热带气旋各个要素对于海表面降温的影响

热带气旋的经过会引起海洋内部强烈的剪切,由剪切不稳定触发的强混合可以将温跃层的冷水卷挟上来,导致海洋混合层加深和海表面温度的下降。本文利用3-Dimensional Price Weller and Pinkel(3DPWP)模式模拟了不同热带气旋下的海表面降温,分别研究了热带气旋各个要素(气旋的强度,最大风速半径和移动速度)对于海表面降温的影响。模拟结果表明,海表面降温的空间分布主要受到气旋移动速度的影响,移动速度越快的降温,右偏现象越明显。海表面降温的幅度以及降温的区域随着气旋强度和最大风速半径的增大而单调递增,随移动速度增加而单调递减。海表面降温与热带气旋3个要素的拟合结果表明,气旋各个要素对于海表面降温影响作用的大小不同:在气旋移动速度较慢(小于4.5m/s)时,海表面降温主要受到气旋级别和移动速度的影响,在气旋移动速度较快(大于4.5m/s)时,气旋移动速度的影响作用减弱,海表面降温主要受气旋级别的影响。气旋最大风速半径的影响作用始终较小。     

磷灰石裂变径迹在确定造山带隆升速率中的应用

矿物裂变径迹技术是一种低温热史及年代学测定技术,广泛应用于含油气盆地热史分析、沉积物来源、造山带隆升剥蚀、地质年代学测定等方面的研究。近年来,磷灰石裂变径迹在研究造山带构造隆升速率方面取得了大量成果。笔者在结合前人研究成果基础上,分别介绍了利用裂变径迹反演热史、裂变年龄和矿物对-封闭温度法确定构造隆升速率的原理、方法和应用,并分析其优缺点,指出应用磷灰石裂变径迹研究构造隆升速率时应该注意的问题。     

Garnet-biotite diffusion mechanisms in complex high-grade orogenic belts: Understanding and constraining petrological cooling rates in granulites from Ribeira Fold Belt (SE Brazil)

Cooling rates based on the retrograde diffusion of Fe²⁺ and Mg between garnet and biotite inclusions commonly show two contrasting scenarios: a) narrow closure temperature range with apparent absence of retrograde diffusion; or b) high result dispersion due to compositional variations in garnet and biotite. Cooling rates from migmatites, felsic and mafic granulites from Ribeira Fold Belt (SE Brazil) also show these two scenarios. Although the former can be explained by very fast cooling, the latter is often the result of open-system behaviour caused by deformation. Retrogressive cooling during the exhumation of granulite-facies rocks is often processed by thrusting and shearing which may cause plastic deformation, fractures and cracks in the garnet megablasts, allowing chemical diffusion outside the garnet megablast – biotite inclusion system.However, a careful use of garnets and biotites with large Fe/Mg variation and software that reduces result dispersion provides a good correlation between closure temperatures and the size of biotite inclusions which are mostly due to diffusion and compositional readjustment to thermal evolution during retrogression.Results show that felsic and mafic granulites have low cooling rates (1–2 °C/Ma) at higher temperatures and high cooling rates (∼100 °C/Ma) at lower temperatures, suggesting a two-step cooling/exhumation process, whereas migmatites show a small decrease in cooling rates during cooling (from 2.0 to 0.5 °C/Ma). These results agree with previously obtained thermochronological data, which indicates that this method is a valid tool to obtain meaningful petrological cooling rates in complex high-grade orogenic belts, such as the Ribeira Fold Belt.     

郯庐断裂带(安徽段)内磁铁石榴角闪岩的形成条件、年代学及构造归属的探究

通过对肥东群南缘特征性岩石——磁铁石榴角闪岩的构造地质学和岩相学研究表明,磁铁石榴角闪岩及其围岩以构造透镜体形式产出,该变质岩具有两个阶段变质矿物组合,热力学评价显示①阶段的温压范围为：T=616~700℃和P=0.66~0.85GPa,平均温压为T=653±35℃和P=0.75±0.09GPa。②阶段的温压范围为：T=597~643℃和P=0.51~0.94GPa,平均温压为T=620±15℃和P=0.73±0.15GPa,并表现出一个快速等压降温P-T演化特征。锆石U-Pb定年和拉曼光谱分析表明,该磁铁石榴角闪岩的变质年龄为2469±49Ma。结合地质背景和前人的研究,可以判定该类岩石可能源于华北板块。由于郯庐断裂的左旋走滑作用被构造并置与扬子板块中。从而进一步推测,郯庐断裂（安徽段）横向宽度可达到10~15km。     

冻土区天然气水合物钻井泥浆冷却系统设计及关键参数计算

泥浆冷却技术是天然气水合物钻探的关键技术之一,低温泥浆可以抑制天然气水合物在钻进和提钻过程中分解,有利于钻获水合物实物样品。新型天然气水合物钻井泥浆冷却系统主要包括载冷剂制冷器、翅片管式换热器、温度监测与记录和防冻装置4部分。制冷机组采用变频启动,减小了野外施工中配套发电机的功率,大幅度降低油料消耗;翅片管式换热器中泥浆与载冷剂对流换热,换热面积大,换热效率高;温度监测与记录装置对4个关键节点的温度进行监测和记录,同时防冻装置可防止泥浆在换热器中结冰堵塞,影响正常使用。运用传热学和流体力学理论对泥浆与载冷剂对流换热过程进行计算,在满足制冷要求的前提下,换热器换热面积是10.58 m2,管路压力损失为0.34 MPa。     

The relationship between apparent equilibrium temperature and closure temperature with application to oxygen isotope geospeedometry

Oxygen isotope fractionation between coexisting minerals in slowly cooled rocks conveys information about their cooling history. By using the fast grain boundary （FGB） model to simulate closed-system diffusive ex- change of oxygen isotopes between coexisting minerals, I show that the apparent equilibrium temperatures （Tae） by the mineral pair with the largest isotopic fractionation （PLIF） always lies between the closure temperatures （To） of those two minerals. Therefore, when the rate of oxygen diffusion and hence Tc for the PLIF chance to be comparable （such as in the case of quartz and magnetite）, Tae will serve as a good approximation of To regardless of variation in mineral proportions. The specialty of the PLIF in constraining Tac within their Tc range can be generalized to other stable isotope systems and element partitioning. By approximating Tc with Tac and inverting Dodson＇s equation, the cooling rate of plutonic or metamorphic rocks can be inferred.     

全新世温度研究回顾及对历史人地关系的启示

最新一些研究结果强调了全新世期间的长期增温趋势,综合全球平均海平面、大陆冰盖面积、大气温室气体和太阳辐射证据来看,这比传统观点所认为的全新世期间的长期降温趋势,更具有合理性。回顾历史,结合最新的一些研究进展,发现支持“中全新世大暖期”和“晚全新世降温趋势”的证据存在明显的不确定性,最核心的问题为晚全新世加强的人类活动对代用指标或者证据的强烈扰动,使得其不能准确地反映真实的气候变化过程。鉴于目前全新世温度历史争论的核心关键在于晚全新世,因此有必要加强晚全新世温度变化研究。在人类活动影响较小的地区,或者利用对人类活动不敏感的代用指标开展研究,有望可以获得更可靠的晚全新世温度历史重建结果,为准确认识中华数千年文明的长期温度变化背景,进而理解期间的“人地关系”演化历史,并最终客观认识现今面临的以全球变暖为主要特征的气候环境问题,提供一定的科学基础。     

制冷控制系统研制与探析

根据实际应用研制制冷控制系统,该系统采用温度测量、PID控制及PWM脉宽调制等技术实现了对目标对象的制冷处理,具有一定的应用价值。     

The effect of Newtonian cooling on vertically propagating magneto-acoustic waves in a thermally conducting isothermal atmosphere (II)

In this article, we examine reflection, dissipation and attenuation of vertically propagating waves in an isothermal atmosphere under the combined effect of Newtonian cooling, thermal conduction and viscosity with a weak horizontal magnetic field. We consider the case in which the combined effect of viscosity and magnetic field is dominated by that of the thermal conduction and for small values of the Newtonian parameter. As a result, the atmosphere can be divided into three distinct regions that are connected by two transition regions. The lower and middle regions are connected by a semi-transparent barrier and the middle and upper regions are connected by an absorbing and reflecting barrier. In the connecting barriers the reflection and transmission of the waves takes place. The presence of Newtonian cooling effects on the adiabatic region, produces attenuation in the amplitudes of the waves and reduces the energy absorption in the transition regions. The reflection coefficient is determined in the lower and middle regions and the results are discussed in the context of the heating of the solar atmosphere.     

The shielding effect of small-scale martian surface geometry on ultraviolet flux

The atmosphere of Mars does little to attenuate incoming ultraviolet (UV) radiation. Large amounts of UV radiation sterilize the hardiest of terrestrial organisms within minutes, and chemically alter the soil such that organic molecules at or near the surface are rapidly destroyed. Thus the survival of any putative martian life near the surface depends to a large extent on how much UV radiation it receives. Variations in small-scale geometry of the surface such as pits, trenches, flat faces and overhangs can have a significant effect on the incident UV flux and may create “safe havens” for organisms and organic molecules. In order to examine this effect, a 1-D radiative transfer sky model with 836 meshed points (plus the Sun) was developed which includes both diffuse and direct components of the surface irradiance. This model derives the variation of UV flux with latitude and an object's Geometric Shielding Ratio (a ratio which describes the geometry of each situation). The best protection is offered by overhangs with flux reduced to a factor of 1.8±0.2×10⁻⁵ of the unprotected value, a reduction which does not vary significantly by latitude. Pits and cracks are less effective with a reduction in UV flux of only up to 4.5±0.5×10⁻³ for the modeled scenarios; however, they are more effective for the same geometric shielding ratio than overhangs at high latitudes due to the low height of the Sun in the sky. Lastly, polar faces of rocks have the least effective shielding geometry with at most a 1.1±0.1×10⁻¹ reduction in UV flux. Polar faces of rocks are most effective at mid latitudes where the Sun is never directly overhead, as at tropical latitudes, and never exposes the back of the rock, as at polar latitudes. In the most favorable cases, UV flux is sufficiently reduced such that organic in-fall could accumulate beneath overhanging surfaces and in pits and cracks. As well, hardy terrestrial microorganisms such as Bacillus pumilus could persist for up to 100 sols on the outer surfaces of typical spacecraft or several tens of martian years in the most shielded surface niches.