基于DTU的加速度强振动记录终端的设计     

吴林斌  陈志高  关伟智  吕瀚  李家明  吴雄伟 《大地测量与地球动力学》2011,31(Z1):155-156,164

设计基于DTU的强振记录终端,采用SOC系列C8051F015型单片机对MEMS加速度计的输出信号进行A/D转换,监测待测体所经受的强振加速度值,并通过DTU内嵌的GPRS无线网络通讯方式将数据发送到远程数据中心.该系统具有体积小,安装与操作方便,免维护等特性.  相似文献   

《震灾防御技术》第6卷(2011年)总目录     

《震灾防御技术》2011,6(4):478-480

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应用WS/GPS技术的粪渣收运监控系统的开发     

钟波 《地理空间信息》2011,(6):45-46,54

通过安装于粪渣收运车辆上的车载称重系统（WS）和全球卫星定位系统（GPS）,经由通用无线分组业务（GPRS）将粪渣收运车载重变化及其位置信息,实时传回监控中心的数据库中[1],并通过集成地理信息系统（GIS）的粪渣收运监控系统浏览、查询、管理粪渣收运情况。主要以车载重量变化信息作为收运监控参考的重要依据,并配合车辆定位...  相似文献   

Upper Ocean Four-Dimensional Variational Data Assimilation in the Arabian Sea and Bay of Bengal     

Suneet Dwivedi  Atul Srivastava  Alok Kumar Mishra 《Marine Geodesy》2018,41(3):230-257

A regional ocean circulation model with four-dimensional variational data assimilation scheme is configured to study the ocean state of the Indian Ocean region (65°E–95°E; 5°N–20°N) covering the Arabian Sea (AS) and Bay of Bengal (BoB). The state estimation setup uses 10 km horizontal resolution and 5 m vertical resolution in the upper ocean. The in-situ temperature and salinity, satellite-derived observations of sea surface height, and blended (in-situ and satellite-derived) observations of sea surface temperature alongwith their associated uncertainties are used for data assimilation with the regionally configured ocean model. The ocean state estimation is carried out for 61 days (1 June to 31 July 2013). The assimilated fields are closer to observations compared to other global state estimates. The mixed layer depth (MLD) of the region shows deepening during the period of assimilation with AS showing higher MLD compared to the BoB. An empirical forecast equation is derived for the prediction of MLD using the air–sea forcing variables as predictors. The surface and sub-surface (50 m) heat and salt budget tendencies of the region are also investigated. It is found that at the sub-surface, only the advection and diffusion temperature and salt tendencies are important.  相似文献   

The Cherenkov Telescope Array potential for the study of young supernova remnants     

《Astroparticle Physics》2015

Supernova remnants (SNRs) are among the most important targets for γ-ray observatories. Being prominent non-thermal sources, they are very likely responsible for the acceleration of the bulk of Galactic cosmic rays (CRs). To firmly establish the SNR paradigm for the origin of cosmic rays, it should be confirmed that protons are indeed accelerated in, and released from, SNRs with the appropriate flux and spectrum. This can be done by detailed theoretical models which account for microphysics of acceleration and various radiation processes of hadrons and leptons. The current generation of Cherenkov telescopes has insufficient sensitivity to constrain theoretical models. A new facility, the Cherenkov Telescope Array (CTA), will have superior capabilities and may finally resolve this long standing issue of high-energy astrophysics. We want to assess the capabilities of CTA to reveal the physics of various types of SNRs in the initial 2000 years of their evolution. During this time, the efficiency to accelerate cosmic rays is highest. We perform time-dependent simulations of the hydrodynamics, the magnetic fields, the cosmic-ray acceleration, and the non-thermal emission for type Ia, Ic and IIP SNRs. We calculate the CTA response to the γ-ray emission from these SNRs for various ages and distances, and we perform a realistic analysis of the simulated data. We derive distance limits for the detectability and resolvability of these SNR types at several ages. We test the ability of CTA to reconstruct their morphological and spectral parameters as a function of their distance. Finally, we estimate how well CTA data will constrain the theoretical models.  相似文献   

地质工程专业普通地质认识实习教学的思考     

许宝田  张勇  王博  杨爱华  解国爱 《高校地质学报》2022,28(3):382-386

文章针对地质工程专业中基础地质学的重要性和普地实习野外教学实际,提出在普地实习中融入地质工程专业知识教学内容。从岩石基本地质特征、力学问题和具体工程地质问题3个方面将基础地质学与地质工程专业知识进行融合、交叉。从而拓展学生视野,实现实习模式创新、内容改革,促进学生学习意识和自主学习的发展,提升专业思维。岩石成分与岩石力学性质、风化特征和水软化性关系密切,节理面的粗糙、起伏和充填物成分影响节理面抗剪、透水等特性,具体工程中的“滑坡”问题是典型的岩体剪切破坏问题,其形成的力学机制与剪节理相同。将上述问题两者联系起来的讲解丰富了普地实习的内容。文章认为普地实习中观察到的现象与地质工程专业课程中很多知识点紧密联系,在基础地质实习教学中融入上述地质工程的专业知识是完全可行性的,采取增加与地质工程专业结合的实践教学环节的办法,既扩大了学生知识面,初步提高学生专业素养,也为实现毕业后成为专业领域合格工程师和科研人员的培养目标迈出重要的第一步。  相似文献   

ISA accelerometer onboard the Mercury Planetary Orbiter: error budget     

Valerio Iafolla  David M. Lucchesi  Sergio Nozzoli  Francesco Santoli 《Celestial Mechanics and Dynamical Astronomy》2007,97(3):165-187

We have estimated a preliminary error budget for the Italian Spring Accelerometer (ISA) that will be allocated onboard the Mercury Planetary Orbiter (MPO) of the European Space Agency (ESA) space mission to Mercury named BepiColombo. The role of the accelerometer is to remove from the list of unknowns the non-gravitational accelerations that perturb the gravitational trajectory followed by the MPO in the strong radiation environment that characterises the orbit of Mercury around the Sun. Such a role is of fundamental importance in the context of the very ambitious goals of the Radio Science Experiments (RSE) of the BepiColombo mission. We have subdivided the errors on the accelerometer measurements into two main families: (i) the pseudo-sinusoidal errors and (ii) the random errors. The former are characterised by a periodic behaviour with the frequency of the satellite mean anomaly and its higher order harmonic components, i.e., they are deterministic errors. The latter are characterised by an unknown frequency distribution and we assumed for them a noise-like spectrum, i.e., they are stochastic errors. Among the pseudo-sinusoidal errors, the main contribution is due to the effects of the gravity gradients and the inertial forces, while among the random-like errors the main disturbing effect is due to the MPO centre-of-mass displacements produced by the onboard High Gain Antenna (HGA) movements and by the fuel consumption and sloshing. Very subtle to be considered are also the random errors produced by the MPO attitude corrections necessary to guarantee the nadir pointing of the spacecraft. We have therefore formulated the ISA error budget and the requirements for the satellite in order to guarantee an orbit reconstruction for the MPO spacecraft with an along-track accuracy of about 1 m over the orbital period of the satellite around Mercury in such a way to satisfy the RSE requirements.  相似文献   

Sustaining marine life beyond boundaries: Options for an implementing agreement for marine biodiversity beyond national jurisdiction under the United Nations Convention on the Law of the Sea     

《Marine Policy》2014

For nearly a decade, governments have been discussing the need to improve efforts to conserve and sustainably use marine biodiversity in areas beyond national jurisdiction (ABNJ). Support for a new international agreement under the United Nations Convention on the Law of the Sea (UNCLOS) – an Implementing Agreement – on the conservation and sustainable use of marine biodiversity in ABNJ has been growing. In June 2012, at the United Nations Conference on Sustainable Development held in Rio de Janeiro, Brazil, States agreed to take a decision on the development of an international instrument under UNCLOS before the end of the 69th session of the United Nations General Assembly (UNGA), which runs from September 2014 to August 2015. In follow-up to this commitment, it was agreed to consider the “scope, parameters and feasibility” of this instrument. To inform these international discussions, this article highlights some potential options for the content of a new UNCLOS Implementing Agreement. It first reviews the history of UN discussions, and then elaborates on options to address key elements identified as priorities for States in 2011: marine genetic resources, including the sharing of benefits, area-based management tools, including marine protected areas, environmental impact assessments, capacity-building and the transfer of marine technology. It addresses cross-cutting issues such as the governing principles, institutional structure as well as on other critical points such as High Seas fishing and flag State responsibilities. The article concludes with suggestions on possible next steps in order to succeed in the negotiations for an agreement.  相似文献   

Cosmological Constant, Minimal Mass and Electroweak Interaction     

Corrado Massa 《Astrophysics and Space Science》2006,306(3):175-176

A lower bound for the mass of a rotating body is derived in the general relativity theory with positive cosmological term Λ. The bound suggests a neutrino rest mass ∼1 meV and a neutrino magnetic moment of 10⁻⁴¹ erg/gauss ∼ Planck's magnetic moment. A connection between gravity and electroweak interaction is suggested.  相似文献   

The Momentum 4-Vector Imparted by Gravitational Waves in Bianchi-Type Metrics     

Ali Havare  Murat Korunur  Mustafa Salti 《Astrophysics and Space Science》2006,301(1-4):43-46

Considering the Møller, Weinberg and Qadir-Sharif's definitions in general relativity, we find the momentum 4-vector of the closed universe based on the Bianchi-type metrics. The momentum 4-vector (due to matter plus fields) is found to be zero. This result supports the viewpoints of Albrow and Tryon and extends the previous works by Cooperstock–Israelit, Rosen, Johri et al., Banerjee–Sen and Vargas who investigated the problem of the energy in Friedmann–Robertson–Walker universe and Salt?-Havare who studied the problem of the energy-momentum of the viscous Kasner-type space-times.  相似文献