手持/便携拉曼光谱仪 532/785/1064 nm
高分辨率光纤光谱仪(200nm-1100nm)
背照式高灵敏紫外光谱仪(200nm-1100nm)
背照式制冷高灵敏光谱仪(200nm-1100nm)
大型数值孔径高灵敏度光谱仪(200-1450nm)
高通量近红外光谱仪(900-2500nm)
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SIMSCOP单点共聚焦显微镜
SIMSCOP线扫共聚焦显微镜
SIMSCOP转盘共聚焦显微镜
SIMSCOP结构光SIM显微镜
SIMSCOP宽场拉曼显微镜
多线连续单模激光器
用于SPAD(APD)测试的TCSPC系统
无掩膜紫外光刻机
多点激光多普勒测振仪 0.1Hz to 5Mhz
OCT成像系统
新品上线
X-ray/XRD 冷热台
光学冷热台
电探针温度台
可调电探针台
拉伸应变温度台
光纤光谱仪 (200nm to 5um)
手持/便携拉曼光谱仪 532/785/1064nm
X射线/极紫外光谱仪 (1-300nm)
高光谱相机 (220nm-4.2μm)
多光谱相机 (400-1000nm)
分光光度计(240-2150nm)
光电倍增管 (PMTs)
可见光单光子探测器(SPD)
红外单光子探测器(SPD)
光电二极管PD(200nm-12um)
热电红外探测器(2-12um)
光电探测器模块
红外光束分析仪(2-16um)
太赫兹光束分析仪(3-20 THz)
扫描狭缝光束轮廓仪(190-2500nm)
光功率计探测器 250-2500nm
功率计控制台
光功率计积分球
电力仪表适配器及附件
VUV/UV摄谱仪
1/8m 单色仪/光谱仪
1/2m &1/4m 单色仪/摄谱仪
单色仪配件
过滤器&滤光片轮
LIV测试系统(LD/LED)
激光多普勒测振仪 0.1Hz to 5Mhz
白光干涉仪
光学镀膜CRD反射计
光学测试测量系统
射频测试测量系统
连续尾纤激光二极管(400-1920nm)
连续激光二极管模块 (375-785nm)
连续多波长激光器
DPSS纳秒脉冲激光器
DFB/FP皮秒激光器(370-1550nm)
高功率飞秒固体激光器
纳秒脉冲光纤激光器(1064-2um)
皮秒脉冲光纤激光器 (515nm - 2um)
飞秒脉冲光纤激光器 780nm-2um
CW光纤激光系统(405nm-2um)
连续窄线宽激光器(1530nm-2um)
C波段可调谐激光器(1529 -1567nm)
L波段可调谐激光器(1554 -1607nm)
超级连续光谱光纤激光器(450-2300nm)
飞秒激光放大器 (650 - 2600nm)
短脉冲OPA(650-2600nm)
宽带飞秒激光器(950-1150nm)
掺铒光纤放大器
掺镱光纤放大器
掺铊光纤放大器
光纤拉曼放大器
半导体光放大器 (SOA)
真空紫外光源
紫外光源
显微镜光源(185-5500nm)
单波长LED光源(240-980nm)
中红外光源
多波长LED光源(240-980nm)
光场合成器
中空纤维压缩机
大功率空心光纤压缩机
超高对比度三阶自相关器
相干超宽带XUV光源
用于激光的增强型腔
太赫兹量子级联激光器(1-4.5Thz)
连续红外量子级联激光(3-12um)
连续长波红外量子级联激光(10-17um)
全自动荧光显微镜
SIMSCOP宽场共焦拉曼显微镜
SIMSCOP科研线扫共聚焦显微镜L系列
宽带手持式共聚拉曼皮肤分析仪
荧光正置/倒置显微镜
生物正/倒置显微镜
相差正置显微镜
暗视野正置显微镜
偏光正置显微镜
金相正置/倒置显微镜
智能三维体视显微镜
USB数字显微镜-带平台
内置数码显微镜
测量仪
金相显微镜
光学测量仪
平场复消色差物镜
工业计划物镜
生物计划物镜
显微镜CCD相机(VIS-NIR)
显微镜 CMOS 摄像头(紫外一近红外)
UV&NIR 增强型CMOS相机
用于显微镜的高光谱相机
用于显微镜的多光谱相机
显微镜光源
软X射线 BSI SCMOS摄像头(80-1000eV)
UV-NIR sCMOS 相机(200-1100nm)
增强型CMOS相机(200-1100nm)
激光增强管
全帧CCD相机(UV VUS NIR)
全帧CCD相机(VUV EUV X-ray)
全画幅真空CCD相机
大幅面真空CCD相机
显微镜CMOS摄像头(紫外一近红外)
UV&NIR增强型CMOS相机
高清晰度多媒体彩色CMOS摄像头(显示器)
高速线扫描摄像机
大幅面摄像机
高速大幅面摄像机
帧抓取器
热释电红外探测器(2-12um)
红外高温计(-40-3000C)
红外线阵列相机
红外线面振相机
黑体校准源 -15 to 1500°C
短波红外摄像机(SWIR)
中波红外摄像机(MWIR)
长波红外摄像机(LWIR)
自由空间声光调制器(AOM)
光纤耦合声光调制器
声光可调滤波器 (AOTF)
声光Q开关 (AOQ)
声光频移 (AOFS)
相位调制器
用于TCSPC的超快脉冲发生器
单光子时间计数器
ID1000定时控制器
电光强度调制器
电光相位调制器
通用脉冲发生器
中高压脉冲发生器
高速脉冲发生器
超高速脉冲发生器
函数发生器
脉冲放大器
脉冲电压
脉冲电流
相位型空间光调制器
振幅型空间光调制器
数字微镜空间光调制器
TPX/HDPE太赫兹平面凸透镜
离轴抛物面反射镜
太赫兹空心逆向反射器
太赫兹金属反射镜
ZnTe/GaSe太赫兹晶体
太赫兹扩束反射
波片
光隔离器
光学偏振片
光束挡板
分束器立方体
二向色分束器
超薄光束挡板
带通滤波器
拉曼光谱滤波器
激光窄滤波器
FISH过滤器
TIRF显微镜过滤器
FRET显微镜过滤器
激光晶体
非线性光学晶体
双折射晶体
光学晶体
电光晶体
微通道板(MCP)
微通道板组件(MCP)
光纤板(FOP)
微孔光学
X射线准直器
混合纤维组件
电动可调光纤延迟线
手动可调光纤延迟线
光学循环器
滤波器耦合器
FA透镜
变焦镜头
电控探针冷热台
外部调节探针冷热台
原位拉伸冷热台
XRD/SEM 原位冷热台
单轴电动压电载物台
XY电动压电载物台
多轴电动压电载物台
XY显微镜压电载物台
真空无磁压电动台
纳米电动执行器
透镜支架
镜架
过滤器支架
13mm 线性位移台
25mm 线性位移台
旋转和倾斜台
齿条和小齿轮级
垂直轴台
2轴台
固体隔振光学台
固体隔振台
气动光学台
带摆杆的气动光学台
蜂窝式光学电路板
Simtrum's high-power Faraday Rotator (780-1080nm, up to 20W), offering low insertion loss, high return loss, excellent reliability, and stability. It's used in fiber optic instruments, sensors, lasers, and coherent detecting. Key features include multiple center wavelength options, specified maximum power handling, and operation within a broad temperature range. The device ensures precision with low polarization mode dispersion and high extinction ratio.
Features
Applications
Specifications
Parameters
Unit
Value
Center Wavelength
nm
1064, 1030, 980, 850, 808, 780
Operating Wavelength Width
±5
Max. Insertion Loss at 23 ℃
dB
1.0
Faraday Rotation Angle for CWL
deg
45
Max. Rotation Angle Tolerance at 23 ℃ for CWL
±2
Min. Extinction Ratio at 23 ℃ (PM Fiber Type)
20
Max. Polarization Dependent Loss at 23 ℃ (SM Fiber Type)
0.15
Max. Polarization Mode Dispersion
ps
0.05
Max. Power Handling (CW)
W
0.5, 1, 5, 10, 20 or Specified
Max. Peak Power for ns Pulse
kW
10 or Specified
Package Dimension
mm
64x28x26
Max. Tensile Load
N
5
Axis Alignment
-
Both axis working
Operating Temperature
℃
-5~+70
Storage Temperature
-40~+85
With connectors, the Max. handling power is 1W only, IL is 0.3dB higher, RL is 5dB lower, and ER is 2dB lower.
Connector key is aligned to slow axis.
Package Dimensions
Ordering Information
STHPMFR-①①①①-②②②-③④-⑤-⑥⑥-⑦⑦⑧⑧ (PM Fiber Type)
ST HPIFR-①①①①-②②②-③④-⑤-⑥⑥-⑦⑦⑧⑧ (SM Fiber Type)
①①①①
- Wavelength:
1064=1064nm, 1030=1030nm, 980=980nm, 780=780nm, SSSS=Specified
②②②
- Fiber Type:
003=PM980, 004=HI1060, 018=PM 10/125DCF, SSS=Specified
③
- Package Dimensions:
0=64x28x26mm, S=Specified
④
- Pigtail Type:
0=bare fiber, 1=900μm loose tube
⑤
- Fiber Length:
0.8=0.8m, 1.0=1m, S=Specified
⑥⑥
- Connector Type:
0=FC/UPC, 1=FC/APC, 2=SC/UPC, 3=SC/APC, N=None, S=Specified
⑦⑦
- Average Power:
00=500mW, 01=1W, 05=5W, 10=10W, SS=Specified
⑧⑧
- Peak Power:
00=Continuous Wave, 01=1kW, 02=2kW, 10=10kW, SS=Specified
Q:What is Faraday Rotator and its use for?
A: Faraday Rotator is an optical device that utilizes the Faraday effect to rotate the polarization plane of light. The Faraday effect, a phenomenon discovered by Michael Faraday, involves the rotation of light's polarization plane when light travels through a material and is subjected to a magnetic field in the direction of propagation.
Here's how a Faraday Rotator works and its uses:
How it Works:
Material with Verdet Constant: The Faraday Rotator typically consists of a piece of material known as a Faraday medium (like flint glass or certain types of garnet), which has a high Verdet constant—a measure of the material's effectiveness in rotating the polarization of light in the presence of a magnetic field.
Application of Magnetic Field: When light passes through this material, and a magnetic field is applied in the direction of the light propagation, the plane of polarization of the light is rotated. The angle of rotation is proportional to the strength of the magnetic field and the length of the path through the material.
Non-reciprocal Rotation: A crucial aspect of the Faraday Rotator is that the rotation of the polarization is non-reciprocal. This means that if the light passes through the material in the opposite direction, the polarization plane rotates in the same direction, not the opposite. This property is fundamental to many of its applications.
Uses:
Isolators in Laser Systems: One of the primary uses of Faraday Rotators is in optical isolators, which allow light to pass in one direction while blocking it in the opposite direction. This is crucial in laser systems to protect the laser from destabilizing feedback and reflected light, which can damage the laser or degrade its performance.
Optical Circulators: Faraday Rotators can be used in devices like optical circulators, which direct light sequentially from one port to another in a unidirectional manner. This is useful in fiber optic communication systems.
Measurement and Sensing: The sensitivity of Faraday Rotators to magnetic fields makes them useful in measuring the strength and direction of magnetic fields, such as in magneto-optical sensors.
Quantum Computing and Cryptography: The non-reciprocal nature of Faraday Rotators is beneficial in certain quantum computing and quantum cryptography setups, where controlling the direction and state of photons is crucial.
The unique properties of Faraday Rotators, especially their non-reciprocal polarization rotation, make them vital components in advanced optical systems, ensuring efficient operation and protection of sensitive components.
Q:What does Insertion loss mean?
A:Insertion loss refers to the loss of signal power resulting from the insertion of a device in a transmission line or optical fiber and is usually expressed in decibels (dB). When a signal passes through any electronic device or a transmission medium, some of its power is lost due to various reasons like absorption, scattering, reflection, and material imperfections.
In the context of electronics and signal processing, insertion loss measures how much the signal has weakened after passing through a filter, cable, connector, or other network component. A lower insertion loss implies that the device has a better performance, meaning it allows more of the signal to pass through with less attenuation.
In the context of optical fibers and systems, insertion loss can refer to the loss of signal power resulting from the insertion of components such as connectors, splices, and fiber length.
It's important in system design and testing to ensure that the total insertion loss does not exceed a certain level to maintain the quality and integrity of the signal or to meet power budget requirements.
Q:What is Extinction Ratio?
A:The Extinction Ratio is a term commonly used in the fields of optics and telecommunications, especially when discussing the performance of optical components like modulators and switches, as well as in fiber optic communications. It is a measure of the effectiveness of a device in distinguishing between its "on" (light) and "off" (dark) states. Here's a more detailed explanation:
1. In Optical Communications: Extinction Ratio pertains to the ratio of the optical power output when the light source is on (Pon) to the optical power output when the light source is off (Poff). It's usually expressed in decibels (dB) and can be calculated using the formula:
A higher extinction ratio indicates a clearer distinction between the on and off states, leading to less ambiguity in signal interpretation, reduced error rates, and overall better performance in digital communication systems.
2. In Optical Components: For components like modulators, which are used to encode information onto a light beam, the extinction ratio measures the contrast between the maximum and minimum optical power levels (representing digital '1' and '0', respectively). In this context, a high extinction ratio is crucial for maintaining signal integrity, as it ensures that the '1's and '0's are distinctly recognizable by the receiving end of the communication system.
3. Importance in System Performance: The extinction ratio is an important parameter in digital optical communication systems because it affects the bit error rate (BER). A low extinction ratio can lead to higher bit error rates as the receiver might find it difficult to distinguish between the '1' and '0' states. Therefore, maintaining a high extinction ratio is essential for the reliability and efficiency of optical communication systems.
In summary, the extinction ratio is a key performance metric in optical systems, indicating the ability of a device to clearly differentiate between its on and off states, which is crucial for the accuracy and reliability of data transmission in fiber optic networks.
Q:What is Rotation Angle Tolerance?
A:Rotation Angle Tolerance is a term commonly used in various fields like manufacturing, engineering, and computer vision to describe the acceptable range of angular deviation from a specified orientation. It defines how much an object, component, or feature can rotate from its intended position before it is considered out of specification or unacceptable. Here's a bit more detail depending on the context:
Manufacturing and Engineering:
In manufacturing, parts are often designed to fit together in a very specific orientation. The Rotation Angle Tolerance would specify the allowable range of rotation for a part about its axis. If a part rotates more than the specified tolerance, it might not fit correctly with other components, leading to assembly issues or functional failures.
Computer Vision and Image Processing:
In these fields, Rotation Angle Tolerance might refer to the degree of rotation an algorithm or system can handle when identifying, matching, or tracking objects in images or video feeds. For example, a facial recognition system might have a Rotation Angle Tolerance of ±15 degrees, meaning it can correctly identify faces that are tilted up to 15 degrees from the vertical
Q:What does Polarization Mode Dispersion mean?
A:Polarization Mode Dispersion (PMD) is a phenomenon in fiber-optic communications that can cause distortion and degradation of the signal. It arises due to the intrinsic imperfections and asymmetries in the optical fibers, which result in different polarization modes (orientations of the electromagnetic waves) traveling at slightly different speeds.
Here's a breakdown of PMD and its implications:
Dual Polarization Nature of Light: Light in fiber optics can be polarized in two perpendicular orientations. In an ideal world, these two polarizations would travel at the same speed. However, due to imperfections in the fiber, this isn't always the case.
Differential Group Delay (DGD): Because of these imperfections, the two polarization modes can propagate at slightly different velocities. This difference in velocities leads to what's called Differential Group Delay (DGD), where one polarization mode arrives slightly before the other. DGD is the primary measure of PMD and is typically expressed in picoseconds.
Impact on Signal Quality:
Broadening of Pulses: In high-speed data transmission, information is sent in very short pulses of light. PMD can cause these pulses to spread out and overlap, making it hard for the receiver to distinguish between them. This effect is more pronounced as data rates increase, making PMD a significant issue for high-speed networks.
Time-Varying: PMD isn't a static phenomenon. Changes in temperature, physical stress on the fiber, or even the passage of time can change the characteristics of PMD in a system, making it a challenging problem to compensate for.
Mitigation and Compensation: Given its potential to impair data transmission, especially in high-speed networks, various techniques are employed to mitigate PMD. These include manufacturing better-quality fibers with less PMD, using PMD compensation devices, and sophisticated signal processing techniques.
PMD is a critical parameter in the design and operation of fiber-optic communication systems, especially as the demand for high-speed data transmission continues to grow.
Q:What is Axis Alignment?
A:Axis alignment generally refers to the process of adjusting or orienting an object, system, or components so that their axes are in a specified position relative to each other or to a reference.
Axis alignment is a critical procedure in many technical and engineering fields. Proper alignment ensures that systems operate correctly, efficiently, and safely, and it often requires precise measurement and adjustment tools.
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