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.
Nireos Hera Iperspettrale SWIR
SWIR Compare
Nireos Hera Iperspettrale SWIR
Spectral range = 900 – 1700 nm
Sensor spatial resolution = 640 x 512 pixels
User adjustable spectral resolution: < 5 nm @ 900 nm/ <20 nm @ 1700 nm
Sensor = cooled InGaAs (?T = 30?)
Number of bits = 14 bits
Software interface = Labview based interface
Number of spectral bands = ?*
Field of view = 11 degrees
Working distance = 1 m - ?
Dimensions = 220 x 160 x 105 mm
Weight = 2.85 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time
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| Nireos Hera Iperspettrale SWIR remove | Resonon Pika UV remove | HySpex Mjolnir VS-620 remove | HySpex VNIR-1800 remove | Specim FX10+ remove | Specim FX50 remove | |
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| Content | 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. | 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 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 VNIR-1800 The HySpex VNIR-1800 hyperspectral camera is developed for field, laboratory, and airborne applications. HySpex VNIR-1800 utilizes a cutting edge actively cooled and stabilized scientific CMOS detector. This makes VNIR-1800 the ideal camera for high-end data acquisitions where high radiometric accuracy is required. The dynamic range of 20 000 ensures outstanding SNR levels even in darker areas of an image of highly dynamic scenes. With a max frame rate of 260 fps, combined with aberration-corrected optics and high optical throughput (f/2.5), HySpex VNIR-1800 offers a unique combination of data quality, high speed, and sensitivity. A wide range of close-up lenses allows the use of the camera at working distances ranging from a few centimeters with a spatial resolution of 24 ?m to infinity e.g. airborne remote sensing. | Specim FX10+ The Specim FX10+ is a high-speed line-scan hyperspectral camera optimized for applications requiring fast imaging. Its high resolution ensures accurate and detailed imaging at a rapid pace. Specim FX10+ operates in the visible and near-infrared (VNIR) region from 400 to 1000 nm. | 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. |
| Description | Spectral range = 900 - 1700 nm Sensor spatial resolution = 640 x 512 pixels User adjustable spectral resolution: < 5 nm @ 900 nm/ <20 nm @ 1700 nm Sensor = cooled InGaAs (?T = 30?) Number of bits = 14 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view = 11 degrees Working distance = 1 m - ? Dimensions = 220 x 160 x 105 mm Weight = 2.85 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time | 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 = 400 - 1000 nm Spatial pixels = 1800 Spectral channels = 186 Spectral sampling = 3.26 nm FOV* = 17? Pixel FOV across/along* = 0.16/0.32 mrad Bit resolution = 16 bit Noise floor = 2.4 e- Dynamic range = 20000 Peak SNR (at full resolution) > 255 Max speed (at full resolution) = 260 fps Power consumption = 30 W Dimensions (l-w-h) = 39 - 9.9 - 15 cm Weight = 5.0 kg Camera Interface = CameraLink *Can be doubled with FOV expander | Spectral Range = 400-1000 nm Spectral resolution (FWHM) = 15 nm, Typical mean Spectral sampling/pixel = 6.3 nm, With default binning Spectral bands = 100, With default binning Numerical aperture = 1.7, With default lens Optics magnification = 0.80 Effective pixel size = 19.9x9.97 ?m, At fore lens image plane Effective slit width = 42 ?m, At fore lens image plane Effective slit length = 10.2 mm, At fore lens image plane SNR @ max. signal = 420 : 1 Spatial samples = 1024 Bit depth = 12 Maximum frame rate = 705 FPS full range. With 2-spectral binning (Bands: Max FPS) = 1:9900/5:6500/20:2800/35:1813/70:985 Binning = 2,4,8 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 the total number of rows included in the mMROI?s Pixel operability = 99.993% Image corrections = Non uniformity correction/Bad pixel replacement/Automatic Image Enhancement (AIE). AIE: Unified spectral calibration + corrected smile and keystone aberrations. One point NUC Sensor material = CMOS Sensor cooling = Passive Full well capacity = 90 ke- Read-out modes = IWR / ITR Optics temperature = Passive Lens mount = Custom mount Fore lens FOV options:12 deg/38 deg (default)/47 deg/51 deg/83 deg. Only the default lens is specifically designed for FX10. With other lens options, optical parameters may vary. Camera digital data output/control interface = GigE Vision Camera control protocols = GenICam, ASCII Power input = 12 V DC (+-10%) Power consumption = Max 4 W Connectors = Industrial Ethernet IP = IP52 Dimensions (L x W x H) 150 x 85 x 71 mm Mounting surface option on three sides. Mounting kit adds 24 mm distance on mounting side. Weight 1.3 kg Storage temperature = -20 ... +50?C (non-condensing) Operating temperature = +5 ? +40?C (non-condensing) Relative humidity = 5% - 95% (non-condensing) | 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) |
