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朱春春  李征航  屈小川  申小平 《大地测量与地球动力学》2015,35(1):81-86

??RINEX HO???????GPS?????λ?????е???(?????????)????????????????????GPS???????е??????????(ΔI_H)^p,q_i,g??????????(ΔI_H)^p,q_i,g????γ?????????????????????????????????????????????????????￡???Bernese 5.0???????????????????????????????δ???и????????????????????л????????????????????????????????Δb_H???????????Δb_H???????С????????????????????Δ??b??H??????????????????????????????????????????ε??С??Δb_H?????????  相似文献   

3维场景植被冠层多波段模拟研究进展     

张阳  柳钦火  覃文汉  刘强  李静  杜永明  谢东辉  黄华国  杨乐  倪文俭 《遥感学报》2015,19(6):894-909

植被冠层辐射散射信号中蕴含了丰富的植被信息,通过构建植被冠层辐射散射模型,可以实现植被结构等生物物理参数的遥感定量反演。迄今为止,可见光/近红外、热红外、微波波段均已发展了大量的模型,这些模型在参数反演方面各具优势,但不同波段的模型又有其自身的局限性。跨波段的联合模拟可以实现模型间的优势互补,进而提高地表参数的反演精度,近年来已有学者专注于可见光/近红外与热红外模型,热红外与微波模型,主被动微波模型,以及可见光/近红外与微波模型的联合模拟和协同反演,但多是两两联合,且主要是基于经验模型或解析模型。基于3维场景的植被冠层辐射散射特性模拟模型可以细致刻画不同组分的结构和空间分布特征,对于由植被结构引起的多次散射和组分比例变化的考虑具有优势。本文主要介绍了3维模拟模型在可见光/近红外、热红外和微波波段,以及跨波段联合模拟方面的研究进展,从模型机理、场景统一、以及组分理化参数的统一的角度,探讨了构建多波段3维模拟系统的可行性,展望了多波段3维模拟模型的发展趋势。  相似文献   

人体乳腺癌矿化的同步辐射研究     

孟繁露  李源  李艳  王长秋  鲁安怀  梅放 《岩石矿物学杂志》2015,34(6):957-962

同步辐射具有常规光源不可比拟的优良性能,可用于微量生物矿化样品的物相、结构、形貌和成分研究。本文利用基于同步辐射光源的X射线粉末衍射(SR-XRD)、傅立叶变换红外光谱(SR-FTIR)、X射线荧光分析(SR-XRF)和X射线三维成像,对人体乳腺癌矿化进行了表征。研究表明,乳腺癌矿化的主要矿物物相为碳羟磷灰石,含有Sr、Zn等微量元素,其中砂粒体矿化具有独特的分层结构。研究结果为乳腺癌的病理研究和诊断提供了矿物学参考信息。  相似文献   

Scaling-laws of Radio Spike Bursts and Their Constraints on New Solar Radio Telescopestwo     

Tan Bao-lin  Cheng Jun  Tan Cheng-ming  Kou Hong-xiang 《Chinese Astronomy and Astrophysics》2019,43(1):59-74

Radio observation is one of important methods in solar physics and space science. Sometimes, it is almost the sole approach to observe the physical processes such as the acceleration, emission, and propagation of non-thermal energetic particles, etc. So far, more than 100 solar radio telescopes have been built in the world, including solar radiometers, dynamic spectrometers, and radioheliographs. Some of them have been closed after the fulfillment of their primary scientific objectives, or for their malfunctions, and thus replaced by other advanced instruments. At the same time, based on some new technologies and scientific ideas, various kinds of new and much more complicated solar radio telescopes are being constructed by solar radio astronomers and space scientists, such as the American E-OVSA and the solar radio observing system under the framework of Chinese Meridian Project II, etc. When we plan to develop a new solar radio telescope, it is crucial to design the most suitable technical parameters, e.g., the observing frequency range and bandwidth, temporal resolution, frequency resolution, spatial resolution, polarization degree, and dynamic range. Then, how do we select a rational set of these parameters? The long-term observation and study revealed that a large strong solar radio burst is frequently composed of a series of small bursts with different time scales. Among them, the radio spike burst is the smallest one with the shortest lifetime, the narrowest bandwidth, and the smallest source region. Solar radio spikes are considered to be related to a single magnetic energy release process, and can be regarded as an elementary burst in solar flares. It is a basic requirement for the new solar radio telescope to observe and discriminate these solar radio spike bursts, even though the temporal and spatial scales of radio spike bursts actually vary with the observing frequency. This paper presents the scaling laws of the lifetime and bandwidth of solar radio spike bursts with respect to the observing frequency, which provide some constraints for the new solar radio telescopes, and help us to select the rational telescope parameters. Besides, we propose a spectrum-image combination mode as the best observation mode for the next-generation solar radio telescopes with high temporal, spectral, and spatial resolutions, which may have an important significance for revealing the physical essence of the various non-thermal processes in violent solar eruptions.  相似文献   

Three dimensional numerical simulation of residential building on shrink–swell soils in response to climatic conditions          下载免费PDF全文

Xiong Zhang  Jean‐Louis Briaud 《国际地质力学数值与分析法杂志》2015,39(13):1369-1409

Shrink–swell soils can cause distresses in buildings, and every year, the economic loss associated with this problem is huge. This paper presents a comprehensive system for simulating the soil–foundation–building system and its response to daily weather conditions. Weather data include rainfall, solar radiation, air temperature, relative humidity, and wind speed, all of which are readily available from a local weather station or the Internet. These data are used to determine simulation flux boundary conditions. Different methods are proposed to simulate different boundary conditions: bare soil, trees, and vegetation. A coupled hydro‐mechanical stress analysis is used to simulate the volume change of shrink–swell soils due to both mechanical stress and water content variations. Coupled hydro‐mechanical stress‐jointed elements are used to simulate the interaction between the soil and the slab, and general shell elements are used to simulate structural behavior. All the models are combined into one finite element program to predict the entire system's behavior. This paper first described the theory for the simulations. A site in Arlington, Texas, is then selected to demonstrate the application of the proposed system. Simulation results are shown, and a comparison between measured and predicted movements for four footings in Arlington, Texas, over a 2‐year period is presented. Finally, a three‐dimensional simulation is made for a virtual residential building on shrink–swell soils to identify the influence of various factors. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献   

A shift towards wetter and windier conditions in southern Sweden around the prominent solar minimum 2750 cal a BP          下载免费PDF全文

ANETTE MELLSTRÖM  NATHALIE VAN DER PUTTEN  RAIMUND MUSCHELER  RIXT DE JONG  SVANTE BJÖRCK 《第四纪科学杂志》2015,30(3):235-244

  相似文献   

Are peatlands in different states with respect to their thermodynamic behaviour? A simple test of peatland energy and entropy budgets     

Fred Worrall  Ross Morrison  Chris Evans  Joerg Kaduk  Susan Page  Alex Cumming  Mark Rayment  Nicholas Kettridge 《水文研究》2021,35(12):e14431

Whilst all ecosystems must obey the second law of thermodynamics, these physical bounds and controls on ecosystem evolution and development are largely ignored across the ecohydrological literature. To unravel the importance of these underlying restraints on ecosystem form and function, and their power to inform our scientific understanding, we have calculated the entropy budget of a range of peat ecosystems. We hypothesize that less disturbed peatlands are ‘near equilibrium’ with respect to the second law of thermodynamics and thus respond to change by minimizing entropy production. This ‘near equilibrium’ state is best achieved by limiting evaporative losses. Alternatively, peatlands ‘far-from-equilibrium’ respond to a change in energy inputs by maximizing entropy production which is best achieved by increasing evapotranspiration. To test these alternatives this study examined the energy balance time series from seven peatlands across a disturbance gradient. We estimate the entropy budgets for each and determine how a change in net radiation (ΔR_n) was transferred to a change in latent heat flux (ΔλE). The study showed that: (i) The transfer of net radiation to latent heat differed significantly between peatlands. One group transferred up to 64% of the change in net radiation to a change in latent heat flux, while the second transferred as little as 27%. (ii) Sites that transferred the most energy to latent heat flux were those that produced the greatest entropy. The study shows that an ecosystem could be ‘near equilibrium’ rather than ‘far from equilibrium’.  相似文献   

低管电压与低对比剂量在肝脏CT增强中的应用          下载免费PDF全文

岑人丽  黎剑宇  夏亭亭  李靖煦  刘琴  黄晓燕  李林 《CT理论与应用研究》2017,26(3):357-364

目的:探讨低管电压(110kVp)与低对比剂量(1.0mL/kg)在肝脏CT增强扫描中的可行性。方法:116例行肝脏CT增强扫描,且BMI<25kg/m2的患者,随机分成A、B两组进行研究,每组58例。A组:管电压110kVp,对比剂碘帕醇(300mgI/mL),对比剂量(1.0mL/kg),采用正弦迭代重建(SAFIRE)。B组:管电压130kVp,对比剂碘帕醇(300mgI/mL),对比剂量(1.2mL/kg),采用滤波反投影重建算法(FBP)。测量动脉期腹主动脉CT值、肝门脉期门静脉CT值及增强扫描3期(动脉期、门脉期、延迟期)的肝右叶肝实质CT值;计算两组图像的肝动脉期对比噪声比(CNR)、信噪比(SNR)及总有效辐射剂量ED;并对两组图像进行评分,进行统计学分析。结果:A组和B组CNR、SNR差异无统计学意义(P>0.05);两组分别在增强扫描3期测得肝右叶肝实质CT值及动脉期腹主动脉CT值差异亦无统计学意义(P>0.05);肝门脉期A组的门静脉CT值低于B组统计学差异有意义(P<0.05)。A组的3期总有效辐射剂量(ED)(9.88±3.56)mSv低于B组(13.91±4.71)mSv,统计学差异有显著意义(P<0.001);A组比B组的对比剂量减少17%。结论:128层MSCT在肝脏增强CT扫描中,应用低管电压(110kVp)和低对比剂量(1.0mL/kg),联合迭代重建技术(SAFIRE),可以得到较好的图像质量,同时降低辐射剂量及人体碘摄入量。   相似文献   

What SDO tells us about structure and evolution of coronal bright points     

N. V. Karachik  E. Minenko  I. Sattarov  A. A. Pevtsov  C. T. Sherdonov 《Astronomische Nachrichten》2014,335(10):1037-1042

Using magnetograms and coronal images from two instruments on board the Solar Dynamics Observatory (SDO), we study structure and evolution of a limited number of coronal bright points (CBPs). Our results show that the relation between CBPs and their magnetic footpoints is not simple. In some cases, CBP may appear as a bright portion of a larger loop (with clearly identifiable footpoints), and in some cases, an isolated CBP may develop between magnetic poles, which might not be the closest ones to each other or which might not be involved in the magnetic flux cancellation. We suggest that the magnetic connectivity responsible for formation of isolated coronal bright points is governed by the orientation of the large‐scale magnetic field. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Distribution of CMEs with Different Angular Widths and Comparison with the Phase of Sunspot Number in the 23rd Solar Cycle     

MENG Wei-juan  LE Gui-ming  LIN Zhao-xiang  ZHANG Yong  YANG Xing-xing 《Chinese Astronomy and Astrophysics》2014

The variation of the number of coronal mass ejections (CMEs) with different angular widths in the period of 1996-2008 is analyzed statistically in this paper, together with a comparison of the feature of time variation between the number of CMEs with some typical angular widths and the number of sunspots.  相似文献