Table of Contents
1. ACM Front Panel 2. ACM Module 3. Close-up view 4. ACM Waveform
Working our way down the front panel, we have the following LEDs and connectors:
These five connectors (I/O 1 through I/O 5) are jumper-configurable to act either as inputs to the TIMER chip, or can be outputs. One likely use will be to activate additional shutters or actuate deployable corner-cube prisms within the telescope.
A view of the ACM board, installed in its mechanical housing that slides into the CAMAC crate. The board itself is an 8-layer design, with generous ground planes and minimal signal-line overlap. From left to right are:
A view of the business-end of the ACM board. From top to bottom are:
This oscilloscope trace shows two of the ACM outputs. The wider pulse is the APD gate request (GTE), lasting 100 ns (this is tunable in multiples of 20 ns). (See the front panel description for definition of signals.) The shorter pulse tucked within the last bit of the gate pulse is the gate-close request (CLS), which results in shutting off the APD gate. The signals are very nicely square, and very clean in the digital sense. Various measurements are presented at right.