The inertial confinement fusion (ICF) community must become more cognizant
of the neutron-induced background levels in charge-coupled device (CCD) det
ectors that are replacing film as the recording medium in many ICF diagnost
ics. This background degrades the signal-to-noise ratio (SNR) of the record
ed signals and for the highest-yield shots comprises a substantial fraction
of the pixel's full well capacity. CCD detectors located anywhere in the O
MEGA Target Bay are precluded from recording high precision signals (SNR >
30) for deuterium-tritium neutron yields greater than 10(13). CCDs make exc
ellent calibrated neutron detectors. The average CCD background level is pr
oportional to the neutron yield, and we have measured a linear response ove
r four decades. The spectrum of deposited energy per pixel is heavily weigh
ted to low energies, < 50 keV, with a few isolated saturated pixels. Most o
f the background recorded by the CCDs is due to secondary radiation produce
d by interactions of the primary neutrons with all the materials in the Tar
get Bay as well as the shield walls and the floor. Since the noise source c
omes from all directions it is very difficult to shield. The fallback posit
ion of using film instead of CCD cameras for high-neutron-yield target shot
s is flawed, as we have observed substantially increased fog levels on our
x-ray recording film as a function of the neutron yield. (C) 2001 American
Institute of Physics.