The SWAN instrument onboard the SOHO spacecraft is a Lyman cu scanning phot
ometer cabable of mapping the whole sky with 1 degrees resolution. Since Ja
nuary 1995 the instrument has produced on average three full sky maps a wee
k with the principal scientific objective of observing the distribution of
heliospheric neutral hydrogen. In addition, these systematic observations a
re a valuable source for studying comets brighter than a visual magnitude o
f 7-11 the observing limit depending on the abundance ratios of produced ra
dicals and the location of the comet relative to the galactic plane. When t
he data before the temporary loss of control of SOHO st the end of June 199
8 were processed, altogether 18 comets were positively identified, of which
one is a new discovery and another 5 can be detected on SWAN images before
their actual discovery date. This demonstrates the feasibility of SWAN as
an instrument for cometary surveys. The observations are used to estimate t
he water production rates of the detected comets near their perihelion pass
ages.