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Large NA High Sensitivity Fiber Spectrometer HiNA Series

  • The HiNA series  Large NA High Sensitivity Spectrometer is a High-performance Spectrometer designed specifically for Raman applications requiring high luminous flux and sensitivity, it is currently available in three different wavelength ranges 532nm, 785 nm and 1064nm.

     

     

    Features

     High luminous flux 

    • Support GPIO 

    • High sensitivity, high UV response 

    • Batch Consistency Control 

    • Various communication interfaces, support USB, serial port 

    • Low-temperature drift, wide operating temperature range: -20~60℃

     

    Technical Advantages

    1. Ultra-high luminous flux

    F/2 is not only fully coupled to the input from 0.22NA fibers but also designed for redundancy and compatibility with special fibers with larger numerical apertures or customised input optical paths.

     

    2. Powerful PC software

    PC software provided with the spectrometer: FLAVOR is powerful software. In addition to the basic spectrum acquisition control functions, it also has functions such as saturation and automatic adjustment of the integration time, recording of the real integration time, and automatic peak finding. At the same time, the software also includes characteristic functions such as wavelet smoothing with patented technology.

    SDK supports Windows, Android, and Linux operating systems, and can provide secondary development packages in C#, C++, Java, Python, and other languages.

     

    3. High stability

    Within 0~40°C temperature drift, the spectral resolution remains unchanged, preferable for industrial applications.

     

    4. Customisable

    A wide choice of reflective flashing gratings allows you to customise the waveband to suit your needs.

     

    Product specifications and Brochures

    Product Brochure Link:  产品手册.png

     

    ModelHiNA532HiNA785HiNA1064
    Raman Range0~3600cm -10~2480cm -10~1700cm -1
    Band Range530~658nm780-975nm1064~1300nm
    Resolution ( @50um slit)

    0.5nm

    16cm -1

    0.7nm

    10cm -1

    0.9nm

    7cm -1

    Slit Width*25~200um50~200um50~200um
    F/#F/2F/2F/2
    Grating*1800l/500nm1200l/850nm830l/1200nm
    CCD Detector**Hamamatsu, S7031-1006SHamamatsu, G14237-512WA
    Built-in Filter

    Minimum wave number

    200cm -1

    Minimum wave number

    200cm -1

    Minimum wave number

    200cm -1

    Size170 x 179 x 64.5mm
    Weight1.5kg

     

    * Customicable

    ** The Spectral Response of the Hamamatsu CCD detector is as follows

     

     

    S7031-1006SG14237-512WA

     


    Multi Channel Upgrade Option

     

    Do you need more precise measurements over a broad wavelength range?  Our multi-channel spectrometers upgrade option offers a solution. Choose the desired spectrometer wavelength range, and we can integrate them into a single system (up to 4 channels) with single fiber or multi fiber output option. Please contact us for more info.

     

     

    Product Size
    格物HiNA光谱仪尺寸.jpg

     

     

    Software Interface

     

    Main software user interface

    1.Detection Panel  (Function menu and operation buttons)

    2.Device Panel (Device list and paremeter settings)

    3.Spectral Window (Spectral curve display and spectral window management)

    4.Spectral Recording Panel (Spectral curve selection and naming)

     

    Key Spectral processing feature 

    ● Wavelength Smoothing 

    ● Defluoresence 

    ● Substract the background signal

    ● Rransmission and reflection measurement 

    ● Absobance measurement 

    ● Multi measurement with different timing



  • Due to the limited number of pixels in the spectrometer detector, at high spectral resolution, only a few pixels form a single spectral peak, resulting in no smooth peak, as shown in the following figure.

    This figure shows an example of peak position drift caused by temperature drift of the spectrometer at different temperatures. The spectral peak is not symmetrical because the number of pixels that make up the spectral peak is very small, and under the influence of temperature drift, the highest pixel of the spectral peak moves one pixel from left to right.


    At this point, we have two methods to evaluate the drift of this peak position.

    1. Check the position of the highest pixel point. Obviously, the peak position has shifted by one pixel, which means approximately 0.15 nm.

    2. Fit the peak values before and after drift, and find the fitted peak point between two pixels. The drift of the fitted peak point is about 0.07nm

     

    So which of these two methods is correct? We believe the second one is correct, reflecting the true drift of the peak position. The reasons are as follows.

    1.High resolution results in a low pixel sampling rate for spectral peaks, and directly observing the shape of a pixel does not reflect the actual shape of the peak.

    2.The spectral peak is physically closer to a symmetrical distribution, and the shift in peak position will not cause a change in peak shape.

    3.By fitting all the pixels that make up the spectral peak, the peak shape obtained is closer to the physical reality of the peak.


    Therefore, using fitted peak shapes to determine peak positions and evaluate spectrometer drift is the correct method.


    Is it necessary to do so in practice? It depends on the actual situation. If

     

    1.Low spectral resolution and high sampling rate of spectral peaks require more pixels to form a peak, and these pixels themselves are connected in a smoother and more symmetrical peak shape. Then, the position of the highest pixel or between two pixels can be directly found, and the peak position can be confirmed through visual evaluation.


    2.With high spectral resolution and the need to accurately know peak values, the above fitting method is required. Fitting can be achieved through spline algorithm or Gaussian or Lorentz fitting, and one can choose based on the spectral properties of the tested sample. If you don't know how to choose, please use spline curves.


  • parts

    For more information about customized accessories, please contact us sales@goptica.com

    ModelCategoryWavelengthCore DiameterLength# Number of coresInterface
    I1000-S/S-L2fiber optic360~2500nm1000um2m1SMA905-SMA905
    V1000-S/S-L2200 ~ 1100 nm1000um2m1SMA905-SMA905
    DV600-S/S-L2190~1100 nm600um2m1SMA905-SMA905
    I600-S/S-L2360~2500nm600um2m1SMA905-SMA905
    V600-S/S-L2200 ~ 1100 nm600um2m1SMA905-SMA905
    DV400-S/S-L2190~1100 nm400um2m1SMA905-SMA905
    I400-S/S-L2360~2500nm400um2m1SMA905-SMA905
    V400-S/S-L2200 ~ 1100 nm400um2m1SMA905-SMA905
    DV200-S/S-L2190~1100 nm200um2m1SMA905-SMA905
    I200-S/S-L2360~2500nm200um2m1SMA905-SMA905
    V200-S/S-L2200 ~ 1100 nm200um2m1SMA905-SMA905
    DV100-S/S-L2190~1100 nm100um2m1SMA905-SMA905
    I100-S/S-L2360~2500nm100um2m1SMA905-SMA905
    V100-S/S-L2200 ~ 1100 nm100um2m1SMA905-SMA905
    I1000-Y*2-S/S-L2

    Forked optical fiber,

     Y-shaped fiber: 2 fibers

    360~2500nm1000um2mA-2 core, B1-1 core, B2-1 coreA-SMA905 / B1-SMA905 / B2-SMA905
    V1000-Y*2-S/S-L2200 ~ 1100 nm1000um2mA-2 core, B1-1 core, B2-1 coreA-SMA905 / B1-SMA905 / B2-SMA905
    DV600-Y*7-S/S-L2190~1100 nm600um2mA-7 core, B1-1 core, B2-6 coreA-SMA905 / B1-SMA905 / B2-SMA905
    I600-Y*7-S/S-L2360~2500nm600um2mA-7 core, B1-1 core, B2-6 coreA-SMA905 / B1-SMA905 / B2-SMA905
    DV600-1*7-S/S-L2multi-core optical fiber190~1100 nm600um2m7SMA905-SMA905
    I600-1*7-S/S-L2360~2500nm600um2m7SMA905-SMA905



    Integral ball

    Wavelength 250 - 2500 nm

    Output ports can be customized

    Black anodized aluminum alloy shell

    Gilded Integral Ball

    Wavelength 1000 - 5000 nm

    Electrochemical Coating with Diffuse Reflective Film

    Halogen light source

    Wavelength 360 - 2500 nm

    Long service life, usually 10000 hours

    SMA905 interface

    Deuterium lamp light source

    Wavelength 190 - 400 nm

    Long service life, usually 1500 hours

    SMA905 interface

    Sample holder for transmittance measurementSample holder with reflectivity measurement bracket
    Colorimetric dish rackOptical support for measuring transmission and reflection samples

    Fiber optic attenuator

    Wavelength 200 - 2500 nm

    Adjustable slit for attenuation

    Fiber collimator

    Wavelength 185 - 2500 nm

    Numerical aperture 0.22 - 0.37 NA,

    Core diameter ≥ 100 µm



3 products in total Add Contrast

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  • Product customization

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