Mathematical modeling of heat transfer process in a variable domain

In this paper, a brief review and generalization of studies on the heat transfer and heat conduction problem in a variable domain are presented. The equations of the process, where the boundary displacement velocity is the control, are obtained taking into account heat inflow. This article was submitted by the authors in English.     

SPOT-5卫星系统性能概述

概要介绍SPOT - 5卫星的主要成像传感器 ,精确定位技术及数据格式。介绍分析卫星数据的应用前景     

2K＋1正则图的自由边

本文利用 Tutte 定理,给出并证明了满足一定条件的2k 1正则图中的每个边都是自由边的结论。     

蜀中名士秦天柱

1998年夏天，暑热正浓的日子，我走进好友萧缤在红瓦寺那间有些沧桑的欧式风格的画室，照例是饮点小酒然后挥毫。当时的萧缤正在省诗书画院进修，师从秦天柱。那时我刚从深圳归来不久，对四川的化艺术界并不是太熟悉，第一次见到那般生动空灵的花鸟画，被画面上扑面而来的诗般的意象所打动，时时临写，记忆犹新。后来虽然中断了绘画，仍然很关注先生的作品，时不时在一些报刊和画集中见到那些打动人心灵的画作。遗憾的是一直无缘与这位才华横溢的画家谋面，但其作品自然流露出的恬淡与闲适高雅之气直相伴我走过高原丘陵和平原。     

新型工具电极制造方法

用电火花加工复杂形状模腔的关键之一是工具电极的制造。为了解决一般电极材料价高，复杂型腔难以加工等问题，通过试验研究，推出了一种以石膏和塑料为基本材料，采用非金属电镀工艺制造工具电极的新方法。     

厌氧胶在液体火箭发动机上的应用研究

简要叙述了厌氧胶在航空和汽车制造业方面的使用,指出了厌氧胶具有的优越防松性能,可以成为取代目前仍在使用的传统的保险丝锁紧方式的途径之一,并重点介绍了厌氧胶在液体火箭发动机上的应用试验研究的内容和方法,给出了试验结论,最后提出了厌氧胶在今后液体火箭发动机应用上应重点解决的几个问题。     

ADμC824在温度测控方面的应用

介绍了ADμC824的部分特性及其在精确控温方面的软硬件设计思路。     

ExoMars 2016 Schiaparelli Module Trajectory and Atmospheric Profiles Reconstruction

On 19^th October 2016 Schiaparelli module of the ExoMars 2016 mission flew through the Mars atmosphere. After successful entry and descent under parachute, the module failed the last part of the descent and crashed on the Mars surface. Nevertheless the data transmitted in real-time by Schiaparelli during the entry and descent, together with the entry state vector as initial condition, have been used to reconstruct both the trajectory and the profiles of atmospheric density, pressure and temperature along the traversed path.The available data-set is only a small sub-set of the whole data acquired by Schiaparelli, with a limited data rate (8 kbps) and a large gap during the entry because of the plasma blackout on the communications.This paper presents the work done by the AMELIA (Atmospheric Mars Entry and Landing Investigations and Analysis) team in the exploitation of the available inertial and radar data. First a reference trajectory is derived by direct integration of the inertial measurements and a strategy to overcome the entry data gap is proposed. First-order covariance analysis is used to estimate the uncertainties on all the derived parameters. Then a refined trajectory is computed incorporating the measurements provided by the on-board radar altimeter.The derived trajectory is consistent with the events reported in the telemetry and also with the impact point identified on the high-resolution images of the landing site.Finally, atmospheric profiles are computed tacking into account the aerodynamic properties of the module. Derived profiles result in good agreement with both atmospheric models and available remote sensing observations.     

The Delivery of Water During Terrestrial Planet Formation

The planetary building blocks that formed in the terrestrial planet region were likely very dry, yet water is comparatively abundant on Earth. Here we review the various mechanisms proposed for the origin of water on the terrestrial planets. Various in-situ mechanisms have been suggested, which allow for the incorporation of water into the local planetesimals in the terrestrial planet region or into the planets themselves from local sources, although all of those mechanisms have difficulties. Comets have also been proposed as a source, although there may be problems fitting isotopic constraints, and the delivery efficiency is very low, such that it may be difficult to deliver even a single Earth ocean of water this way. The most promising route for water delivery is the accretion of material from beyond the snow line, similar to carbonaceous chondrites, that is scattered into the terrestrial planet region as the planets are growing. Two main scenarios are discussed in detail. First is the classical scenario in which the giant planets begin roughly in their final locations and the disk of planetesimals and embryos in the terrestrial planet region extends all the way into the outer asteroid belt region. Second is the Grand Tack scenario, where early inward and outward migration of the giant planets implants material from beyond the snow line into the asteroid belt and terrestrial planet region, where it can be accreted by the growing planets. Sufficient water is delivered to the terrestrial planets in both scenarios. While the Grand Tack scenario provides a better fit to most constraints, namely the small mass of Mars, planets may form too fast in the nominal case discussed here. This discrepancy may be reduced as a wider range of initial conditions is explored. Finally, we discuss several more recent models that may have important implications for water delivery to the terrestrial planets.     

含能材料低温松驰WLF方程的两种求值法

通过玻璃化转变温度和表同活化能以及由ＶＦＴ方程导得ＷＬＦ方程粘弹系数的两种新方法,用该方法分别计算１０个体系的粘弹系数,结果表明,用ＤＳＣ技术可以获得ＷＬＦ方程,３种计算方法获得的粘弹系数符合较好。