HIGH INTENSITY LIGHT SOURCE -- D-165The Model D-165 High Intensity Light Source is an optimum efficiency (low intensity loss) illuminator ideally applicable to industrial use where limited space and manifold requirements prohibit normal source installations.
The principal application is as an illuminance source for one or more optical or electrooptical instruments where flexibility and interchangeability are important. Optimum illuminating efficiency is insured by employing all solid state circuitry, an easily serviceable reflector/quartzline lamp and fan-cooled operation. Design of the Model D-165 enables the use of all standard sized metal ferrule flexible (fiber optic) light guides. |
Detailed Specifications:
| Input power | 117 ±5 volts, 60 Hz | |
| Lamp | G.E. Reflector/Ouartzline
P/N 333-0070-005 |
|
| Optical Output | 70 Watts maximum | |
| Light Intensity | Low | 28,000 foot lamberts |
| High | 356,000 foot lamberts | |
| Lamp Life | approximately 200 hours | |
| Dimensions | Height | 7" |
| Width | 5¾" | |
| Length | 8½" | |
| Finish | Ivory Enamel | |
| Light Source Weight | 5½ pounds | |
| Shipping weight | 8 pounds | |
The available Model D-165-101 uses 220 ±5 volt, 50Hz power.
Three flexible Light Guide lengths are available:
| Part Number | Diameter of Fiber Optics Bundle | Metal Tip O.D ±0.005" | Length |
| 613-0305-012 | ¼" | 0.316" | 12" |
| 613-0305-024 | ¼" | 0.316" | 24" |
| 613-0305-036 | ¼" | 0.316" | 36" |
Available Instrument to Light Guide Adapters include:
| Instrument Model Number | Part Number |
| D-271 Alignment Telescope | 530-0066 |
| D-275 Alignment Telescope | 530-0066 |
| D-600 Comparison Autocollimator | 530-0066 |
| D-602 Manual Autocollimator | 530-0066 |
| D-638 Coordinate Autocollimator | 100-0117 |
| D-652 Two Axis Autocollimator | 100-0128 |
| D-656 Two Axis Autocollimator | 100-0117 |
| D-657 Tooling Autocollimator | 530-0066 |
| D-660 Tooling Autocollimator | 100-0171 |
Davidson Optronics, Inc.
Phone: (626) 962-5181
Fax: (626) 962-5188
E-mail: sales@davidsonoptronics.com
