10 Hz (surface rate)
----» 1 Hz ----» 0.5 Hz ----» 0.3 Hz
which we of course expect
to see. We will, however, need to
correct for these "raw" values for
1. detector efficiency (even a 95% efficient detector will miss
counting 5% of the cosmic rays, requiring us to "scale up" the numbers)
2. acceptance (size/geometry - we'll want to report these rates in
counts/cm2sec)
3. accidental coincidences collected by our detectors.
We will learn how to do all of these steps, one at a time.