掺钛蓝宝石激光放大器中放大自发辐射效应研究

给出了描述掺钛蓝宝石激光放大器的速率方程组,通过对放大介质内反转粒子数密度和放大自发辐射的时间和空间特性的数值计算与分析,提出可通过控制泵浦光脉冲和信号光之间的时间延迟来有效地抑制放大自发辐射对放大器增益的影响。     

大口径掺钛蓝宝石晶体放大的实验研究

 分析了口径为80 mm的钛宝石晶体内的增益特性,对大口径钛宝石晶体中的泵浦光能量密度和泵浦光口径进行了优化设计。对于80 mm×17 mm的晶体,最佳工作光束口径为55 mm,泵浦能量为50 J;对于80 mm×30 mm的晶体,最佳工作光束口径为60 mm,泵浦能量为90 J,且其横向小信号增益远小于80 mm×17 mm晶体的。对影响大口径钛宝石晶体放大的横向放大自发辐射（ASE）和寄生振荡采用折射率匹配的包边技术进行了抑制。实验表明,该方法把允许横向增益从13提高到了2 100。实验系统为100 J绿光台面泵浦激光器,100 TW主放大器采用四程空间构型放大光路。80 mm×17 mm钛宝石晶体c轴水平放置,泵浦光和主激光均为水平偏振。当以泵浦光能量为49 J对主放大器进行双端泵浦,注入信号光能量为1.2 J,光束口径60 mm时,获得了14.2 J的放大光输出和286 TW的最高峰值功率。     

大口径掺钛蓝宝石晶体放大的实验研究

分析了口径为80 mm的钛宝石晶体内的增益特性,对大口径钛宝石晶体中的泵浦光能量密度和泵浦光口径进行了优化设计。对于80 mm×17 mm的晶体,最佳工作光束口径为55 mm,泵浦能量为50 J;对于80 mm×30 mm的晶体,最佳工作光束口径为60 mm,泵浦能量为90 J,且其横向小信号增益远小于80 mm×17 mm晶体的。对影响大口径钛宝石晶体放大的横向放大自发辐射（ASE）和寄生振荡采用折射率匹配的包边技术进行了抑制。实验表明,该方法把允许横向增益从13提高到了2 100。实验系统为100 J绿光台面泵浦激光器,100 TW主放大器采用四程空间构型放大光路。80 mm×17 mm钛宝石晶体c轴水平放置,泵浦光和主激光均为水平偏振。当以泵浦光能量为49 J对主放大器进行双端泵浦,注入信号光能量为1.2 J,光束口径60 mm时,获得了14.2 J的放大光输出和286 TW的最高峰值功率。     

准分子激光放大器中的三维放大自发辐射效应

发展了小纵横比条件下、具有圆柱对称性介质的高功能ＫｒＦ准分子激光放大器中，放大自发辐射效应的三维理论模型和计算程序。考虑自发辐射的频率分布效应以及侧壁表面反射效应。结果分析表明，当纵横比及入射负载均较小时，放大自发辐射对输出光束质量有较大的影响。     

高功率激光片状放大器中自发辐射放大研究

采用理论模拟和实验研究相结合的方法,研究了高功率激光片状放大器中的自发辐射放大(ASE)效应。建立了一套较完整的包含空间和时间的3维ASE模型,分析了不同电压、不同储能分布和不同泵浦时刻、不同增益长度积条件下ASE效应对放大器储能效率和小信号增益系数的影响。对4×2×3组合式放大器的计算结果表明：随着泵浦电压升高,ASE效应明显加强;23kV泵浦电压下,ASE效应造成的平均储能下降210%,小信号增益系数损耗为16.62%,增益不均匀性为7.44%;增益长度积可以作为判断ASE效应的依据,其值越大,ASE效应越强。     

高功率激光片状放大器中自发辐射放大研究

 采用理论模拟和实验研究相结合的方法,研究了高功率激光片状放大器中的自发辐射放大(ASE)效应。建立了一套较完整的包含空间和时间的3维ASE模型,分析了不同电压、不同储能分布和不同泵浦时刻、不同增益长度积条件下ASE效应对放大器储能效率和小信号增益系数的影响。对4×2×3组合式放大器的计算结果表明：随着泵浦电压升高,ASE效应明显加强;23kV泵浦电压下,ASE效应造成的平均储能下降210%,小信号增益系数损耗为16.62%,增益不均匀性为7.44%;增益长度积可以作为判断ASE效应的依据,其值越大,ASE效应越强。     

钕玻璃片状激光放大器自发辐射放大特性的研究

编制了一套用蒙特卡罗方法计算钕玻璃片状放大器内自发辐射放大(ASE)的模拟计算程序,考虑了光线在两大表面不同入射角对反射率的影响.计算了包边吸收的ASE能量沿周边的分布,以便于对放大器热畸变特性的研究;以及片的横向尺寸对储能密度的影响.关键词：     

掺钛蓝宝石再生放大器的光谱整形

采用腔内和腔外两种方法对激光脉冲进行光谱整形。在掺钛蓝宝石再生放大器中插入一定厚度的石英双折射晶体片,通过调节晶体光轴的空间取向,对再生放大器输出的脉冲光谱进行腔内整形,使再生放大器输出脉冲的谱宽从20nm左右增加到35nm左右,接近进入再生放大器的激光种子脉冲的谱宽。另外用镀反射膜的平板滤光片进行了腔外光谱整形的实验,使再生放大器输出脉冲谱宽展宽到28nm左右。     

PW级掺钛蓝宝石激光放大器中横向寄生振荡控制

介绍了目前世界上在建的第一台掺钛蓝宝石激光系统中大口径晶体内横向寄生振荡的抑制方法。采用一种掺炭的热塑料MeltMount 1.704作为折射率匹配材料,掺入炭粉作为吸收体。理论上它可以将晶体中的寄生振荡阈值从13增加到2100。     

PW级掺钛蓝宝石激光放大器中横向寄生振荡控制

 介绍了目前世界上在建的第一台掺钛蓝宝石激光系统中大口径晶体内横向寄生振荡的抑制方法。采用一种掺炭的热塑料MeltMount 1.704作为折射率匹配材料,掺入炭粉作为吸收体。理论上它可以将晶体中的寄生振荡阈值从13增加到2100。     

L-band all-optical gain-clamped EDFA by utilizing C-band backward ASE

By using an optical circulator and C/L-band wavelength division multiplexer to recycle the C-band backward ASE, an L-band gain-clamped erbium-doped fiber amplifier is presented. We have experimentally studied the static gain clamping property of this amplifier. As the ASE feedback attenuation is set to 0, the gain at 1585 nm can be clamped at 18.84 ± 0.26 dB within dynamic range of 25 dB and the critical power reaches about −15.09 dBm. The gain variation and saturated output power at 1585 nm for 0 dB attenuation are 1 dB lower and 2.17 dB higher than those for 30 dB attenuation, which indicates that the L-band EDFA gain can be effectively clamped via the ASE injection technique.     

Impact of ASE noise in WDM systems

The small signal analysis method is presented for the discussion of amplified spontaneous emission (ASE) noise in dispersion and nonlinear transmission fibers in wavelength division multiplex (WDM) systems. Based on it, the complete ASE noise spectra (include the ASE noise, the ASE noise enhanced by parametric gain and the crosstalk caused by ASE noise and parametric gain) are described and the factors impacting on them are discussed. The crosstalk caused by ASE noise and parametric gain in single mode fibers, non-zero dispersion shift fibers and dispersion compensation fibers are analyzed. Taking into account the dispersion effect in the transmission fibers, the three types of ASE noise may decrease.     

Suppression of the amplified spontaneous emission in ultraintense and ultrashort lasers by a highly efficient saturable absorber

For ultraintense and ultrashort laser facilities, there are few efficient and reliable methods for suppressing the amplified spontaneous emission (ASE) generated in the last several amplifiers. In the paper, we applied a highly efficient saturable absorber to suppress the ASE. Experiments were carried out to study the absorption property of the saturable absorber and the enhancement of temporal contrast with it in the front-end system of the SILEX-I laser facility with a central wavelength of 800 nm. We also analyzed the effects of the saturable absorber on other laser parameters, such as the spectrum, the spatial beam profile, and energy stability. The results show that the saturable absorber is highly efficient and the transmissivity is as high as 90%. The temporal contrast is improved by more than one order of magnitude. Meanwhile, the saturable absorber has little impact on other parameters. With these advantages, the saturable absorber is an efficient, appropriate and convenient solution to suppressing the ASE generated in the front-end system and also in the last several amplification stages for ultraintense and ultrashort lasers.     

An approach to enhance the receiver sensitivity with SOA for optical communication systems

In this paper, we investigate an SOA (semiconductor optical amplifier) preamplifier structure by optimizing the carrier lifetime in order to reduce the amplified spontaneous emission (ASE) noise and crosstalk, with adequate gain increase. This proposed SOA optical preamplifier has no need of optical alignment and antireflection coating. This structure of SOA eliminates the need of optical filter, and exhibits large tolerance to the input light wavelength. The receiver sensitivity is investigated for single and multi channel transmission links. The received power of − 50.34 dBm is observed at bit error rate (BER) 10^− 12 for 10 Gb/s with PIN receiver. Further, the impact of gain, amplified spontaneous emission power and gain variation for different carrier lifetime with input power for OOK system is illustrated. The proposed SOA has constant gain of 30.06 dB up to gain saturation for carrier lifetime 0.18 ns. It is predicted that low value of carrier lifetime suffers less from ASE noise.     

Gain-clamping in two-stage L-band EDFA using an unwanted backward ase from second stage

A gain clamping technique for the long wavelength band erbium-doped fiber amplifier (L-band EDFA) is presented. It uses two circulators and a broad band fiber Bragg grating to route wasted backward C-band ASE from the second stage and launch it back into the input end of the first stage of a two-stage amplifier. The two-stage L-band EDFA has shown a small signal gain improvement of 5.7 dB compared to a single-stage amplifier with a slight noise figure degradation. By utilizing the wasted backward ASE, a L-band gain-clamped EDFA with high gain can be realized. Compared to the unclamped case, this gain-clamping technique is effective in reducing the total gain variation as small as 0.3 dB.     

Pre-amp EDFA ASE noise minimization for optical receiver transmission performance optimization

Amplified spontaneous emission (ASE) noise mitigation from the pre-amp erbium-doped fiber amplifier (EDFA) to the photon detector (PD) in optical receivers can be reduced by optimizing the EDFA at the optical receiver level to achieve optimal optical receiver transmission performance.     

Simulation of DWDM signals using optimum span scheme with cascaded optimized semiconductor optical amplifiers

We numerically simulated the ten channels at 10 Gb/s dense wavelength division multiplexing (DWDM) transmission faithfully over 17,227 km using 70 km span of single mode fiber (SMF) and dispersion compensating fiber (DCF) using optimum span scheme at channel spacing 20 GHz. For this purpose, inline optimized semiconductor optical amplifiers (SOAs) and DPSK format are used. We optimized the SOA parameters for inline amplifier with minimum crosstalk and amplified spontaneous emission noise with sufficient gain at bias current 400 mA. For this bias current, constant gain 36.5 dB is obtained up to saturation power 21.35 mW. We have also optimized the optical phase modulator bandwidth for 400 mA current which is around 5.5 GHz with crosstalk −14.2 dB between two channels at spacing 20 GHz.We show the 10×10 Gb/s transmission over 70 km distance with inline amplifier has good signal power received as compared to without amplifier, even at equal quality factor. We further investigated the optimum span scheme for 5670 km transmission distance for 10×10 Gb/s with channel spacing 20 at 5.5 GHz optical phase modulator bandwidth. As we increase the transmission distance up to 17,227 km, there is increase in power penalty with reasonable quality.The impact of optical power received and Q factor at 5670 and 17,227 km transmission distance for different span schemes for all channels has been illustrated. For launched optical power less than saturation, all channels are obtained at bit error rate floor of 10⁻¹⁰.     

Suppression of amplified spontaneous emission in a femtosecond chirped-pulse amplifier

The suppression of amplified spontaneous emission (ASE) that arises during the femtosecond chirped-pulse amplification is presented. On the basis of the distinct differences in the spatial, temporal and spectral region between ASE and the amplified laser signal, the noise arising from ASE was effectively filtered out. The ratio between the amplified femtosecond pulse and the ASE peak power was higher than 10⁷. Pulses as short as 38 fs were amplified to peak power of 1.4 TW.