Maury MW - Manual Noise Generators - NC6000A-8000A Series
- Additive white Gaussian noise
- Integrated amplifier
- Manual attenuator
- NC6000A -BER testing, and SNR applications
- NC8000A – Secure signal jamming
- Military Applications
- Custom configurations available (consult factory)
The NC6000A and NC8000A Series instruments are designed for general-purpose noise applications on the bench, or in a rack test station. The manual controls make it simple to operate and reduce test set up time. Standard units can be modified for specific customer requirements. Please consult the factory for pricing and availability of these requests.
|
Output |
Attenuator Range |
Impedance |
Typical VSWR |
|---|---|---|---|
|
White Gaussian noise up to 26.5 GHz |
0 to 10 dB in 1 dB steps |
50 Ohms |
1.5:1 |
More Product Information
Safran’s SEEING™ 130 Wide includes a unique medium focal length catadioptric optics, limited by diffraction only and with ultra-low distortion, offering perfect imaging over 35 mm full-frame image format. It is fitted with a 10megapixel sensor.
SEEING™ 130 Wide enables high Signal to Noise Ratio for multispectral (MS), hyperspectral (HS) and low light level imaging. SEEING™ 130 Wide includes a spectral filter with 23 bands covering Blue, Green, Red, Near InfraRed and Red Edge MS, for a broad spectral range between 475 and 900nm. SEEING™ 130 Wide has a large Field of View of 6.3° x 4.3° / 54 x 36 km2 from a 500km/310 miles orbit.
In addition to its a thermal design within a robust structure, SEEING™ 130 Wide has a low SWaP, saving launch and operational costs.
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Camera Link InGaAs SWIR camera
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VGA resolution
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Large pixel with high dynamic
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Strong sensor cooling
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No condensation
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Very strong sensor cooling for low-noise imaging with long exposure times
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Camera Link interface with GenCP support
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Comprehensive I/O control options
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Automated on-board image correction
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Extended operating temperature range
Image optimization features:
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Auto gain (manual gain control: 0 to 32 dB)
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Auto exposure (manual exposure control: 35 µs to 26.8 s)
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Auto white balance (GT4907C only)
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Binning (horizontal and vertical)
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Color correction, hue, saturation (GT4907C only)
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Column defect masking
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Decimation X/Y
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Gamma correction
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Three look-up tables (LUTs)
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Region of interest (ROI), separate ROI for auto features
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Reverse X/Y
Camera control features:
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EF lens control (order option -18)
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Event channel
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Image chunk data
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IEEE 1588 Precision Time Protocol (PTP)
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RS232
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Storable user sets
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StreamBytesPerSecond (bandwidth control)
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Stream hold
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Sync out modes: Trigger ready, input, exposing, readout, imaging, strobe, GPO
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Tap mode switchable in Vimba Viewer 2.0 or later (four-tap, one-tap)
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Temperature monitoring (main board and sensor board)
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Trigger over Ethernet (ToE) Action Commands
Image optimization features:
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Auto gain (manual gain control: 0 to 33 dB)
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Auto exposure (manual exposure control: 15 µs to 26.8 s)
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Auto white balance (GT4905C only)
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Binning (horizontal and vertical)
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Color correction, hue, saturation (GT4905C only)
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Column defect masking
-
Decimation X/Y
-
Gamma correction
-
Three look-up tables (LUTs)
-
Region of interest (ROI), separate ROI for auto features
-
Reverse X/Y
Camera control features:
-
EF lens control (order option -18)
-
Event channel
-
Image chunk data
-
IEEE 1588 Precision Time Protocol (PTP)
-
RS232
-
Storable user sets
-
StreamBytesPerSecond (bandwidth control)
-
Stream hold
-
Sync out modes: Trigger ready, input, exposing, readout, imaging, strobe, GPO
-
Tap mode switchable in Vimba Viewer 2.0 or later (four-tap, one-tap)
-
Temperature monitoring (main board and sensor board)
-
Trigger over Ethernet (ToE) Action Commands
- Complete solution - battery test, simulation & solar array simulator software included
- Highest power density up to 37 kW in 4U rack height (9.25 kW/U)
- Fastest and cleanest power available (fastest transient response and low output ripple and noise)
- Universal 3-Phase AC Input accepts 180 VAC to 528 VAC
- Longest manufacturer-based reliability guarantee: 5-year warranty
- Parallel system power up to 1.2 MW
- Output voltage up to 2,000 V
- Bidirectional output current up to ±150 A, up to ±4,800 A in parallel
- True extended wide-range autoranging output
- Regenerative to 95%
- Color touch panel user interface
- Seamless transition between source and sink
- Built-in islanding detection
- Calibration-grade metrology standards
- Used for VNA calibration and/or calibration validation
Maury mismatch airlines have been designed as verification standards to be used in VNA calibration validation. Each mismatch airline is provided with factory S-parameters data that can be compared with user-measured S-parameters for VNA calibration validation. Measurement uncertainty is also provided, and uncertainty boundaries can be used for definitive calibration validation when used in conjunction with MT940B Insight Real-Time Uncertainty Add-On.
- Automated Absolute and Additive (Residual) Measurements
- Real Time Cross Correlation
- Only analyzer available that allows actual noise floor measurement
- Unparalleled analog performance
- Repeatable data
The HA7162D Real Time Phase Noise Analyzer delivers proven accuracy, high reliability, automation and flexibility. The real time engine covers the full measurement bandwidth with extremely fast measurement speeds to reduce product development time and optimizes ATE manufacturing throughput.
Image optimization features:
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Auto gain (manual gain control: 0 to 32 dB)
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Auto exposure (manual exposure control: 30 µs to 33.5 s)
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Auto white balance (GT6600C model only)
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Binning (horizontal and vertical)
-
Color correction, hue, saturation (GT6600C only)
-
Column defect masking
-
Decimation X/Y
-
Gamma correction
-
Three look-up tables (LUTs)
-
Region of interest (ROI), separate ROI for auto features
-
Reverse X/Y
Camera control features:
-
EF lens control (order option -18)
-
Event channel
-
Image chunk data
-
IEEE 1588 Precision Time Protocol (PTP)
-
RS232
-
Storable user sets
-
StreamBytesPerSecond (bandwidth control)
-
Stream hold
-
Sync out modes: Trigger ready, input, exposing, readout, imaging, strobe, GPO
-
Tap mode switchable in Vimba Viewer 2.0 or later (four-tap, one-tap)
-
Temperature monitoring (main board and sensor board)
-
Trigger over Ethernet (ToE) Action Commands
Thin plate broadband antenna has been developed for efficient immunity testing against hand-held transmitters and cellular phones. Many pieces of spot frequency antennas had to be used in turn thus fur. This new Thin-plate Broadband Antenna is a single antenna solution eliminating the need for antenna changes and dramatically reducing the test time. Furthermore, this antenna with its small-size and lightweight properties and a flexible handle is suitable for testing in narrow spaces.
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A wide frequency range eliminating the need for antenna changes
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30W maximum power input allows high filed strengths
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High efficiency due to a low VSWR and high gain
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Suitable for broadband digital modulation thanks to a good VSWR flatness
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Small, light-weight and flat antenna easy to use in narrow spaces
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Easy handling with a flexible arm
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A wide radiation pattern makes directivity of the fields no longer an issue
Maury Microwave
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Maury Microwave is a pioneering leader in the design and manufacture of precision RF and Microwave calibration, test & measurement, and modeling solutions that are powering global efforts toward a more secure, more connected, future.
Maury Microwave offers Measurement and Modeling Device Characterization Systems and Services including nonlinear passive, active and hybrid-active fundamental and harmonic load pull, non-50Ω X-Parameter modeling, pulsed IV Pulsed s-parameters and compact transistor modeling, and patent-pending ultra-fast/accurate noise parameters.
