An Anisotropic Cosmic-Ray Enhancement Event on 07-June-2015: A Possible Origin

A usual event, called anisotropic cosmic-ray enhancement (ACRE), was observed as a small increase (\({\leq}\,5\%\)) in the count rates of polar neutron monitors during 12?–?19 UT on 07 June 2015. The enhancement was highly anisotropic, as detected only by neutron monitors with asymptotic directions in the southwest quadrant in geocentric solar ecliptic (GSE) coordinates. The estimated rigidity of the corresponding particles is \({\leq}\,1\) GV. No associated detectable increase was found in the space-borne data from the Geostationary Operational Environmental Satellite (GOES), the Energetic and Relativistic Nuclei and Electron (ERNE) on board the Solar and Heliospheric Observatory (SOHO), or the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) instruments, whose sensitivity was not sufficient to detect the event. No solar energetic particles were present during that time interval. The heliospheric conditions were slightly disturbed, so that the interplanetary magnetic field strength gradually increased during the event, followed by an increase of the solar wind speed after the event. It is proposed that the event was related to a crossing of the boundary layer between two regions with different heliospheric parameters, with a strong gradient of low-rigidity (\({<}\,1\) GV) particles. It was apparently similar to another cosmic-ray enhancement (e.g., on 22 June 2015) that is thought to have been caused by the local anisotropy of Forbush decreases, with the difference that in our case, the interplanetary disturbance was not observed at Earth, but passed by southward for this event.     

Teleportation and thermal entanglement in two-qubit Heisenberg XYZ spin chain with the Dzyaloshinski—Moriya interaction and the inhomogeneous magnetic field

This paper studies the average fidelity of teleportation and thermal entanglement for a two-qubit Heisenberg XYZ chain in the presence of both an inhomogeneous magnetic field and a Dzyaloshinski--Moriya interaction. It shows that for a fixed D_z, the increase of b_z will broaden the critical temperature at the cost of decreasing the thermal entanglement. And it can modulate the inhomogeneous magnetic field and the Dzyaloshinski--Moriya interaction for the average fidelity of teleportation to be optimal.     

三疣梭子蟹和华溪蟹主要器官比较组织学的初步研究

近年来随着养殖业的发展,蟹类病害频繁发生,日趋严重。在开展病害研究过程中,由于三疣梭子蟹Portunus trituberculatus的SPF(无特定病原体)材料难于获得,而试验蟹的获得又受到养殖条件、养殖周期等因素的限制,因此阻碍了相关研究的开展,尤其是病毒学研究的进展。筛选一种可替代的模式生物,并开展相关研究显得尤为迫切。华溪蟹Sinopotamon和三疣梭子蟹亲缘关系较近,作为野生的蟹类容易获得,价格低廉,也容易在实验室条件下饲养。笔者在梭子蟹病原研究中发现,华溪蟹不带梭子蟹病原,但在实验条件下可感染相关病原,是开展此两类蟹病原体研究的较好实验动物,有必要开展这两种蟹的组织比较形态学的基础研究,以支持相关的应用研究。笔者经过对三疣梭子蟹和华溪蟹的组织石蜡切片观察发现,两种蟹的各组织器官结构基本相似,各组织结构都由4层构成,即粘膜层、粘膜下层、肌层和外膜。上皮细胞分泌物形成几丁质板,覆盖在上皮细胞表面。三疣梭子蟹的食管粘膜下层较发达。华溪蟹食管粘膜下层的肌层均相对较薄,食管腔较小。这两种蟹的胃壁结构无明显差别。在三疣梭子蟹的局部胃壁,可见嗜酸性几丁质层,上皮细胞顶部间有间隙,间隙中有一些嗜碱性物质。三疣梭子蟹肠粘膜下层不明显。华溪蟹的中肠非常细小,被肝胰腺等组织包裹,难以分离,管腔小,管壁外结缔组织少。两种蟹肝胰腺均由许多分枝的肝小管组成,小管间为结缔组织,血窦。肝小管由单层柱状上皮构成,高低不等,可以明显区分出分泌细胞、吸收细胞、储存细胞和胚性细胞4种形态的细胞,其功能也不同。三疣梭子蟹鳃轴基本弯曲,窄处鳃轴与鳃丝粗细相当,鳃丝和鳃小片间隔较大。华溪蟹鳃轴笔直延伸,窄处鳃轴明显粗于鳃丝,鳃丝间隔较小。两者鳃小片均由扁平上皮组成,外侧有薄层几丁质板。华溪蟹的鳃血管中可以明显看到较多染成红色的血细胞。三疣梭子蟹心肌纤维排列松散,线粒体较少,形态多样。华溪蟹心肌纤维排列致密,线粒体多呈群分布,且数量更多。心肌由梭形心肌细胞组成,有横纹,彼此相连成网,其周围有少量原生质。肌细胞的核呈棒状。     

内湾沉积物生物硅化学测定法的实验条件探讨

对国内外已经建立的几种生物硅的测定方法进行简要的评述,并详细地对内湾沉积物中生物硅化学提取法的条件选取进行实验探讨,对低生物硅含量的内湾沉积物测定提出了较优的条件。     

绿鳍马面鲀重复发育雄性生殖腺结构与发育组织学观察

采用常规石蜡切片、HE组织染色法研究了性成熟绿鳍马面鲀雄性生殖腺结构和发育组织学。结果表明,性成熟绿鳍马面鲀精巢从外形上明显分为上、下两段,上段为生精部,下段为贮精囊。生精部分为2支,呈黄色、长条状;生精部为典型的小叶型结构;精小叶间有间质(Leydig)细胞。其生精部的发育历程可分为重复发育Ⅲ期、精子形成Ⅳ期、精子成熟Ⅴ期和退化吸收Ⅵ期。贮精囊位于精巢的后方并通过壶腹与生精部相连,贮精囊为椭圆形,白色不分支,其组织结构与贮存精子功能相适应,由许多被结缔组织分开的管状囊腔组成;贮精囊组织学变化与生精部周期性的变化相关,又有相对的独立性,也有周期发育,可分为恢复期、生殖期和退化期。     

内蒙古干湿环境演变与地区生态建设优势气候背景分析

通过内蒙古地区近46 a降水和潜在蒸散量以及湿润度在气温突变前后的倾向率和差值变化分析,得出该区域主要植被类型干湿环境演变的时空变化特征。研究结果表明：降水在气温突变前“东增西减”,突变后呈相反的变化趋势。46 a降水倾向率增加区域主要集中在呼伦贝尔市东部和乌兰察布市以西大部地区;潜在蒸散量在气温突变前呈减少趋势,突变后有增加趋势,突变后潜在蒸散量明显小于突变前。内蒙古46 a潜在蒸散量倾向率大部地区偏小,偏大区域仅存在于中东部偏北地区,气温突变后全区大部地区存在明显的“蒸发悖论”;大兴安岭西麓和乌兰察布市以西地区突变后湿润度增加明显,暖湿的气候环境有利于当地植被建设和生态恢复,内蒙古东南部、呼伦贝尔草原和锡林郭勒盟草原区有暖干化趋势,上述草原区存在潜在退化风险。     

放牧对浑善达克沙地丘间低地植被群落及土壤的影响

为探究放牧对丘间低地植被群落及土壤的影响,分析了浑善达克沙地丘间低地在重度和轻度放牧下植被的地上生物量、物种重要值、物种丰富度、Shannon-Wiener多样性指数、Pielou均匀度指数、Simpson生态优势度指数及0~10 cm土壤中黏粒、粉粒、砂粒、有机碳和全氮含量。结果表明：（1）植被地上生物量、土壤黏粒、粉粒、砂粒、土壤有机碳和全氮含量在不同放牧程度下存在极显著差异（P<0.01）,物种丰富度、Shannon-Wiener多样性指数和Pielou均匀度指数在不同放牧程度下差异不显著（P>0.05）,Simpson生态优势度指数在不同放牧程度下差异显著（P<0.05）。（2）放牧区植被以禾本科为主,禾本科植被地上生物量占整个植被群落的54.88%~57.76%;重度放牧区植被地上生物量为63.59 g·m^-2,比轻度放牧区低26.61%。（3）羊草（Leymus chinensis）和狗尾草（Setaria viridis）是放牧区的优势种,其重要值依次为14.16%（重度放牧区）和19.10%（轻度放牧区）、13.40%（重度放牧区）和15.42%（轻度放牧区）,重度放牧下雾滨藜（Bassia dasyphylla）、克氏针茅（Stipa krylovii）和猪毛蒿（Artemisia scoparia）的重要值较显著高于轻度放牧区,而羊草则低于轻度放牧区。（4）重度放牧加剧了土壤沙漠化,使砂粒含量增加,草地生产力下降,土壤有机碳和全氮含量降低。     

浅谈计算机技术在煤矿储量估算中的应用

介绍了在煤矿储量估算中应用Microsoft Excel制作各种表格及计算,同时应用MAPGIS软件直接绘制储量估算图,提高图件的精度及节省绘制图件的时间。     

前期印度洋海温异常对中国春季降水的影响

为了进一步认识印度洋海温的异常变化与中国降水的关系,采用SVD分析、相关分析及合成差值分析讨论了前期冬季关键区海温的异常变化对中国春季降水影响的差异,探讨了产生这种影响的原因。结果表明:前期冬季关键区海温的异常增高(降低),会造成后期春季中国华北往南到华中、华东、华南东部及西北的新疆地区的降水明显增多(减少),西南的四川、贵州及华南的广西等地降水会有所减少(增多)。与关键区冷年相比,在关键区的暖年,环流形势反映出东欧槽显著减弱,北方气压显著降低,蒙古高压明显减弱,冷空气南下更为明显,而华南东部、华中、华东及华北一直被较为显著的南风气流控制,海洋的暖湿气流向中国内陆输送更为显著,使得东部及中部大部分地区水汽较为充沛,形成大面积的降水。     

Gyldén Model: The Slowly Changing Equivalent Gravitational Parameter

In the Gyldén problem, the case of slowly changing equivalent gravitational parameter (e.g.p.) is studied. Assuming the following law for the variation of the e.g.p.: μ (t) = μ₀+ εμ (εt), ε< μ₀, we obtained a) a O(ε⁴ T⁴)-approximation of the solution, on a shortened time scale (0,T), with T of order o(ε^-1),for the general case (i.e. the support function μ is O(1)-valued and admits an expansion in power series of its argument), and b) a O(ε²)-approximation of the solution, on a natural timescale of order O(1/ε), for the case of a bounded variation rate (i.e. the support function μ and its derivative are both O(1)-valued). For the study of the first problem we introduced a type of Lissajous variables and used the Lie-Hori normalization scheme; for the second problem we used the Delaunay variables and applied the von Zeipel method for approximate integration. The physical interpretation of the results is in both cases the same: within the corresponding limits of approximation, the variation of e.g.p. (i) has no effect on the size of the osculating ellipse, (ii) it sets the pericenter in slow rotation and (iii) it introduces a secular variation in the longitudes. This revised version was published online in July 2006 with corrections to the Cover Date.