Category Archives: Amplifiers

Power Handling

Maximum power handling is a common concern of our customers. Nothing is worse than plugging in an expensive device only for it to be immediately destroyed. Understanding power handing is important to us as well so that we can address customer concerns about reliability and to develop devices that are able to tolerate higher power levels. The purpose of this document is to describe the failure mode and maximum power handling of several Marki Microwave product lines. It lists the power required to destroy the device and describes what part of the device fails at that power.

An Introduction to Microwave Amplifiers Part 1: Microwave Amplifier Applications

types-of-microwave-amplifiers

This is a (virtually) math-free introduction to microwave amplifiers from an applications standpoint. There are many references available for the aspiring amplifier designer; this series of posts will attempt to quickly elucidate the relevant factors for the RF system design engineer working to evaluate the appropriate amplifier for her system design.

Types of Microwave Amplifiers

types-of-microwave-amplifiers

There are many ways to classify microwave amplifiers, but we will group them into four categories based on what role they would play in a generic superheterodyne receiver (shown above). The above system could represent a cellular, backhaul, satellite, or other radio communications link; it could also represent a radar or other imaging system. The transmitter alone could represent a jammer or exciter, and the receiver alone could represent an electronic warfare scanner or a test instrument. The requirements that drive the amplifier selection will be the same for most applications.

Driving Doublers with Amplifiers

Frequency multipliers are used to generate higher harmonics from an input sinusoid.  In particular, the job of the doubler is to output only the 2nd harmonic.  Invariably, the fundamental tone and higher harmonics will leak to the output as well; how much lower the power of these tones are compared to the 2nd harmonic is known as their “suppression”.

Doublers generally require a large input signal (greater than 12 dBm) to work properly.  To reduce stress on your signal generator, you might consider feeding a smaller signal into an amplifier, and using the amplifier to drive the doubler.  Unfortunately, you will observe that the suppressions of the fundamental and 3rd harmonic are much worse with the amplifier attached.  What happened?  Why should the amplifier make a difference?
doubler_graphs1

Marki Microwave Amplifier Operation Guide

We sell a large product line of packaged amplifiers, primarily for use as LO buffer amplifiers, but that can also be used as general purpose gain blocks. While we don’t design the actual amplifier chips, our expertise is in selecting and packaging these chips to provide easy and guaranteed performance from very low (kHz) to microwave frequencies. Amplifiers can be tricky to deal with, since they generate a large amount of RF power and heat, and use MMIC amplifier chips that can break when not used properly. Here are some guidelines for using Marki Microwave amplifiers:

  • Always bias the negative port first: This is because the negative voltage is required to pinch off the gate voltage and ensure that the positive current is limited. If the negative voltage is removed the positive current will flow unimpeded, causing the amplifier to heat up until it burns. This is the easiest way to break a Marki amplifier.
  • Only operate the amplifier with a matched load on the output: If the amplifier is run with the output open or shorted, the power has no place to go, and the reflected power may (or may not) burn out the chip. In fact, if you are performing an experiment where the circuit might open or short then measures must be taken to protect the amplifier from the reflection, such as adding an attenuator or circulator.
  • Obey the datasheet levels for input power: Providing too much input power will cause the amplifier to clip excessively, and may cause damage.
  • Provide some type of heat sinking: Our connectorized amplifiers will operate properly in a room temperature environment with just cabling to remove the heat. If in a heated environment the amplifier will need some way to dissipate heat. For surface mount units make sure that the ground pad has sufficient heat sinking capability to a good chassis or case.

In addition to these precautions to avoid damage, there are some further considerations to optimize performance of the amps:

  • For linear operation, input to the amplifier should be below around -15 dBm. This is variable with the gain of the amp, but typically non-linear saturation effects occur around this level. These can be seen with an oscilloscope as clipping of a sine wave, or on a spectrum analyzer as creation of harmonic products (particularly odd harmonics).
  • For square wave operation, such as for driving a T3, drive the amplifier at the minimum recommended input power level to ensure clipping and good square wave generation. This can also be seen on an oscilloscope. For T3 optimization the desired goal is to minimize the rise/fall time of the signal.

Do microwave signal amplifiers add flicker (1/f) noise?

Phase noise, and amplifier noise in particular, has been a pet project of Ferenc’s for some time. This stems from the fact that, as I will detail in a future post, a passive silicon schottky diode mixer adds very little noise. Normally when customers find excess noise on a conversion it is because of LO noise transmitting to the IF/RF output. We found a recent article called “Phase Noise in RF and Microwave Amplifiers”, by Rodolphe Boudot and Enrico Rubiola (IEEE Trans. Ultrasonics, Ferroelectrics, and Frequency Control, vol. 59, no. 12, Dec. 2012) where they show plots of phase noise of an oscillator after amplification with different output powers. We decided to perform the same measurement. In our experiment we take a reference 80 MHz oscillator (a Wenzel low phase noise crystal) and measure the phase noise. Then we attenuate the signal by 50 dB and amplify it back up by 50 dB. The input noise floor is at -159.4 dBm/Hz, and the output is at 106.5 dBm/Hz. The noise floor increase is as a result of the amplification and noise figure of the amplifier. The phase noise plots are show below, along with an extra line showing the phase noise of the oscillator with a constant noise level equal to the noise floor of the amplifier added to it.

As you can see, there is very little difference between the phase noise of the amplified signal and the phase noise of the oscillator with white noise added to it. Hence the question, do amplifiers add flicker noise? In the frequency range near the carrier we see hardly any noise addition. This suggest that at a minimum, the flicker noise addition for the amplifier we used (a Centellax wideband amplifier similar to our T3 driver amps) is very low. So low that it’s hard for us to believe that it adds flicker noise at all.