Nireos Hera Iperspettrale Extended SWIR

Nireos Hera Iperspettrale Extended SWIR

Spectral range = 900 – 2300 nm
Sensor spatial resolution = 320 x 256 pixels
User adjustable spectral resolution: < 5 nm @ 900 nm/ <30 nm @ 2300 nm Detector type = T2SL photodiode array with CTIA ROIC, 4-stage TE cooler Number of bits = 14 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view 16 degrees Working distance = 110 cm - ? Dimensions = 240 x 170 x 120 mm Weight = 5 kg Minimum Computer Requirements = 16 GB RAM, SSD drive suggested * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement

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HERA IPERSPETTRALE is a compact and rugged camera that enables an innovative approach to spectral imaging.
With its unique and patented technology based on time-domain Fourier Transform (FT) detection, HERA provides exceptional spatial-spectral resolution and superior sensitivity in low-light illumination conditions.
HERA is based on a Fourier Transform (FT) approach: the data-cube is acquired in the time-domain, by step-scanning a compact ultra-stable interferometer in front of the bidimensional sensor.
The software then automatically computes an FT at each and every pixel of the image, providing the final hyperspectral data-cube.
As a result of an FT, the spectrum at each pixel is a continuous curve, so the number of bands is virtually unlimited, not defined by the hardware.
As in any other FT techniques, the spectral resolution is not constant as a function of the wavelength. Also, the spectral resolution can be simply varied via software: at each measurement, you can decide whether to acquire a high spectral resolution-image, or – if not required – a faster and lower spectral resolution-image.
Regardless of this choice, the exceptional light throughput is not affected, thanks to the FT approach.

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ContentHERA IPERSPETTRALE is a compact and rugged camera that enables an innovative approach to spectral imaging. With its unique and patented technology based on time-domain Fourier Transform (FT) detection, HERA provides exceptional spatial-spectral resolution and superior sensitivity in low-light illumination conditions. HERA is based on a Fourier Transform (FT) approach: the data-cube is acquired in the time-domain, by step-scanning a compact ultra-stable interferometer in front of the bidimensional sensor. The software then automatically computes an FT at each and every pixel of the image, providing the final hyperspectral data-cube. As a result of an FT, the spectrum at each pixel is a continuous curve, so the number of bands is virtually unlimited, not defined by the hardware. As in any other FT techniques, the spectral resolution is not constant as a function of the wavelength. Also, the spectral resolution can be simply varied via software: at each measurement, you can decide whether to acquire a high spectral resolution-image, or - if not required - a faster and lower spectral resolution-image. Regardless of this choice, the exceptional light throughput is not affected, thanks to the FT approach.Pika L 400 - 1000 nm Lightweight, Compact VNIR The Pika L is a lightweight, compact hyperspectral camera that covers the Visible + Near-Infrared (VNIR) spectral range. It is our most popular imager for remote sensing applications. The Pika L can be used in our airborne, laboratory, and outdoor hyperspectral systems, as well as standalone or integrated into your system.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.HySpex Baldur V-1024 N Baldur V-1024 N covers the full VNIR spectral range from 400-1000nm and is configurable within one octave in the same range. 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 V-1024 N is better than 1.7 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.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.
DescriptionSpectral range = 900 - 2300 nm Sensor spatial resolution = 320 x 256 pixels User adjustable spectral resolution: < 5 nm @ 900 nm/ <30 nm @ 2300 nm Detector type = T2SL photodiode array with CTIA ROIC, 4-stage TE cooler Number of bits = 14 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view 16 degrees Working distance = 110 cm - ? Dimensions = 240 x 170 x 120 mm Weight = 5 kg Minimum Computer Requirements = 16 GB RAM, SSD drive suggested * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurementSpectral Range (nm) = 400 - 1000 Spectral Channels = 281 Spectral Bandwidth (nm) = 2.1 Spectral Resolution - FWHM (nm) = 3.3 Spatial Pixels = 900 Max Frame Rate (fps) = 249 f/# = 2.4 Interface = USB 3.0 Dimensions (mm) = 115 x 104 x 66 Weight, w/o lens (kg) = 0.64Spectral 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) = 2.27Spectral Range = 400-800/485-960/400-1000 nm Spatial pixels = 1024 Spectral bands = 72/88/106 Max speed* = 1000/800/700 fps Spectral sampling = 5.5 nm Spectral FWHM <2 bands? Spatial FWHM < 1.7 pixels Keystone <15% of a pixel Smile <15% of band FOV = 16? / 40? Bit resolution = 12 Noise floor = 11e Peak SNR >286 Dynamic range = 2560 ROI* = 8 independent ROIs Dimensions (l-w-h) = 316 - 105 - 153 mm Camera Interface = CameraLink * Reducing the number of spectral channels with ROI will proportionally increase the max framerateSpectral 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)
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