降水对荒漠土壤水热性质强迫研究

利用“我国西北干旱区陆气相互作用试验”在甘肃省敦煌的观测资料,分析了不同大小的降水对土壤湿度、反照率以及地表温度的影响;随着降水量的增大,各地表物理量恢复到原先的状态也越慢;强降水时,5cm土壤湿度的驰豫期为7天．中降水为4天,微量降水为2天。由于降水性质(水和雪)和土壤状态的差异,冬季和夏季相比．降水对地表物理量的影响差不多,但冬季地表物理量的恢复时间要比夏季长得多。土壤湿度和反照率的驰豫期与降水有很好的相关。     

广州城市交通系统与空间格局互动影响研究

该文在评述国内外相关研究的基础上,阐释城市交通系统与空间格局之间的互动影响关系。对广州城市交通系统与空间格局之间的互动影响关系的研究结果表明：广州城市交通系统的发展对空间格局的形成与发展有引导作用;城市空间格局的变化会产生反馈作用,客观上影响着交通系统的空间布局,两者之间存在—个互动反馈作用环。     

混合热源与热泵联动空调技术及其在天津"975"工程中的应用

混合热源与热泵联动空调技术以天然、廉价和低品位的资源为主,以高品位资源为尖峰负荷的系统能源配置设计新方法,实现以单投入多功能的新型能源利用方式替代多投入单功能传统的能源利用方式,使建筑物的空调系统具有经济、节能与环保等特点.该项技术能较好地应用于能源获取难度大、单一冷热源不能满足要求的工程.在天津"975"工程供暖及制冷系统中的应用结果表明:混合热源与热泵联动空调技术成功地解决了系统的冷热源、热(冷)负荷需求大等难题,具有明显的环境与经济效益.     

中国历史大疫的时空分布及其规律研究

文章从甲骨文、二十五史、十三经、古医书、笔记和杂录、地方志、类书中,获取了中国历史大疫385条(公元前13世纪至1911年)。进而,对385奈疫情的烈度进行定量分级,分析中国历史大疫的时间分布、空间分布,并提出了一些规律性见解：在历史上中国是大疫频繁发生的国家;3000多年大疫史上有两个活跃期(公元2～3世纪、16～19世纪),且有愈后愈多之势,从百年一遇,到数十年一遇、数年一遇;东部多,西部少,以长江中下游和黄河中下游地区为最甚;存在着灾害链,有旱—疫、涝—疫、饥—疫等10多种灾害链。     

A new mixing equation for bed material composition in bed form dominant conditions

Vertical mixing beneath the bed surface and its effect on sediment composition has long been underestimated. This paper proposes a mixing equation to illustrate the temporal and spatial variations of bed material composition for bed form dominant rivers. A continuous mass conservation equation for elevation-specific nonuniform bed material composition is initially presented. A vertical mixing equation is finally derived as a diffusion-type partial differential equation with a source term charact...     

Chromothermal oscillations and collapse of strange stars to black holes: astrophysical implications

We study the effects of temperature on strange stars. It is found that the maximum mass of the star decreases with the increase of temperature, as at high temperatures the equations of state become softer. Moreover, if the temperature of a strange star increases, keeping its baryon number fixed, its gravitational mass increases and its radius decreases. This leads to a limiting temperature, where it turns into a black hole. These features are the result of a combined effect of the change of gluon mass and the quark distribution with temperature. We report on a new type of radial oscillation of strange stars, driven by what we call 'chromothermal' instability. We also discuss the relevance of our findings in the astrophysics of core collapse supernovae and gamma-ray bursts.     

On the extraction of extended structure from Herschel-SPIRE scanning observations in the presence of 1/f noise

We present results from a study of the impact of uncorrelated 1/ f noise on the extraction of spatial structure, on a range of scales, from sky mapping observations made using the Herschel-SPIRE (the spectral and photometric imaging receiver) photometer in the scan-map mode. These studies were carried out using a detailed instrument simulator, and the output reduced using the map-making algorithm to be implemented in the SPIRE data pipeline. The influence of source size scale, telescope-scanning rate and 1/ f noise knee frequency is investigated, and operational bounds to the expected losses are presented, using the case of zero 1/ f (white) noise as a benchmark. Both cross-linked and non-cross-linked observing options are studied. The results presented here represent the best current estimate of the sensitivity of the SPIRE photometer to emission on arbitrary scales. The data presented are general and scalable to any SPIRE observation made using the scanning mode.     

Comparison of Meteoroid Flux Models for Near Earth Space

Over the last decade several new models for the sporadic interplanetary meteoroid flux have been developed. These include the Divine-Staubach and the Dikarev model. They typically cover mass ranges from 10⁻¹⁸ g to 1 g and are applicable for model specific Sun distance ranges between 0.1 AU and 20 AU Near 1 AU averaged fluxes (over direction and velocities) for all these models are tuned to the well established interplanetary model by Grün et al. However, in many respects these models differ considerably. Examples are the velocity and directional distributions and the assumed meteoroid sources. In this paper flux predictions by the various models to Earth orbiting spacecraft are compared. Main differences are presented and analysed. The persisting differences even for near Earth space can be seen as surprising in view of the numerous ground based (optical and radar) and in situ (captured Inter Stellar Dust Particles, in situ detectors and analysis of retrieved hardware) measurements and simulations.     

Fast rotation of neutron stars and equation of state of dense matter

Fast rotation of compact stars (at sub-millisecond period) and, in particular, their stability, are sensitive to the equation of state (EOS) of dense matter. Recent observations of XTE J1739-285 suggest that it contains a neutron star rotating at 1122 Hz. At such rotational frequency the effects of rotation on star’s structure are significant. We study the interplay of fast rotation, EOS, and gravitational mass of a sub-millisecond pulsar. We discuss the EOS dependence of spin-up to a sub-millisecond period, via mass accretion from a disk in a low-mass X-ray binary.     

济阳坳陷西部惠民凹陷第三纪火山岩型油藏成藏机理研究

在全面剖析济阳坳陷惠民凹陷第三纪火成岩空间分布规律的基础上 ,对本区火山岩的成藏机理进行了深入研究 ,总结了惠民凹陷火山岩型油气藏的成藏模式。惠民凹陷的主要烃源岩来自于南部的临南洼陷和北部的滋镇洼陷 ,由于本区火成岩主要沿 2个生烃凹陷间隆起带的临邑帚状断裂带展布 ,保证了火山岩带有充足的油源条件。油气运移的输导体系是由渗透性砂岩、断层、裂缝和不整合面的三维空间组合 ,研究区的临邑帚状断裂带、多期发育的裂缝和不整合面对油气向火山岩储层的运移至关重要。储集空间是储层质量好坏的决定因素 ,惠民凹陷的火山岩储层存在各种的原生储集空间 ,同时由于次生的断层活动和火成岩拱张作用形成了丰富的次生储集空间 ,极大地改善了本区火成岩的储层物性 ,是本区形成各类火成岩圈闭和油藏的保证。本区火成岩存在 3种类型的油气藏 ,即火成岩作为储层、火成岩作为盖层或遮挡层以及火成岩侵入动力型油气藏