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

- Boost performance by up to 3x over its precursor thanks to an Intel x6000 series embedded processor
- Capture high-resolution images at high speed through a choice of CMOS sensors from two to 16 Megapixels
- Deploy in dirty, humid, or harsh industrial environments by way of a compact IP67-rated design
- Communicate actions and results to other automation and enterprise equipment via real-time digital I/Os, and Ethernet (TCP/IP, CC-Link IE Field Basic, EtherNet/IP™2, Modbus® , PROFINET® , and native robot interfaces)
- Handle Human-Machine Interface (HMI) function by way of VGA and USB connectivity
- Simplify vision setup and upkeep via integrated lens focusing and illumination intensity control
- Synchronize to the manufacturing line through the support for incremental rotary encoders
- Solve machine vision applications efficiently with Aurora Design Assistant by constructing flowcharts instead of writing program code
- Maintain control and independence through the ability to code custom flowchart steps
- Tackle machine vision applications with utmost confidence using field-proven tools for analyzing, locating, classifying, measuring, reading, and verifying
- Leverage deep learning for visual inspection through image classification and segmentation tools

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Quick and easy probe tip navigation
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Z drive can work in the same range as the chuck
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Enables higher separation gap while the DUT stays in focus
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Automatically configure and optimize performance
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24/7 operating
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Increased MTBF
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Protects the measurement setup
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Prevents involuntary mechanical contact between lens and probes


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Type APS-H CMOS sensor
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IEEE 1588 PTP
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Power over Ethernet
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4.59 fps at full resolution
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Monochrome (GT5120) model
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GigE Vision interface with Power over Ethernet
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Screw mount RJ45 Ethernet connector for secure operation in industrial environments
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Supports cable lengths up to 100 meters (CAT-6 recommended)
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Trigger over Ethernet Action Commands allow for a single cable solution to reduce system costs
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Comprehensive I/O functionality for simplified system integration
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Planarity adjusted (PA) EF Lens Mount (option -18) for electronic control of aperture and autofocus
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Easy camera mounting via standard M3 threads at all sides and 1/4-20 tripod mounting hole
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Easy software integration with Allied Vision's Vimba Suite and compatibility to the most popular third party image-processing libraries.
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Enhanced Defect Pixel Correction feature with a new Defective Pixel List Manager tool that allows you to load different user defined defective pixel lists to match your application and optimize the life cycle of the camera

- Tiny “all-in-one” solution: no external control board needed
- Superior image quality: sub-micron lens movement with very low tilt. Now with higher dynamic stability
- Low voltage & power: 3.3 VDC input, zero power position hold
- Simple system integration: accepts high-level motion commands over standard serial interface (I2C or SPI)
- Flexible, production-ready system: compatible with M8 to M16 lenses and with typical image formats from 1/3” to 1/1.8”
- Lowest cost, fastest time to market: Fully-engineered “plug and play” solution

- Reduced dark noise levels and improved dark offset
- Improved sensitivity, including NIR response
- In-camera image pre-processing (lens shading correction, pixel correction)
- Large full well when using in-sensor binning >142Ke
- Thousands of frames per second in Partial Scan Mode (ROI)
- Multi-ROI support (up to 32 ROI) and Cycling Mode
- Advanced Sequencer functions of different features

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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

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From 100MHz to 120GHz we use the slide screw technique in which a reflective probe is inserted into a low loss slotted transmission line.
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For frequencies from 10MHz to 170MHz we use a lumped element technology, whereby variable capacitors are connected with optimized lengths of coaxial cable. To view our Low Frequency Tuners, Click Here!

Noise measurements allow the determination of the four Noise Parameters of a device (transistor). There are four Noise Parameters which fully describe the noise behaviour of an active or passive device at a given frequency.

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
Test & Measurement
