1. Multiple Detection Search During the last month we've been searching the science
data base for radio signals seen two or more times. Since the SETI@home participants have
already analyzed 1.5 years of data from the Arecibo telescope, there are already many
places on the sky we've observed two or more times.
We search for signals that recur at almost exactly the same place on the sky and almost
exactly the same frequency. We also search for signals whose frequency may have drifted
significantly over the many months between observations. Signals might drift in frequency
because of the "doppler effect" - a transmitter on a rotating and revolving
planet will move toward and away from earth, and this acceleration produces a shift in the
observed frequency. Another civilization might correct for their motion if they are
deliberately transmitting a signal towards us; then their transmitter's frequency would
remain steady, assuming we account for our own planet's motion. But we don't know if
extraterrestrial civilizations will correct for their motion, so we look for both drifting
and non-drifting signals.
So far, we've identified two pairs of strong gaussian shaped signals, both seen on two
different observations. We've also found three trios of weaker gaussian signals, each
signal seen on three different observations. We are examining these data further, and also
examining some even weaker signals. But these multiple detections are almost certainly
from noise, and not signals from another civilization. We are searching through a data
base of 50 million gaussian signals, and a few of these 50 million signals will randomly
occur at almost the same place and the almost the same frequency. We've examined thousands
of these kinds of multiple detections in our 25 years of searching, and so far they've
always turned out to be noise or radio pollution from terrestrials, not extraterrestrials.
2. Pulse Detection
We've also been developing a new version of the SETI@home screensaver program that
searches for pulsing radio signals. We hope to beta test this new program next month and
make it available for all SETI@home participants sometime this summer.
The new pulse software searches for regularly spaced radio pulses. Much like a light
house sends out regular optical flashes, another civilization might send out regular radio
pulses. If we converted these radio waves into sound waves, you might hear "click,
click, click...".
The pulse hunting software uses two different algorithms - one algorithm searches for
three pulses evenly spaced in time. This "triplet" algorithm doesn't take much
computer time, but it can only detect powerful pulses. The second algorithm, developed by
Eric Korpela, can find very weak pulses if they are regularly repeated tens, hundreds or
thousands of times.
The new pulse searching code adds several hours of computation to each work unit.
However, we've also been optimizing version 2.04 analysis software, and when we combine
the extra computational burden from the pulse search and the speed up from the
optimization, the new version 3.0 doesn't take that much longer than version 2.04, and
will allow a search for a whole new class of signals.