First results from todays "Fun with (Ice-) TEA dept.":
So I decided to use the 33120A and the amplifier as the signal source, and the RTB2004, HP34401A as meters for some plausibility checks.
The RTB2004 has a pretty nice feature, one can get its live screen onto a computer just by your favourite browser. The WT1600 has an VGA output that was captured with a grabber device. Finally the 34401A ouput was captured through a simple serial terminal.
This way I have all the interesting readings side by side on the computer screen.
I've started measuring at 100Hz, and stopped at 1.5MHz.
Each step I took a screenshot, like these:
Using human eye powered OCR, I've transferred the interesting measurements into a simple plain text file and made a small graph using gnuplot:
Below maybe 200kHz, I've used the 34401A reading to adjust the 33120A output level, above that the cycle RMS reading from the scope. The scope was connected through a standard 10:1 probe, whose gain error at low frequency (100Hz) was adjusted by fine tuning the scale factor. One can see, the probe isn't perfectly compensated, it drops at 1kHz and peaks at 100kHz a bit.
At the second screen shot (taken at 1.5MHz), one can see the amplifier is at its limits and starts distorting the waveform.
The WT1600 current channel shows 0mA at 100Hz, then 9.24mA at 1.5MHz - this is channel to channel crosstalk due to the high frequency.