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 CMOS 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.
Thanks to the absence of aperture slits and gratings, and to the 1 cm Clear Aperture, HERA is specifically designed to provide an extremely high light throughput, making it the ideal device for low light conditions or delicate samples.
Nireos Hera Iperspettrale VIS-NIR
VNIR-SWIR Compare
Nireos Hera Iperspettrale VIS-NIR
Spectral range = 400 – 1000 nm
Sensor spatial resolution = 1280 x 1024 pixels
User adjustable spectral resolution: <1.5 nm @ 400 nm/ <10 nm @ 1000 nm
Sensor = CMOS
Number of bits = 12 bits
Software interface = Labview based interface
Number of spectral bands = ?*
Field of view 8 degrees**
Working distance = 1 m - ?
Dimensions = 205 x 150 x 83.5 mm
Weight = 2 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time
** The Field of View can be doubled (up to 16 degrees) by adding an optional lens in front of the camera
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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 CMOS 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. Thanks to the absence of aperture slits and gratings, and to the 1 cm Clear Aperture, HERA is specifically designed to provide an extremely high light throughput, making it the ideal device for low light conditions or delicate samples. | 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 AFX10 Specim AFX10 is a VNIR hyperspectral imaging solution with an HSI camera, a small and powerful computer and a high-end GNSS/IMU unit in a compact enclosure that can be installed on multiple drone types. | 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. | 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. | Fenix FENIX is optimized for the most demanding geological, law enforcement, and environmental applications. In a single continuous image, FENIX spectral camera delivers the best hyperspectral data ever seen over VNIR, NIR, and SWIR wavelengths. FENIX offers extreme ruggedness and 75% reduction in size and weight compared to previous multi-sensor systems. The excellence in technical performance and physical size has been achieved through innovative and unique ?single optics dual spectrograph? design. |
| Description | Spectral range = 400 - 1000 nm Sensor spatial resolution = 1280 x 1024 pixels User adjustable spectral resolution: <1.5 nm @ 400 nm/ <10 nm @ 1000 nm Sensor = CMOS Number of bits = 12 bits Software interface = Labview based interface Number of spectral bands = ?* Field of view 8 degrees** Working distance = 1 m - ? Dimensions = 205 x 150 x 83.5 mm Weight = 2 kg * HERA is FT spectroscopy based instrument and number of spectral bands is software selectable and independent from measurement time ** The Field of View can be doubled (up to 16 degrees) by adding an optional lens in front of the camera | Spectral Range = 400 - 1000 nm Spectral sampling = 2.68 nm Spectral resolution = 5.5 nm Fore lens focal length = 15 mm Field of view = 38 deg F/# = 1.7 Spectral bands = 224 Binned by 2 Spatial pixels = 1024 Spectral binning options = 2, 4, 8 Spatial binning options = 1, 2 Multiple ROI = User-selectable Maximum frame rate = 330 fps Full frame Dynamic range = 1420 SNR = 400:1 2 spectral binning, 1 spatial binning Power input = 10-30 VDC. Use separate battery or UAV/gimbal power Power consumption = 17 W Typical Connectors = ANT, DC IN, ETH GPS Antenna, Power In, Web UI / Data download Storage temperature = -20 ? +50C Operating temperature = +5 ? +40C Relative humidity = 5 - 90 %. Non-condensing Drone options = Multirotor with gimbal/ Multirotor, no gimbal/ Fixed Wing UAV. Any drone with adequate payload capacity can be used. Gimbal = Optimized for MoVI pro. Other suitable gimbals may also be used Gimbal weight = 2.2 - 2.7 kg. Typical gimbal solution Operating height = 15 - 150 m. Typical, local limitations may apply GNSS/IMU = Trimble APX-15 GPS Antenna = Trimble AV 14 Internal Memory = 512GB SSD Dimensions (W x H x L) = 131 x 152 x 202 mm Weight (without gimbal) = 2.1 kg Weight (with gimbal) = 4.8 kg. Typical gimbal solution | 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 (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) = 0.64 |
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