.     

宇宙常数与宇宙年龄问题

本文用球对称扰动模型导出了星系暗晕的平均密度与形成时间的关系 ,并由此估算银河系的形成时间tV.我们把球状星团的年龄作为银河系年龄tG 的代表 ,则tG tV 是宇宙年龄 .对Ωλ=0 ,0 .7和 0 .8的平坦宇宙模型 ,本文计算并讨论了能与它相洽的哈勃常数的范围 .结果表明 ,若哈勃常数大到 80km·s- 1 Mpc- 1 左右 ,引入宇宙常数并不一定能解决宇宙年龄的矛盾     

Sequences in the Hardness Ratio-Peak Energy Plane of Gamma-Ray Bursts

The narrowness of the distribution of the peak energy of the vFv spectrum of gamma-ray bursts (GRBs) and the unification of GRB populations are great puzzles yet to be solved. We investigate the two puzzles based on the global spectral behaviors of different GRB populations, the long GRBs, the short GRBs, and the X-ray flashes (XRFs), in the HR - Ep plane (HR the spectral hardness ratio) with BATSE and HETE-2 observations. It is found that the long GRBs and the XRFs observed by HETE-2 seem to follow the same sequence in the HR-Ep plane, with the XRFs at the low end of this sequence. We fit the sequence by a universal Band function, and find that this sequence is mainly defined by the low energy index α, and is insensitive to the high energy index,β. With fixed β=-5, a best fit is given by α=-1.00 with X^2min/dof=2.2. The long and short GRBs observed by BATSE follow significantly different sequences in the HR-Ep plane, with most of the short GRBs having a larger hardness ratio than the long GRBs at a given Ep. For the long GRBs a best-fit yields α=-0.30 and β=-2.05. For the short GRBs, a best fit gives α=-0.60 with x^2min=1.1 (withβfixed at-2.0 because it is numerically unstable). The α value for the short GRBs is significantly greater than that for the long GRBs. These results indicate that the global spectral behaviors of the long GRB sample and the XRF sample are similar, while that of the short GRBs is different. The short GRBs seem to be a unique subclass of GRBs, and they are not the higher energy extension of the long GRBs.     

Rhombic Cell Analysis. Ⅱ. Application to the IRAS／PSCz Catalogue

Rhombic cell analysis as outlined in the first paper of the present seriesis applied to samples of varying depths and liming luminosities of the IRAS/PSCzCatalogue. Numerical indices are introduced to summarize essential information.Because of the discrete nature of the analysis and of the space distribution of galax-ies, the indices for a given sample must be regarded as each having an irreduciblescatter. Despite the scatter, the mean indices show remarkable variations acrossthe samples. The underlying factor for the variations is shown to be the limitingluminosity rather than the sampling depth. As samples of more and more luminousgalaxies are considered over a range of some 2.5 magnitudes (a factor of some 75in space density), the morphology of the filled and empty regions defined by thegalaxies degrades steadily towards insignificance, and the degrading is faster for thefilled than the empty region.     

山东招远金矿矿石中首次发现宇宙尘埃—镍纹石

招远金矿田的人工重砂样品中首次发现宇宙尘埃——镍纹石.文中介绍了镍纹石的形态特征、物理性质和x射线粉晶与红外光谱分析结果.在此基础上,作者进一步认定招远金矿是在地层经过混合岩化和花岗岩化作用保留下来的产物.     

白城农村集体土地使用权流转的几点思考

在市场经济条件下，土地作为一种资源和生产要素，必然要求合理流动和优化配置。这是一个不可阻挡的发展趋势。近年来，各地围绕农村集体土地的流转问题进行了大胆的探索，创造出了农地流转的各种模式。吉林省白城市在这个改革的大潮中，有2万多农户自发地投入了这个潮流。他们的实践带给了我们许多宝贵的启示。     

次生悬浮颗粒物与海域生命元素的内循环

重点讨论近岸海域海洋资源开发过程中所诱发产生的次生悬浮颗粒物的产生机制，及其对近岸海域水体中生命元素的生物地球化学的行为，过程和内循环等诸环节的效应。该物质很大程度上决定了海域水体中的生命元素的存在形态，含量水平。因此，可能成为近岸水体富营养化的潜在威胁。     

矿集区预测中的探索式空间分析方法及应用——以中亚铜矿集区预测为例

随着地理信息科学和计算机技术的发展,计算环境下矿集区预测方法的研究热潮也初现端倪.依据矿集区所包含的理论内涵(矿床密集区、潜力密集区的聚集内涵),提出了应用探索式空间分析法进行矿集区预测的设想,并以北至科克舍套,南至帕米尔高原,西至乌拉尔山,东至新疆边境的中亚区域为研究区,利用探索式空间分析方法从含矿潜力的确定及其空间分布模式的探索入手,对研究区铜矿集区进行了预测,初步圈定了乌拉尔、矿区阿尔泰、北滨巴尔喀什、斋桑、塔尔巴合台等17处铜矿集区.研究成果除包含了研究区已知矿集区外,还有7处新区,反映了探索式空间分析法在矿集区预测中的应用潜力.