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What is A Cosmic Ray?
If you were to leave the shutter open
on your digital camera in a dark room and take a long exposure image,
you would see something like the end of the movie playing above. And if you
were an astronomer trying to take a picture of a celsestial object, those
little streaks and spots that randomly appear would make you curse the
very heavenly bodies you sought to photograph.
The streaky, spotty blemishes that show up randomly throughout the movie
are referred to as cosmic rays. A cosmic ray can be an electron, a muon, a
gamma ray, and perhaps even other exotic particles. These particles, like the
photons of light we want to record in our images carry energy. And that energy
can liberate electron hole pairs in a detector, generating the same signal
as that caused by a visible photon.
Fortunately for the typical digital camera user, the light levels and exposure
time of typical pictures are such that cosmic rays do not pose a problem.
But for astronomers taking pictures of very dim objects in the night sky, they
do. Special techniques are used, especially for space-based telescopes where
the atmosphere does not filter out cosmic rays, to remove them from
astronomical images. Luckily, because of their random nature it is unlikely
that a cosmic ray will hit the same location in a detector in successive images, allowing one to filter them out in software by combining multiple images.
Unlike lightning, however, cosmic rays can strike twice; you just have to
expose long enough.
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