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

SKU: Nireos Hera Iperspettrale VIS-NIR Category: VNIR-SWIR Tag: Mounted

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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 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.

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	Nireos Hera Iperspettrale VIS-NIR remove	HySpex VNIR-3000N remove	HySpex Baldur S-384 N remove	HySpex Mjolnir S-620 remove	HySpex Baldur V-1024 N remove	Specim FX17 remove
Name	Nireos Hera Iperspettrale VIS-NIR remove	HySpex VNIR-3000N remove	HySpex Baldur S-384 N remove	HySpex Mjolnir S-620 remove	HySpex Baldur V-1024 N remove	Specim FX17 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 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 VNIR-3000 N HySpex VNIR-3000 N is developed for field, laboratory, and airborne applications. HySpex VNIR-3000 N utilizes the same spectrograph as the other classical HySpex VNIR models. With a pixel size of 3.45?m, compared to 6. 5?m for VNIR-1800, HySpex VNIR-3000 N will have less than 1.6 pixels per FWHM of the PSF spatially and less than 1.8 bands spectrally, ensuring that narrow band features will be resolved equally for all cameras. With 3000 spatial pixels, 300 bands and a noise floor of 2.4e-, HySpex VNIR-3000N will provide outstanding SNR levels in dark environments. The camera is offered with a USB connection, allowing camera operation from any computer and reducing the cost of supplementing equipment. To visualize that the camera has a wider PSF per pixel and band relative to our normal extremely sharp cameras, we have added an N for Nyquist to the model name.	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 S-620 The HySpex Mjolnir S-620 hyperspectral imaging system for UAVs is the SWIR version of the Mjolnir camera series. Similar to the VNIR version, it 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 4.5 kg and less than 50 W power consumption, HySpex Mjolnir S-620 is very well suited for a wide range of UAVs. NEO offers high-performance unmanned aerial vehicles, fully integrated with the HySpex Mjolnir S-620. 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.	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.	Specim FX17 Specim FX17 hyperspectral camera operates in the near-infrared region and can literally see the invisible. It can reveal the targets? chemical composition, moisture, and foreign objects that are invisible to the human eye. Specim FX17 can, for example, detect different plastic types for recycling and measure the sugar level of fruits and vegetables and the moisture percentage of baked goods.
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 Spatial pixels = 3000 Spectral channels = 300 Spectral sampling = 2.0 nm FOV* = 16? Pixel FOV across/along* = 0.096/0.32 mrad Bit resolution = 12 bit Noise floor = 2.37 e- Dynamic range = 11000 Peak SNR (at full resolution) > 170 Max speed (at full resolution) = 117 fps Power consumption = 30 W Dimensions (l-w-h) = 39 - 9.9- 15 cm Weight = 5.0 kg Camera Interface = USB3 *Can be doubled with FOV expander	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	Spectral range = 970 - 2500 nm Spatial pixels = 620 Spectral channels and sampling = 300 bands @ 5.1 nm F-number = F1.9 FOV = 20? Pixel FOV across/along = 0.54/0.54 mrad Bit resolution = 16 bit Noise floor = 80 e- Dynamic range = 10000 Peak SNR (at full resolution) > 900 Max speed (at full resolution) = 170 fps Power consumption* = 50 W Dimensions (l-w-h)* = 254 - 175 - 170 mm Weight* < 4.5 kg *Includes IMU/GPS and DAU - <5 kg including standard battery	Spectral 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 framerate	Spectral Range = 900-1700 nm Spectral resolution (FWHM) = 8 nm (mean) Spectral sampling/pixel = 3.5 nm Spectral bands = 224 With default binning Numerical aperture = 1.7 With default lens Optics magnification = 0.80 Effective pixel size = 18.7 ?m At fore lens image plane Effective slit width Physical width = 42?m. Projection on sensor = 32 ?m (M=1.3) At fore lens image plane Effective slit length = 12.0 mm At fore lens image plane SNR @ max. signal = 1000:1 Bit depth = 12 Maximum frame rate = 670 (FX17)/ 527 (FX17e) FPS full range Binning = 1,2,4 spectral and spatial Default: 1 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 and the total number of rows included in the mMROI?s. Pixel operability = 99.5%. Allowed clusters: Size 2-6 pixels: N/A/ Size 7-12 pixels: ? 6/ Size 13-19 pixels: ? 2/ Size 20-35 pixels: ? 1/ Size > 35: 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 = InGaAs Sensor cooling = TEC Full well capacity = 1.44 Me- Read-out modes = IWR / ITR Optics temperature = Passive Default is 20 degrees Celsius Lens mount = Custom mount Fore lens FOV options = 12 deg/38 deg (default)/53 deg/66 deg/75 deg/90 deg. Only the default lens is specifically designed for FX17. With other lens options, optical parameters may vary. Camera digital data output/control interface = GigE Vision, CameraLink Camera control protocols = GenICam, ASCII Power input = 12 V DC (+-10%) Power consumption = Max 24 W Connectors = Industrial Ethernet OR CameraLink (standard MDR 26-pin). Power - Fischer 12pin DBPLU1031Z012\|130G IP = IP52 Dimensions (L x W x H) = 150 x 75 x 85 mm Mounting surface option on three sides. Mounting kit adds 24 mm distance on mounting side. Weight = 1.56 kg Storage temperature = -20 ... +50 oC (non-condensing) Operating temperature = +5 ... +40 oC (non-condensing) Relative humidity = 5% - 95% (non-condensing)