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Cu^+-Na^+离子交换BK7玻璃波导特性研究
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作者 王鹏飞 郑杰 G.C.Ringini 《光子学报》 EI CAS CSCD 北大核心 2002年第0Z2期185-188,共4页
利用Cu^+-Na^+离子交换技术制备了BK7玻璃平面光波导,在632.8nm波长的耦合光下测量了波导的有效折射率,根据反WKB方法确定折射率分布轮廓,近似符合高斯分布。求出了所制备玻璃平面光波导在570℃下,Cu^+-Na^+离子交换过程的扩散系数... 利用Cu^+-Na^+离子交换技术制备了BK7玻璃平面光波导,在632.8nm波长的耦合光下测量了波导的有效折射率,根据反WKB方法确定折射率分布轮廓,近似符合高斯分布。求出了所制备玻璃平面光波导在570℃下,Cu^+-Na^+离子交换过程的扩散系数为Dc≈7.644×10^15m^2/s。 展开更多
关键词 有效折射率 BK7玻璃平面光波导 离子交换 特性 反WKB方法 扩散系数 高斯分布函数
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Diagnostic techniques for photonic materials based on Raman and Brillouin spectroscopies 被引量:11
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作者 M. Mattarelli S.Caponi +11 位作者 A. Chiappini M. Montagna E. Moser F. Rossi C.Tosello C. Armellini A. Chiasera M. Ferrari Y. Jestin G. Nunzi Conti S. Pelli G.C. Righini 《Optoelectronics Letters》 EI 2007年第3期188-191,共4页
The elastic and vibrational properties of a material, bulk or planar waveguide, are studied by BriUouin and Raman spectroscopy to follow the process of nanocrystals growth in glass-ceramics. The nanoparticles cause th... The elastic and vibrational properties of a material, bulk or planar waveguide, are studied by BriUouin and Raman spectroscopy to follow the process of nanocrystals growth in glass-ceramics. The nanoparticles cause the appearance, in the low frequency Raman spectrum, of characteristic peaks, whose position depends on the size of the crystals. At the same time, sharp crystal peaks, due to optical phonons, appear in the Raman spectra, allowing the determination of the nucleated phase, and a frequency shift of the BriUouin peaks is observed. 展开更多
关键词 拉曼光谱 布里渊光谱 光子材料 诊断技术
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Er^(3+)-activated silica inverse opals synthesized by the solgel method 被引量:2
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作者 A. Chiappini C.Armellini +11 位作者 A. Chiasera Y. Jestin M. Ferrari M. Mattarelli M. Montagna E. Moser C. Tosello L. Zampedri G. Nunzi Conti S. Pelli R. M. Almeida G. C. Righini 《Optoelectronics Letters》 EI 2007年第3期184-187,共4页
We present the details of the sol-gel processing used to realize inverse silica opal,where the silica was activated with 0.3 mol% of Er3+ ions. The template(direct opal) was obtained assembling polystyrene spheres of ... We present the details of the sol-gel processing used to realize inverse silica opal,where the silica was activated with 0.3 mol% of Er3+ ions. The template(direct opal) was obtained assembling polystyrene spheres of the dimensions of 260 nm by means of a vertical deposition technique. The Er3+-activated silica inverse opal was obtained infiltrating,into the void of the template,the silica sol doped with Er3+ ions and subsequently removing the polystyrene spheres by means of calcinations. Scanning electron microscope showed that the inverse opals possess a fcc structure with a air hollows of about 210 nm and a photonic band gap,in the visible range,was observed from reflectance measurements. Spectroscopic properties of Er3+-activated silica inverse opal were investigated by luminescence spectroscopy,where,upon excitation at 514.5 nm,an emission of 4I13/2 → 4I15/2 of Er3+ ions transition with a 21 nm bandwidth was observed. Moreover the 4I13/2 level decay curve presents a single-exponential profile,with a measured lifetime of 18 ms,corresponding a high quantum efficiency of the system. 展开更多
关键词 铒掺杂 活性硅 反opal结构 溶胶-凝胶法 合成
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高斯折射率分布Cu^+-Na^+离子交换玻璃波导的制备 被引量:5
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作者 王鹏飞 郑杰 G.C.Righini 《中国激光》 EI CAS CSCD 北大核心 2004年第1期37-40,共4页
利用Cu+ Na+ 离子交换技术制备了玻璃平面光波导 ,在 6 32 8nm波长下 ,用棱镜耦合技术测量出所制备波导的有效折射率 ,利用反WKB方法确定了平面光波导的折射率分布 ,并对折射率分布进行了函数拟合 ,近似符合高斯分布。求出了所制备玻... 利用Cu+ Na+ 离子交换技术制备了玻璃平面光波导 ,在 6 32 8nm波长下 ,用棱镜耦合技术测量出所制备波导的有效折射率 ,利用反WKB方法确定了平面光波导的折射率分布 ,并对折射率分布进行了函数拟合 ,近似符合高斯分布。求出了所制备玻璃平面光波导在 5 80℃的扩散系数为De ≈ 2 2 2 3× 10 -15m2 /s。 展开更多
关键词 光波导 玻璃平面波导 Cu^+-Na^+离子交换 高斯折射率分布
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The HEPD particle detector of the CSES satellite mission for investigating seismo-associated perturbations of the Van Allen belts 被引量:6
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作者 AMBROSI Giovanni BARTOCCI Simona +39 位作者 BASARA Laurent BATTISTON Roberto BURGER William J. CARFORA Luca CASTELLINI Guido CIPOLLONE Piero CONTI Livio CONTIN Andrea DE DONATO Cinzia DE SANTIS Cristian FOLLEGA Francesco M. GUANDALINI Cristina IONICA Maria IUPPA Roberto LAURENTI Giuliano LAZZIZZERA Ignazio LOLLI Mauro MANEA Christian MARCELLI Laura MASCIANTONIO Giuseppe MERGE Matteo OSTERIA Giuseppe PACINI Lorenzo PALMA Francesco PALMONARI Federico PANICO Beatrice PATRIZII Laura PERFETTO Francesco PICOZZA Piergiorgio POZZATO Michele PUEL Matteo RASHEVSKAYA Irina RICCI Ester RICCI Marco RICCIARINI Sergio Bruno SCOTTI Valentina SOTGIU Alessando SPARVOLI Roberta SPATARO Bruno VITALE Vincenzo 《Science China(Technological Sciences)》 SCIE EI CAS CSCD 2018年第5期643-652,共10页
CSES(China Seismo-Electromagnetic Satellite) is a mission developed by CNSA(Chinese National Space Administration) and ASI(Italian Space Agency), to investigate the near-Earth electromagnetic, plasma and particle envi... CSES(China Seismo-Electromagnetic Satellite) is a mission developed by CNSA(Chinese National Space Administration) and ASI(Italian Space Agency), to investigate the near-Earth electromagnetic, plasma and particle environment, for studying the seismo-associated disturbances in the ionosphere-magnetosphere transition zone. The anthropogenic and electromagnetic noise,as well as the natural non-seismic electromagnetic emissions is mainly due to tropospheric activity. In particular, the mission aims to confirming the existence of possible temporal correlations between the occurrence of earthquakes for medium and strong magnitude and the observation in space of electromagnetic perturbations, plasma variations and precipitation of bursts with highenergy charged particles from the inner Van Allen belt. In this framework, the high energy particle detector(HEPD) of the CSES mission has been developed by the Italian LIMADOU Collaboration. HEPD is an advanced detector based on a tower of scintillators and a silicon tracker that provides good energy and angular resolution and a wide angular acceptance, for electrons of 3–100 Me V, protons of 30–200 Me V and light nuclei up to the oxygen. CSES satellite has been launched on February 2^(nd), 2018 from the Jiuquan Satellite Launch Center(China). 展开更多
关键词 earthquake seismic-precursors particle detector Van Allen belts magnetosphere ionosphere space weather cosmic rays
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