Focus Microwaves - Noise Modules
of the cold-source noise figure measurement technique. This specific technique requires a noise source to determine the kBG (gain-bandwidth constant) of the system and a passive mechanical tuner is used to characterize the noise receiver across both the impedance and frequency space. This step is imperative to obtain fully vector-source-corrected measurements.
A RF down conversion stage might be required if the frequency of noise measured exceeds the receiver’s bandwidth. Focus offers noise modules which support down conversion for optimal speed and performance.
Hardware
Noise Measurement System
Model | Frequency | Insertion Loss | VSWR | Min. Gain | Max. VSWR | Connector |
NMS-2600 | up to 26.5 GHz | 0.80 dB | 1.61 | 29 for 0.8-26.5GHz | 1.8:1 | 3.5mm |
NMS-4000 | up to 40 GHz | 0.91 dB | 1.81 | 30 for ≤26.5GHz, 29 for 26-40GHz | 2.1:1 | 2.9mm |
NMS-5000 | up to 50 GHz | 0.99 dB | 1.8:1 |
27 for ≤26.5GHz, 27 for 26-40GHz, 28 for 40-50GHz |
2:1 | 2.4mm |
NMS-6700 | up to 67 GHz | 1.12 dB | 1.91 |
29 for ≤26.5GHz, 28.5 for 26-40GHz, 28 for 40-50GHz, 21 for 50-65GHz |
3:1 | 1.85mm |
NMS-6700-DC* | up to 67 GHz | 1.12 dB | 1.9:1 |
29 for ≤26.5GHz, 28.5 for 26-40GHz, 28 for 40-50GHz, 37 for 50-65GHz |
3:1 | 1.85 mm |
NMS-75500-DC* | 50 to 75 GHz | 0.4dB | 1.2:1** | 40 for 50-75GHz | 1.6:1** | WR-15 |
NMS-90600-DC* | 60 to 90 GHz | 0.9dB | 1.3:1** | 35 for 60-90GHz | 1.8:1** | WR-12 |
NMS-110750-DC* | 75 to 110 GHz | 1.1dB | 1.3:1** | 36 for 75-110GHz | 1.9:1** | WR-10 |
NMS-1701100-DC* | 110 to 170 GHz | 1.3dB | 1.4:1** | 36 for 110-170GHz | 2:1** | WR-6.5 |
* with Downconverter
** +/-10%
Graphs
Noise Parameters
Noise Circles & Stability Regions
Noise Parameters: Minimum Noise Figure / Rn / Gamma Opt / Phase of Gamma Opt
Setup
More Product Information
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Low running costs, less vibration, less noise, reduced maintenance
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Large convenient experimental access: Up to 12 line-of-sight ISO100 ports located on perimeter of plates
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CMN calibrated thermometry on MC plate
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Operation via touch panel controller: Remote operation via ethernet interface
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Network Enabled Distribution Amplifier
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Low Phase Noise Reference Frequency Outputs
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Fault Alarm Output
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1U 19″ Rack Mount
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Frequency Synthesizer Option
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Hitless Switching of Reference
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Programmable Amplitude
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Propagation Delay Compensation
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10 MHz Standard, Other Frequencies Available
The low frequency tuners are a unique product technology using MPT algorithms for low frequency wideband tuning. Three or more cascaded tuning sections use series transmission cables and parallel rotary capacitors.
The length of the cables and number of tuning sections are optimized for maximum tuning range over a given bandwidth. HLFT tuners use 6 tuning sections allowing second harmonic frequency tuning.
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Auto gain (manual gain control: 0 to 22 dB)
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Auto exposure (manual exposure control: 100 µs to 1 s, 1 µs increments)
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Binning (horizontal and vertical) (sum)
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Decimation X/Y
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Enhanced Defect Pixel Correction (DPC)
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Fixed Pattern Noise Correction (FPNC)
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Gamma correction
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Three look-up tables (LUTs)
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Region of interest (ROI)
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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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Temperature monitoring (main board and sensor board)
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Trigger over Ethernet (ToE) Action Commands
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3 isolated low phase noise 10MHz outputs
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Internal GPS Tracking Receiver
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External 1 PPS input
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Small footprint designed for easy integration
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Disciplined high stability OCXO
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Low Noise
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Excellent line/load regulation
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Remote sense
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Coarse and fine voltage controls
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Constant voltage or constant current operation with automatic crossover and mode indication
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Individual On/Off switch per output (not including fixed output)
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Variable ( 1.5V to 5V ) Auxiliary Output
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Shrouded socket-compatible with bare wire and shrouded safety plug connections up to 4 mm
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Fiber coupled to allow easy movement
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Ultra-broadband measurement
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Transmitted or reflected data collection
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Mates with collinear adapter (AXA40n1)
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High signal to noise ratio
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Hot swappable with other transmitters
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Low noise to enable rapid data collection
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Adjustable lens tube for focusing
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Multiple lenses available
Probing with long leads or accessories is sometimes necessary to reach the test points, but it comes at the expense of reduced bandwidth, increased capacitance, and added noise. The ZD accessories are engineered to provide the best signal fidelity without ringing or distortions commonly introduced with tip accessories.
Focus Microwaves
Focus Microwaves is a pioneering engineering company, built around the innovations of its founder Dr. Christos Tsironis who developed his first manual tuner in 1973 and is the inventor of most existing electro-mechanical tuner families. The success of Focus is based on the engineering and manufacturing skills of its highly motivated and experienced team of engineers and technicians, who have been trained and encouraged to develop new technologies. In addition, listening to our customers needs and insights helps us discover and develop new and measurement methods on an ongoing basis, relentlessly pushing the limits of what is possible.
From humble beginnings in 1988, Focus has become the main supplier of advanced Load Pull and Noise Tuner Systems. Our mission is to provide effective, reliable and innovative solutions for non-50 Ohm testing (Noise and Load Pull) of RF microwave transistors, thus enabling our customers to compete in the marketplace with better designs and to advance the understanding and knowledge of the field.
Contact Details
Focus Microwaves Inc. Main Head Office
4555 Chem. du Bois-Franc, Saint-Laurent, QC H4S 1A8, Canada
Phone: +1-514-684-4554