
Olympus' DUV system uses a 248 imaging band that is corrected to prevent chromatic aberrations. This results in bright, high-contrast images with resolutions down to 80 nm. The module can be mounted to the Olympus family of optical microscope.
The optical system optimized for 248 nm provides resolutions down to 80nm, two times better than that available with the visible light. The 248 ±4nm imaging band is corrected to prevent chromatic aberrations. This technique makes it possible to observe both high-contrast and high-resolution features without preprocessing. Common applications for DUV observation include detailed inspections of semiconductor patterns, gap and pole identification on magnetic heads, and microlithography.
Deep Ultraviolet Observation |
Visible Light Observation |
DUV Objective Lens |
The DUV lens is specially designed with a unique "non-cemented" technology to prevent deterioration found in other DUV lenses, making it an ideal solution for long-term use. |
Deep Ultraviolet Observation Module |
The modularity of the DUV system not only allows for integration with the Olympus MX and BX series of microscopes, but allows the mercury-xenon power supply to be independent of the microscope and directs the illumination to the DUV module via a UV light guide. The shutter design employed protects the operator by directing the illumination to the DUV objective lens and camera only. In addition, since the light source is set apart from the microscope and the intensity can be independently controlled to the optimum level, heat transition to the sample is minimized. |
The high resolution DUV digital camera is software controlled and capable of high-speed data acquisition. Images captured on the computer can be quickly documented and analyzed for easy storage in a database and report generation.
The DUV intermediate tube is simple with no moving parts or external control; this allows the tube to be half the size and weight of conventional DUV microscope systems.
Lamphouse and Power Supply |
A long-life mercury xenon lamp is used to power the DUV module. Its average lifetime is >1000 hours, thus reducing operating costs and minimizing lamp replacements. |
Integration of Deep Ultraviolet optical units with a compatible microscope frame enables a DUV observation microscope. For the detail of compatible microscopes, refer to the Specification of each microscope.
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Deep-ultraviolet Observation Units
| U-UVF Specifications | |||
| UV248 Lens Tube U-UVF248IM | DUV Optical System | Wavelength Used | 248±4nm |
| Light Source | 80W Mercury Xenon Lamp | ||
| Objective Lens | Dedicated DUV100x Objective Lens: N.A. 0.9, WD 0.2mm | ||
| Intermediate Magnification | 2.5x | ||
| Field Number |
12.5
(Actual Field of View: 50µm) | ||
| Applicable Operating Environment | 23±5°C | ||
| Visible-light Optical System | Objective Lens | UIS Objective Lens | |
| Intermediate Magnification | 1x | ||
| Field Number |
22
(20 for Camera Observation) | ||
| UV248 Light Source Box U-UVF248LB | Light-intensity Control Shutter |
Non-step Manual Control from 0 to 100%
Vertical Slide Switching Lever | |
| UV Light Guide U-UVF2FB/5FB | Length: 2m or 5m | ||
| Mercury Xenon Lamp House U-LH80HGXE | 80W Mercury Xenon Lamp Installed | ||
| Power Supply Unit | USHIO Product (100V to 120V) | ||
> MX61A: Motorized Model Compatible with 300mm Wafers while Enabling Integrated Control over Peripheral Devices
> MX61L/ MX61: Motorized Model Compatible with 300 mm/ 200 mm Wafers
> MX51: Manual Model Compatible with 150mm Wafers
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