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Mini-Circuits Wideband Amplifier 0.1 to 18 GHz

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Features Multiple, independent channels per radio and multiple radios per Access Point that deliver exceptional throughput advantages over convention Access Points 162 Mbps per radio – basic (3-channel) configuration provides over 50x increased throughput performance versus single-channel access points Uses industry-leading, proprietary data converter technology Roving Monitor that acts as a sniffer looking for rogue […]

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WR90 Waveguide and Calibration Kit

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The Agilent DSAX91604A is a 16 GHz real time oscilloscope with 4 analog channels. 256-level intensity-grading emphasizes signal anomalies by lightly-shading infrequent waveforms. Agilent DSA oscilloscopes come with 50 Mpts memory and built-in software (EZJIT, EZJIT Plus, EZJIT Complete, and Serial Data Analysis). The three EZJIT software packages provide jitter analysis capabilities and jitter measurement floor of 100 fs. The equipped Infiniiscan option enables triggering on unique events such as zones on multiple channels and non-monotonic edges. Agilent N5449A High-Impedance Adapters are included for probes that require a 1 MΩ interface.

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Agilent ( Hewlett-Packard) 346B Noise Source, 10 MHz to 18 GHz, Nominal ENR 15 dB

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The Keysight 346B is a general-purpose broadband noise source that eliminates the need for several sources at varying frequencies. Excess noise ratios for each 1 GHz interval from 10 MHz to 18 GHz are printed on the noise source. Low VSWR reduces uncertainty from the reflection of test signals. Useful for noise figure measurements using the Y-factor method.

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Agilent U2002A USB Average Power Sensor

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The Agilent U2002A Average Power Sense offers power analysis up to 24 GHz and outputs from a USB connection. The U2002A is equipped with internal zeroing, preventing the user from having to power-off the DUT or disconnect the sensor between measurements. Calibration, temperature, and linearity correction data has been pre-entered on an internal EEPROM. Triggering can be derived internally from an RF signal or controlled externally via TTL input. The sensor can be rented alone or, if being used for source power calibration, with one of three Keysight PNA network analyzers also available from CMC’s Equipment Rental Program.

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phoo of Keysight U5855A TrueIR Thermal Imager - for temperature measurement up to 350°C

Keysight U5855A TrueIR Thermal Imager – for temperature measurement up to 350°C

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The U5855A is ideal for predictive maintenance activities, from hot spot detection to thermal profiling. With this thermal imager, you get 320×240 Fine Resolution. Ability to magnify the thermal image of a far‑away object by 4 times to reveal finer details and quickly spot problems. Also, take thermal images of close-fit or minute components from as close as 10 cm away clearly and accurately.

The U5855A also comes with a variety of measurement and analysis tools to help you monitor temperature over time, do min and max temperature tracking and more so that you can easily obtain heat patterns, dissipation and etc. The U5855A comes with a built-in quick start tutorial to help you get familiar with thermal imager quickly.

What’s more, with the complimentary TrueIR Analysis and Reporting Tool, you can easily import, analyze and edit thermal images and quickly generate reports using ready templates. You can also display thermal images, visual images or thermal-visual images side-by-side for further analysis.

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Agilent (Hewlett-Packard) 8970B Noise Figure Meter

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The Agilent 8970B makes noise figure measurements in the 0 to 30 dB range. Measured noise can be displayed as noise figure or equivalent input noise temperature. Excess Noise Ratio (ENR) data can be entered in data tables on the noise figure meter. The meter uses this information to correct for ENR vs. frequency variations. The 8970B can be used with Agilent 346 (CMC loans the Agilent 346B Solid State Noise Source separately) or 347 noise sources.

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Agilent 87405A Preamplifier, 10 MHz to 3 GHz

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The 87405A Preamplifier is a multi-purpose instrument for any application that requires low noise and additional gain. The SNR of the final signal in an RF system is greatly impacted by the initial amplification of the signal and its original SNR. By having low noise figure in a preamplifier, the final signal will have a lower noise than without the preamplifier.

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