The GigaTrack™ family of 2-GS/s track-and-hold amplifiers (THA) from Inphi® Corp. (Westlake Village, CA) delivers ultra-wide 18-GHz analog bandwidth.

The bandwidth, sample rate, and linearity make direct conversion and software-defined receivers possible, and help advance highsample- rate test and measurement equipment. The GigaTrack amplifiers operate from a single -5.2 V power supply and dissipates 1.3 W. They are available in a 49-pin ceramic ball-grid array and in 24-pin QFN packages. The devices are designed for engineers designing next-generation instrumentation, ATE, and military equipment. They enable engineers to replace numerous components in heterodyne receiver architectures with a track-and-hold and a high-samplerate ADC. A direct conversion receiver can serve multiple applications with system differentiation occurring in software or firmware. The GigaTrack family consists of four track-and-hold amplifiers with 2-GS/s sample rates. The ball-grid-array versions offer 18-GHz (small signal) and 15-GHZ (0.5V pp) input analog bandwidths, with settling times >60 ps and power consumption of 1.3 W. Plastic QFN versions offer 13-GHz analog bandwidth (100mV pp).

To deliver a wider hold time window for the downstream ADC, a master/ slave (dual) track-and-hold architecture was developed, increasing the hold time window to almost one full cycle of the THA. For users who want to sub-sample the output of the master track-and-hold with the slave trackand- hold, the 1821TH and 1321TH devices provide a flexible clock mode select pin that, in one mode, allows the user to provide different clocks to the master and slave track-and-holds. The devices feature total harmonic distortion of -70 dB typical at 1 GHz and 500 mV pp input, and aperture jitter <50 fs. By eliminating the need for two separate power supply voltages, the devices reduce power consumption.

For Free Info Click Here 



Magazine cover
Embedded Technology Magazine

This article first appeared in the November, 2006 issue of Embedded Technology Magazine (Vol. 30 No. 11).

Read more articles from the archives here.