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