  The effects of the in-flight behaviour of the bolometer arrays of the
Herschel/PACS instrument under impacts of Galactic cosmic rays are explored.
This instrument is part of the ESA-Herschel payload, which will be launched at
the end of 2008 and will operate at the Lagrangian L2 point of the Sun-Earth
system. We find that the components external to the detectors (the spacecraft,
the cryostat, the PACS box, collectively referred to as the `shield') are the
major source of secondary events affecting the detector behaviour. The impacts
deposit energy on the bolometer chips and influence the behaviour of nearby
pixels. 25% of hits affect the adjacent pixels. The energy deposited raises the
bolometer temperature by a factor ranging from 1 to 6 percent of the nominal
value. We discuss the effects on the observations and compare simulations with
laboratory tests.
