|
| Calibration and testing of: | | Development and production of: | | Monitoring and Measurement of |
 | fLIR test systems |
| |
| camouflage materials |
| |
| atmospheric transmission |
|
| E-O simulators |
| |
| E-O countermeasures |
| |
| temprature |
|
| E-O sources |
| |
| E-O jammers |
| |
| emissivity |
|
| E-O jammers |
| |
| rocket engines |
| |
| reflectivity |
|
| Materials |
| |
| jet engines |
| |
| moisture content |
|
| |
| E-O heat seekers |
| |
| air pollution |
|
| |
| E-O sensors |
| |
| gas burning by-products |
|
|
| ADVANTAGES
 |
|
| High sensitivity |
| |
| Wide spectral band (UV to IR) |
| |
| Wide spectral band (UV to IR) |
|
| High accuracy |
| |
| High reliability |
| |
| Usable in laboratory or field |
|
|
|
FEATURES
|
|
| Automatic self calibration |
| |
| Spectral mode measurements (radiance vs. wavelength) |
| | |
| Real-time data analysis and display |
| |
| Radiometric mode measurements (radiance vs. time) |
| | |
| Rapid scan rates |
| |
| Full keyboard control |
| | |
| Flexible software packages |
| |
| Accurate even for measurement of objects that are at ambient temperatures |
|
| Computation of calibrated spectra is a matter of seconds |
| | | | |
|
|
SIGNAL PROCESSING
|
|
| Signal processing for improved sensitivity |
| |
| Lowtran software for atmospheric transmittance |
| | |
| Mathematical computations with spectral data |
| |
| Spectral emmissivity |
| | |
| Transient analysis of rapidly occuring events |
| |
| Effective temperature measurement |
| | |
| 3-D plots (radiance vs. time and wavelength) |
| |
| Countermeasures analysis |
| | |
|
|
SPECIFICATIONS
|
|
| Optics: | | 5" diameter fully reflective telescope f/no=4 (f/no=2 for SR5000W) |
| Focusing range: | | 2.5m to infinity | | |
| Spectral range: | | 0.2 to 25 microns | | |
| Segments spectral resolution | | 2% of wavelength (typical segment dependent) | | |
| Scan rates: | | 0.015 to 30 scans/sec | | |
| Aiming: | | Non parallex though optics on line sighting | | |
| Uniformity of FOV: | | 10% (typically 5%) | | |
| Detector types: | | User interchangeable (even in field) with no need to realign |
| Internal Blackbody: | | At ambient temperature, monitoring accuracy better than 0.1oC | | |
| Chpping Frequency: | | 100 to 1800 Hz. | | |
| Noise performance: | | Wavelength and detector dependent. Example: Maximum 5 mdeg NET with InSb detector and CVF at 5ym, 1Hz bandwidth, 100oC Blackbody filling 6 mrad FOV | |
|
| |
