WHAT KIND OF SIGNALS DO WE LOOK FOR?
The best communication method known to us is through radio waves.
Radio waves have the information carrying capacity and they can be
transmitted using equipment that is cheap to build. The information also
travels at the speed of light. Moreover we can receive signals from various
directions and communicate simultaneously with many different
civilizations.
The electromagnetic spectrum is very large and the signals can be sent at
any frequency. So we should find a reasonably small region of it to begin
our search.
The galaxy produces noise at low frequencies and the atmosphere at
higher frequencies. Between the two noisy regions we have a relatively
quiet region -- from about 1 GHz to about 10 GHz.
Neutral hydrogen gas emits radio signals at 1.42 GHz and the hydroxyl
emits signals at around 1.64 GHz. We know that the water molecule is
composed of these two species. Accepting the fundamental need of water
for life to exist, we find ourselves with a frequency range between these
two emissions which is a quiet region of the spectrum and is termed "the
water hole." This gives us a nice limited frequency range to start our
search.
Nature of the spectrum of the signals we look for:
A message transmitted on many frequencies is not efficient as it
consumes lots of power. However, if one selects a very narrow frequency
bandwidth to concentrate the power of the signal, then the signal can be
transmitted easier through the background noise. Considering the
distances over which these signals must travel before they reach our
planet, we expect intelligent extra-terrestrials to send a very specific
frequency message.

To distinguish these signals from local earth-based signals, we recognize
the fact that local signals maintain more or less constant intensities with
time. However in case of a SETI telescope, it is the sky that is seen to drift
past the focus of the telescope. In 12 seconds a target typically crosses
the focus (target beam) of the telescope. Thus an extraterrestrial signal is
expected to grow in intensity and then diminish over the 12 second time
period. This shape is described by the Gaussian curve.

Due to the relative motion of planets, we are likely to observe a Doppler
shifting or frequency shifting of the signal due to relative motion of the
telescope during the 12 second period. This would cause the signal to rise
or fall in frequency slightly over the time length of 12 seconds. These
signals are called chirped signals. Also if alien civilizations are sending
information our way then the signals are surely going to be pulsed in
nature. Thus we may refine our search by checking for chirped signals
containing pulses.
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