| Content | OCI?-1000 series VIS-NIR hyperspectral imaging cameras are extremely compact, light, and rugged. They cover visible - near-infrared (VIS - NIR) spectral range from 470 - 1000 nm. Unlike conventional hyperspectral imagers which rely on intensive software effort on hyperspectral image cube construction, the innovative design of the OCI?-1000 series imagers feature true push broom and ultrafast data transfer rates, with automatic data capturing and processing, they can move to scan at random speeds. The elegant completely integrated design and manufacturing in our quality certified production facility with master quality control to deliver high precision, superb signal-to-noise, excellent spectral & spatial resolution, and outstanding imaging quality. With the free packed operation software, OCI? - 1000 series hyperspectral cameras are automatic and minimum human intervention. They are ideally catered to various unmanned aerial vehicles/systems (UAV/UAS) and remotely operated vehicles (ROV). BaySpec also provides ready-to-fly hyperspectral solutions. Extreme compactness with uncompromised performance, automatic operation and data processing makes the OCI-UAV a straightforward system for board fields applications such as precision agriculture, geological survey, oceanography, remote sensing, security/defense, and anti-counterfeiting. | Pika UV
330 - 800 nm
Ultraviolet + Visible
The Pika UV (formerly NUV2) is a hyperspectral camera that scans the Visible and Near Ultraviolet (VIS+NUV) spectral range. An optimized objective lens provides excellent imaging throughout the entire spectral range.
Because halogen lights have low output in much of the NUV, Resonon offers an NUV lighting module to augment illumination for our desktop system.
The Pika UV can be used in our airborne, laboratory, and outdoor hyperspectral systems, as well as standalone or integrated into your system. | 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-384 N
Baldur S-384 N covers the spectral range from 960-2500 nm.
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-384 N is better than 1.5 pixels, yielding a very sharp camera. | HySpex Mjolnir VS-620
For applications requiring low mass, combined with high-performance specifications and scientific grade data quality on the full VNIR-SWIR range, HySpex Mjolnir VS-620 is an ideal solution. Sharing the onboard data acquisition unit and navigation system, HySpex Mjolnir VS-620 is both space-efficient and cost-effective.
The VNIR and SWIR optical axis are coaligned in the along-track direction, assuring perfect coregistration in the flight direction. In addition to the high-quality hyperspectral data cube, covering the spectral range from 400 - 2500 nm, with 490 bands, double resolution data in the VNIR range is always readily available. With smile and keystone less than 0.1 pixels for each spectral range, the merged Mjolnir VS-620 data product will have coregistration/keystone better than 0.2 pixels for the full VNIR-SWIR range. | 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 = 600 - 1000 nm
Spectral Resolution = 5 nm FWHM
Number of Spectral Bands = 150
Frame Rate = 120 frames/sec
Dimension = 3 x 3 x 3 cm3
Weight = 45.3 g | Spectral Range (nm) = 330 - 800
Spectral Channels = 255
Spectral Bandwidth (nm) = 1.8
Spectral Resolution - FWHM (nm) = 2.8
Spatial Pixels = 1500
Max Frame Rate (fps) = 142
f/# = 2.8
InterfaceUSB = 3.0
Dimensions (mm) = 230 x 107 x 85
Weight, w/o lens (kg) = 2.27 | 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 = 960 - 2500nm
Spectral bands = 288
Max speed* = 500 fps
Spectral sampling = 5.45 nm
Spectral FWHM <2 bands
Spatial FWHM <1.3 pixels
Spatial pixels = 384
Keystone <15% of a pixel
Smile <15% of band
FOV = 16? / 40?
Bit resolution = 16 bit
Noise floor = 150 e-
Peak SNR >1100
Dynamic range = 7500
ROI* = All bands can be selected/deselected individually
External trigger options LVDS, 5V/12V/24V TTL
Dimensions (l-w-h) = 368 - 131 - 175 mm
Camera Interface = CameraLink
* Reducing the number of spectral channels with ROI will proportionally increase the max framerate | | |
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