Flir ThermovisionVoyager II Operators Manual
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51 Weather Environmental conditions, including time of day, humidity, and precipitation, will aff ect image quality and contrast. Fog, smog and rain will decrease the range at which you can detect a given target. After sunset, objects warmed by the sun during the day will radiate their stored heat for several hours. Early in the morning, many of these objects will appear cooler than their surroundings, so be sure to look for subtle temperature diff erences in the scene, not just hot (white) targets.
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52 MORE ABOUT INFRARED At fi rst blush, new technologies can appear intimidating. Infrared cameras may seem imposing, but they are not so diff erent from digital camcorders. In fact, you can get years of enjoyable, productive use out of your Voyager without knowing anything in this section. But, if you would like to learn more about thermal imaging – how it was discovered and developed – read on. Infrared – the early years Th e road to modern thermal imaging began way back in 1666, when Sir Isaac...
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53 53 High school physics revisited Infrared radiation combines with Gamma rays, X-rays, Ultra Violet, Visible Light, Microwaves and Radio Waves to form a range of energy called the Electromagnetic Spectrum. Th ese are not independent types of energy – in fact, the primary diff erence between each of these types of radiation is wavelength: Radio Waves have the longest wavelength and Gamma Rays have the shortest. Wavelengths are measured in micrometers, or “microns” (μ), which are equal to one...
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54 2) At a given temperature, the amount of thermal energy radiated by an object depends on its emissivity. Emissivity is the measure of an object’s effi ciency at radiating thermal energy. For example, shiny metals are poor emitters. Instead of radiating their own thermal energy, they tend to refl ect radiation from their surroundings. Infrared, from theory to practical application Infrared imagers operate by detecting the relative intensities of thermal energy radiated from the surfaces of...
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55 Th ermal energy doesn’t pass through much, but it does “transmit” through some plastics. When a material is not transparent to infrared radiation, it is said to be “opaque.” Most commonly viewed materials are opaque to infrared radiation. Materials that mirror the infrared signatures around them are “refl ective.” Ever y thing is refl ective to one degree or another, but the most highly refl ective objects are those made of polished, unpainted metal. Painted metals, glass, and even wood can...
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56 Under typical conditions however, atmospheric moisture and dust scatter can absorb some of the radiated energy before it reaches the imager. Th e eff ect of this is to weaken the overall thermal signal and shorten the range at which you can detect it. Th e weather can impact more than just the range at which the Voyager can detect a specifi c object – it can also aff ect an entire scene’s thermal contrast and aff ect overall system performance. Cloud cover aff ects the diurnal cycle in two ways:...
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58 APPENDIX Parts List Th e Voyager includes the following thermal imaging components: If the components you have are diff erent from those enumerated in this parts list, please call us immediately at 888.747.3547. Vo y a g e rFLIR Part Number Camera Body7. 3 ”x 4 . 0 ”x 8 . 0 ” 432-0002-01-00 432-0002-01-00S 432-0002-02-00 432-0002-02-00S Bulkhead Box6lb500-0348-00 Joystick Control Unit (JCU)500-0353-00 Camera Cable 50’ or 10 0 ’308-0149-50 or 308-0149-100 JCU Cable10 0 ’ 308- 0139- 0 0 Operator’s...
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59 SYSTEM OVERVIEW Size15” x 23” Weight45 lb. Azimuth Field-of-Regard360° Continuous Elevation Field-of-Regard+/-90° Slew RateVariable to 120°/sec. Thermal Imaging Performance Sensor Type2 Microbolometer Cameras Wide FOV Imager20° x 15° (35mm) Narrow FOV Imager5° x 3.75° (140mm) Spectral Range7.5 to 13.5 μm Daylight Imaging Performance Sensor Type1/4” Super HAD Wide FOV Limit42° horiz. @ F1.6 Narrow FOV Limit1.6° horiz. @ F3.8 System Speci cations Pan/Tilt Coverage360° Az./ +/-90° El. Video outputNTSC...