Micro-Hyperspec NIR sensors come in either 320- or 640-spatial-pixel models for field or lab use. They are CE certified, small and light with Base CameraLink interface and low power requirements. However, many researchers who undertake remote-sensing missions using drones or field kits will choose the Co-Aligned VNIR-SWIR system because of its greater wavelength range.
Headwall Micro-Hyperspec NIR 320
Quick Comparison
| Headwall Micro-Hyperspec NIR 320 remove | HySpex Mjolnir V-1240 remove | Resonon Pika IR-L+ remove | Specim FX50 remove | HySpex Baldur S-640i N remove | HySpex VS-1200 remove | |
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| Name | Headwall Micro-Hyperspec NIR 320 remove | HySpex Mjolnir V-1240 remove | Resonon Pika IR-L+ remove | Specim FX50 remove | HySpex Baldur S-640i N remove | HySpex VS-1200 remove |
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| Content | Micro-Hyperspec NIR sensors come in either 320- or 640-spatial-pixel models for field or lab use. They are CE certified, small and light with Base CameraLink interface and low power requirements. However, many researchers who undertake remote-sensing missions using drones or field kits will choose the Co-Aligned VNIR-SWIR system because of its greater wavelength range. | HySpex Mjolnir V-1240 The HySpex Mjolnir V-1240 hyperspectral imaging system for UAVs provides a unique combination of small form factor and low mass, combined with high-performance specifications and scientific grade data quality. With a weight of less than 4 kg and less than 50 W power consumption, HySpex Mjolnir V-1240 is very well suited for a wide range of UAVs. The system is also compatible with several off-the-shelf gimbals. NEO offers high-performance unmanned aerial vehicles, fully integrated with the HySpex Mjolnir V-1240. The UAV is fitted with a standard battery package allowing up to 30 minutes of flight time. All HySpex Mjolnir systems can also be mounted on a tripod and rotation stage for ground use. | Pika IR-L+ 925 - 1700 nm Lightweight, High-Precision Infrared The Pika IR-L+ imager is a high spatial and spectral resolution Near-Infrared (925-1,700 nm) imager in a lightweight, compact format. It is well suited for field research, yet compatible with all imaging platforms (airborne, benchtop, or outdoor). For a compact, lightweight Visible light spectral range option, please see the Pika L. For higher imaging speeds, please see the Pika IR-L. | Specim FX50 Specim FX50 is the only hyperspectral camera on the market covering the full mid-wave infrared (MWIR) spectral range of 2.7 - 5.3 ?m required, for example, in black plastics sorting. Specim FX50 is a high-speed, accurate, and efficient line-scan hyperspectral camera designed specifically for industrial environments. | HySpex Baldur S-640i N Baldur S-640i N covers the spectral range from 950-1730nm. All Baldur cameras are Nyquist cameras giving a spectral resolution of 2 spectral bands while capturing 4 times as much light as the classic systems. To ensure that the most information per framerate is provided, the spectral resolution is kept very close to 2 bands. Additionally, the spatial resolution of Baldur S-640i N is better than 1.5 pixels, yielding a very sharp camera. | HySpex VS-1200 The HySpex VS-1200 hyperspectral camera is developed for airborne applications requiring extreme resolution in both VNIR and SWIR spectral regions. The HySpex VS-1200 is a novel high-resolution instrument designed for airborne applications at altitudes greater than 400m. The camera produces the highest scientific grade level data, commercially available, having FWHM less than 1.2 pixels spatially and less than 1.5 pixels spectrally. The combined VNIR-SWIR cube has coregistration errors, and smile and keystone of less than 10% of a pixel. With 40 degrees FOV, the camera is ideal for mapping large areas with high accuracy and resolution. The camera is delivered with an integrated high-performance IMU/GPS and data acquisition unit with removable storage bays as a standard. Existing navigation systems can also be integrated/utilized. A standard passive damping solution is included as a part of the default delivery package, but mounting plates for active damping solutions, such as GSM4000 or PAV80 can be supplied. |
| Description | Spectral range = 400 - 1000 nm Spatial pixels = 1240 Spectral channels and sampling = 200 bands @ 3 nm F-number = F1.8 FOV = 20? Pixel FOV across/along = 0.27/0.27 mrad Bit resolution = 12 bit Noise floor = 2.3 e- Dynamic range = 4400 Peak SNR (at full resolution) > 180 Max speed (at full resolution) = 285 fps Power consumption = 50 W Dimensions (l-w-h) = 250 - 175 - 170 mm Weight < 4 kg *Includes IMU/GPS and DAU - <6.5 kg including standard battery | Spectral Range (nm) = 925 - 1700 Spectral Channels = 470 Spectral Bandwidth (nm) = 1.7 Spectral Resolution - FWHM (nm) = 3.8 Spatial Pixels = 640 Max Frame Rate (fps) = 176 f/# = 1.8 Interface = GigE Dimensions (mm) = 210 x 68 x 63 Weight, w/o lens (kg) = 1.01 | Spectral Range = 2.7 - 5.3 ?m Spectral resolution (FWHM) = 35 nm Spectral sampling/pixel = 8.44 nm, Without binning Spectral bands = 154, With default binning Numerical aperture = 2.0 Optics magnification = 0.5 Effective pixel size = 30 ?m, At fore lens image plane Effective slit width = 104 ?m, At fore lens image plane Effective slit length = 19.2 mm, At fore lens image plane Dynamic Range = 1600:1 with 1.5 ms exposure time Usable dynamic range / noise Spatial samples = 640 Bit depth = 16 Maximum frame rate = 380 fps, Full image with default binning Binning = 1,2,4 spectral and spatial, Default: 2 spectral x 1 spatial ROI = Freely selectable multiple bands of interest. Minimum height of ROI is two 1-binned rows. Maximum frame rate is determined by total number of rows between first row of first mROI and last row of last mROI - not the total number of rows included in the mMROI?s. Pixel operability = Number of operable pixels >99.7%. Allowed clusters: Size 4-8 pixels: <= 12/ Size 9-12 pixels: 2/ Size 13-19 pixels: 1/ Size >19 pixels: 0 Image corrections = Non uniformity correction/Bad pixel replacement/Automatic Image Enhancement (AIE). One point NUC. AIE: Unified spectral calibration + corrected smile and keystone aberrations Sensor material = InSb Integrated cooler = Stirling Up to 10000 hours Full well capacity = 5.1 Me- Read-out modes = IWR / ITR Optics temperature = TEC-stabilized Default is 20 degrees Celsius Lens mount = Custom mount Fore lens options = OLEM43, OLEM23, OLEM17 Field of view = 24 deg, 45 deg, 60 deg Camera digital data output/control interface = GigE Vision, Custom ethernet Camera control protocols = GenICam, JSON-RPC Power input = 24 V DC Power consumption = Max 90 W, Typical 40 W, During simultaneous cool-down of optics and detector Connectors = Ethernet/ Aux - 0306423 (09-0428-90-08) Binder 8pin/ Power - 0306627 (LF10WBR-4P) Hirose 4pin Trigger in IP = IP40 Dimensions (L x W x H) = 280 x 202 x 169 mm Mounting surface option on three sides. Mounting kit adds 24 mm distance on mounting side. Weight = 7 kg Storage temperature = -20 ... +50 oC Operating temperature = +5 ... +40 oC Relative humidity = 5% - 95% (non-condensing) | Spectral Range = 950 - 1730 nm Spectral bands = 232 Max speed* = 500 fps Spectral sampling = 3.36 nm Spectral FWHM <2 bands Spatial FWHM <1.5 pixels Spatial pixels = 640 Keystone <20% of a pixel Smile <20% of band FOV = 16? / 40? Bit resolution = 12 bit Noise floor = HG:8.5/MG:32/LG:270 e- Peak SNR = HG:150/MG:275/LG:800 Dynamic range = HG:2650/MG:2360/LG:2360 ROI* = All bands can be selected/deselected individually External trigger options = LVDS, 5V/12V/24V TTL Dimensions (l-w-h) = 364 - 105 - 153 mm Camera Interface = GigE * Reducing the number of spectral channels with ROI will proportionally increase the max framerate |
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