一种采用解析积分的直线单元的边界元法

本文提出一种采用解析的直线单元计算受有离心力的二维问题的边界元法,推导了相应直线单元的积分解析式。算例表明,本文方法能获得较高的数值精度,尤其在计算靠近边界的内点应力时,效果更好。     

行星着陆探测中的动力学与控制研究进展

着陆探测是获取行星特性和科学数据最直接、最有效的途径,也是目前技术难度最大、最为复杂的探测方式。在行星着陆探测过程中,动力学与控制是影响任务成败的关键因素之一。文章首先分析了行星着陆探测动力学与控制研究所面临的挑战与难题;然后,针对火星和小行星的着陆探测,重点分析了火星着陆进入段和下降段所涉及的动力学与控制,小行星附着探测动力学建模与制导控制的研究现状与关键问题;最后,提出了我国在行星着陆探测动力学与控制领域的未来重点发展方向。     

制样压应力对显微拉曼光谱法获取碳材料结构参数的影响

为了研究金相制样过程中压应力对获取碳材料拉曼特征参数R的影响,对不同温度处理的碳纤维和树脂碳进行了研究.结果表明,制样过程中的压应力对准确获取碳材料的拉曼特征参数具有一定的影响,尤其是对经过高温处理硬度较小的碳材料的影响更大,造成了碳材料R的增大.建议在制备碳材料的显微拉曼光谱测试试样时采用较小的压应力.     

更多测试 更多安全

<正>Agilent U1250系列数字手持式数字万用表的强大功能特性和性能指标超过了客户的预期,能满足客户最苛刻的测量要求和应用需要。     

Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares

High-energy X-rays and ??-rays from solar flares were discovered just over fifty years ago. Since that time, the standard for the interpretation of spatially integrated flare X-ray spectra at energies above several tens of keV has been the collisional thick-target model. After the launch of the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) in early 2002, X-ray spectra and images have been of sufficient quality to allow a greater focus on the energetic electrons responsible for the X-ray emission, including their origin and their interactions with the flare plasma and magnetic field. The result has been new insights into the flaring process, as well as more quantitative models for both electron acceleration and propagation, and for the flare environment with which the electrons interact. In this article we review our current understanding of electron acceleration, energy loss, and propagation in flares. Implications of these new results for the collisional thick-target model, for general flare models, and for future flare studies are discussed.     

Characterization and Calibration of the CheMin Mineralogical Instrument on Mars Science Laboratory

A principal goal of the Mars Science Laboratory (MSL) rover Curiosity is to identify and characterize past habitable environments on Mars. Determination of the mineralogical and chemical composition of Martian rocks and soils constrains their formation and alteration pathways, providing information on climate and habitability through time. The CheMin X-ray diffraction (XRD) and X-ray fluorescence (XRF) instrument on MSL will return accurate mineralogical identifications and quantitative phase abundances for scooped soil samples and drilled rock powders collected at Gale Crater during Curiosity’s 1-Mars-year nominal mission. The instrument has a Co X-ray source and a cooled charge-coupled device (CCD) detector arranged in transmission geometry with the sample. CheMin’s angular range of 5^° to 50^° 2θ with <0.35^° 2θ resolution is sufficient to identify and quantify virtually all minerals. CheMin’s XRF requirement was descoped for technical and budgetary reasons. However, X-ray energy discrimination is still required to separate Co?Kα from Co?Kβ and Fe?Kα photons. The X-ray energy-dispersive histograms (EDH) returned along with XRD for instrument evaluation should be useful in identifying elements Z>13 that are contained in the sample. The CheMin XRD is equipped with internal chemical and mineralogical standards and 27 reusable sample cells with either Mylar^? or Kapton^? windows to accommodate acidic-to-basic environmental conditions. The CheMin flight model (FM) instrument will be calibrated utilizing analyses of common samples against a demonstration-model (DM) instrument and CheMin-like laboratory instruments. The samples include phyllosilicate and sulfate minerals that are expected at Gale crater on the basis of remote sensing observations.     

A Twin-CME Scenario for Ground Level Enhancement Events

Ground Level Enhancement (GLEs) events are extreme Solar Energetic Particle (SEP) events. Protons in these events often reach ～GeV/nucleon. Understanding the underlying particle acceleration mechanism in these events is a major goal for Space Weather studies. In Solar Cycle 23, a total of 16 GLEs have been identified. Most of them have preceding CMEs and in-situ energetic particle observations show some of them are enhanced in ICME or flare-like material. Motivated by this observation, we discuss here a scenario in which two CMEs erupt in sequence during a short period of time from the same Active Region (AR) with a pseudo-streamer-like pre-eruption magnetic field configuration. The first CME is narrower and slower and the second CME is wider and faster. We show that the magnetic field configuration in our proposed scenario can lead to magnetic reconnection between the open and closed field lines that drape and enclose the first CME and its driven shock. The combined effect of the presence of the first shock and the existence of the open close reconnection is that when the second CME erupts and drives a second shock, one finds both an excess of seed population and an enhanced turbulence level at the front of the second shock than the case of a single CME-driven shock. Therefore, a more efficient particle acceleration will occur. The implications of our proposed scenario are discussed.