Gigahertz-Optik 徽标

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Gigahertz Optik GmbH (总部)
Phone: +49 (0)8193-93700-0
info@gigahertz-optik.de

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整合球体光源

具有连续宽带或LED窄带发射光谱的集成球体光源。均匀光源可作为相机校准的亮度标准,用于确定遮挡眩光,用于调整夜视设备等等。均匀光源的直径从50毫米到500毫米,监控探测器选项,通过手动和远程光圈控制信号输出等。

自几个世纪以来,Gigahertz-Optik 一直是标准和专业配置的高质量均匀积分球光源的专家。通过我们的 集成球体建造套件 多种模块,我们能够生产所需的配置。

在积分球光源上可以设计什么?

  • 以球输出端口和球直径本身为基础
  • 根据对均匀性的要求,确定光源的位置、数量和挡板(如果需要,不均匀度为 0.25)
  • 通过可变孔径对多个强度量级进行高动态强度控制
  • 适合控制任务的参考探测器(光谱辐射计、积分探测器)
  • 用于多种用途的附加端口,如光纤耦合、第二参考探测器等
  • 球形输出的校准选项和 ISO 17025 测试(如光谱辐射度)
  • 通过机架式电子设备或 PC 软件控制

由于这种灵活性,我们的积分球光源可用作以下用途

  • 亮度标准(转移标准)
  • 用于照相机校准的亮度光源
  • 用于确定遮蔽眩光(如镜头)的光源
  • 用于调整夜视设备的光源
  • 用于坏像素检测和相机白平衡的光源

我们设计的均匀积分球光源直径从 50 毫米到 500 毫米不等,完全满足您的需求,确保精确度。

另请参阅我们的其他产品部分 28[/ategory_link] 和我们最新的 基于光谱可调 LED 的光源

Selection of integrating sphere light sources. Please contact us if a customized solution is needed.

 

Model Image Sphere Diameter Light output port Calibrated spectral range / nm Light source Output range Output adjustment Remark
ISS-5P ISS-5P 50 mm

20 mm

(380 - 1100) nm Integrated 10 W tungsten-halogen None Compact and portable transfer standard lamp
ISS-5P-SR-FS ISS-5P-SR-FS 50 mm (380 - 1700) nm LH-5-UV-Quartz halogen None e.g. for fluorescence spectrometer calibration
ISS-8P-HP ISS-8P-HP 80 mm

19 mm

(380 - 1100) nm External up to 100W tungsten-halogen (120, 12 & 1.2) kcd/m² @ CCT 2960K (75, 75, 0.75) kcd/m² @ CCT 2856K Exchangeable OD0, OD1 & ODx filters Constant color temperature and uniformity as luminance varied.
ISS-8P-VA ISS-8P-VA 80 mm

19 mm

(380 - 1100) nm External up to 100W tungsten-halogen (0 - 95000) cd/m² @ CCT 2960K (0 - 63000) cd/m² @ CCT 2856K Manual control variable aperture Continually variable intensity control.
ISS-8P-VAHP ISS-8P-VAHP 80 mm

19 mm

(380 - 1100) nm External up to 100W tungsten-halogen (0 - 57000) cd/m² @ CCT 2960K (0 - 39000) cd/m² @ CCT 2856K Exchangeable OD0, OD1 & OD filters + variable aperture Fine adjustment, continually variable intensity control.
ISS-8P-RVA-ROD ISS-8P-RVA-ROD 80 mm 360 - 830 nm R 632nm, G 520nm, B 449nm, W R 1.99 cd/m2 G 2.01 cd/m2 B 1.98 cd/m2 W 2.00 cd/m2 Manual or remote controlled Light field projected 200 mm in front of sphere. E.g. suitable for use with climatic chambers
ISS-15-RGBW ISS-15-RGBW 150 mm 360 nm - 830 nm LED Depends on single LED settings Current setting. Integrating sphere light source for EMVA 1288 standard with LED light source and continuous intensity adjustment
ISS-17-VA ISS-17-VA 170 mm

50 mm with resolution tube to suppress the lateral incident light (UMPA-2.0-xx)

(380 - 800) nm External 100W tungsten-halogen (3 - 7.500) cd/m² @ CCT 2856K (5 - 15.000) cd/m² @ CCT 3100K Manual control variable aperture Monitor detector calibrated for color temperature and luminance
ISS-17-VAM ISS-17-VA 170 mm

50 mm with resolution tube to suppress the lateral incident light (UMPA-2.0-xx)

(380 - 800) nm External 100W tungsten-halogen (3 - 7.500) cd/m² @ CCT 2856K (5 - 15.000) cd/m² @ CCT 3100K Motorised variable aperture Monitor detector calibrated for color temperature and luminance
ISS-30-TLS ISS-17-RGBW_23.10.2023_09.10.09 300 mm

100 mm

360 nm - 830 nm multiple LED, depending on configuration dependent on LED configuration S-ISS software control Integrating sphere light source with spectral LED adjustment, continuous intensity adjustment and spectral reference sensor
ISS-30-VA ISS-30-VA 300 mm

100 mm

(300 - 1100) nm @ CCT 2960K External 100W tungsten-halogen (0 - 3500) cd/m² @ CCT 2960K Manual control variable aperture Monitor detector calibrated for output port luminance
ISS-30-VAM ISS-30-VA 300 mm

100 mm

(300 - 1100) nm @ CCT 2960K External 100W tungsten-halogen (0 - 3500) cd/m² @ CCT 2960K Motorised variable aperture Monitor detector calibrated for output port luminance
ISS-30-VA-V05 ISS-30-VA-V05 300 mm 300 nm - 1100nm LED and halogen See product page Integrating sphere light source with homogeneous light field for applications of camera calibration, etc. based on LED and halogen lamp.
ISS-50-LU-FE ISS-50-LU-FE 500 mm - 3 x 100W tungsten-halogen each 2856K, 5000K or 6000K, filter wheel selected - - Hemispheric illuminated field due to position of super wide-angle or fish-eye cameras in the sphere center. Three different color temperatures, switchable with filter wheels.