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Kurth WS Gurnett DA Clarke JT Zarka P Desch MD Kaiser ML Cecconi B Lecacheux A Farrell WM Galopeau P Gérard JC Grodent D Prangé R Dougherty MK Crary FJ 《Nature》2005,433(7027):722-725
Saturn is a source of intense kilometre-wavelength radio emissions that are believed to be associated with its polar aurorae, and which provide an important remote diagnostic of its magnetospheric activity. Previous observations implied that the radio emission originated in the polar regions, and indicated a strong correlation with solar wind dynamic pressure. The radio source also appeared to be fixed near local noon and at the latitude of the ultraviolet aurora. There have, however, been no observations relating the radio emissions to detailed auroral structures. Here we report measurements of the radio emissions, which, along with high-resolution images of Saturn's ultraviolet auroral emissions, suggest that although there are differences in the global morphology of the aurorae, Saturn's radio emissions exhibit an Earth-like correspondence between bright auroral features and the radio emissions. This demonstrates the universality of the mechanism that results in emissions near the electron cyclotron frequency narrowly beamed at large angles to the magnetic field. 相似文献
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The use of microring resonators to assist in the evanescent field coupling between dissimilar waveguides is proposed and analyzed. Theoretical analysis based on the coupled mode theory and nu-merical example show that complete cross power transfers can be obtained near the microring resonances. Applications of the device include power dividers, low-power thermo-optic or electro-optic switches, and modulators. 相似文献
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验证彩色多普勒超声对腹壁下动脉穿支血管术前探查的有效性,寻找腹壁下动脉穿支术前优势穿支的选择标准。利用彩色多普勒超声探查腹壁下动脉穿支皮瓣行乳房再造患者52例,重点记录穿支血管穿腹直肌前鞘点的体表投影、口径、血流信息,并通过分析比较以上信息,选择优势穿支。结果52例患者腹壁下动脉穿支穿腹直肌前鞘点于超声下均可显示,平均每侧下腹部3支,距脐平均(5.7±2.09)cm,其中条件适用于显微外科的穿支平均口径(0.95±0.32)cm,血流峰速平均约16.4 cm/s,阻力指数平均0.7。术中优势穿支采用率92.31%。说明高频彩色多普勒超声适用于腹壁下动脉穿支皮瓣术前血管探查,可精确指导穿支的术前选择,辅助手术方案制定以及皮瓣设计。 相似文献
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Laurie CC Laurie CA Rice K Doheny KF Zelnick LR McHugh CP Ling H Hetrick KN Pugh EW Amos C Wei Q Wang LE Lee JE Barnes KC Hansel NN Mathias R Daley D Beaty TH Scott AF Ruczinski I Scharpf RB Bierut LJ Hartz SM Landi MT Freedman ND Goldin LR Ginsburg D Li J Desch KC Strom SS Blot WJ Signorello LB Ingles SA Chanock SJ Berndt SI Le Marchand L Henderson BE Monroe KR Heit JA de Andrade M Armasu SM Regnier C Lowe WL Hayes MG Marazita ML Feingold E Murray JC Melbye M Feenstra B Kang JH Wiggs JL 《Nature genetics》2012,44(6):642-650
We detected clonal mosaicism for large chromosomal anomalies (duplications, deletions and uniparental disomy) using SNP microarray data from over 50,000 subjects recruited for genome-wide association studies. This detection method requires a relatively high frequency of cells with the same abnormal karyotype (>5-10%; presumably of clonal origin) in the presence of normal cells. The frequency of detectable clonal mosaicism in peripheral blood is low (<0.5%) from birth until 50 years of age, after which it rapidly rises to 2-3% in the elderly. Many of the mosaic anomalies are characteristic of those found in hematological cancers and identify common deleted regions with genes previously associated with these cancers. Although only 3% of subjects with detectable clonal mosaicism had any record of hematological cancer before DNA sampling, those without a previous diagnosis have an estimated tenfold higher risk of a subsequent hematological cancer (95% confidence interval = 6-18). 相似文献
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Gurnett DA Kurth WS Hospodarsky GB Persoon AM Zarka P Lecacheux A Bolton SJ Desch MD Farrell WM Kaiser ML Ladreiter HP Rucker HO Galopeau P Louarn P Young DT Pryor WR Dougherty MK 《Nature》2002,415(6875):985-987
Radio emissions from Jupiter provided the first evidence that this giant planet has a strong magnetic field and a large magnetosphere. Jupiter also has polar aurorae, which are similar in many respects to Earth's aurorae. The radio emissions are believed to be generated along the high-latitude magnetic field lines by the same electrons that produce the aurorae, and both the radio emission in the hectometric frequency range and the aurorae vary considerably. The origin of the variability, however, has been poorly understood. Here we report simultaneous observations using the Cassini and Galileo spacecraft of hectometric radio emissions and extreme ultraviolet auroral emissions from Jupiter. Our results show that both of these emissions are triggered by interplanetary shocks propagating outward from the Sun. When such a shock arrives at Jupiter, it seems to cause a major compression and reconfiguration of the magnetosphere, which produces strong electric fields and therefore electron acceleration along the auroral field lines, similar to the processes that occur during geomagnetic storms at the Earth. 相似文献
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Cambon-Thomsen A Thorisson GA Mabile L Andrieu S Bertier G Boeckhout M Cambon-Thomsen A Carpenter J Dagher G Dalgleish R Deschênes M di Donato JH Filocamo M Goldberg M Hewitt R Hofman P Kauffmann F Leitsalu L Lomba I Mabile L Melegh B Metspalu A Miranda L Napolitani F Oestergaard MZ Parodi B Pasterk M Reiche A Rial-Sebbag E Rivalle G Rochaix P Susbielle G Tarasova L Thomsen M Thorisson GA Zawati MH Zins M;BRIF workshop group 《Nature genetics》2011,43(6):503-504
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Based on the sticking point of the low intelligence of the existing management decision system, this paper puts forward the idea of enriching and refining the knowledge of the system and endowing it with the ability to learn by means of adopting three types of heterogeneous knowledge representation and knowledge management measures. At length, this paper outlines the basic framework of an intelligence system for the sake of management decision problem. 相似文献
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Jinghui Li Rui Kang Ali Mosleh Xing Pan .School of Reliability Systems Engineering Beihang University Beijing P.R.China .Center for Risk Reliability University of Maryl College Park MD USA 《系统工程与电子技术(英文版)》2011,(6):1015-1022
This paper presents a methodology for automatically generating risk scenarios for dynamic reliability applications in which some dynamic characteristics(e.g.,the order,timing and magnitude of events,the value of relevant process parameters and initial conditions) have a significant influence on the evolution of the system.The main idea of the methodology is:(i) making the system model "express itself" through simulation by having the model driven by an elaborated simulation engine;(ii) exploiting uniform design to pick out a small subset of representative design points from the space of relevant dynamic characteristics;(iii) for each selected design point,employing a depth-first systematic exploration strategy to cover all possible scenario branches at each branch point.A highly dynamic example adapted from the literature(a chemical batch reactor) is studied to test the effectiveness of the proposed methodology. 相似文献
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