We present a photochemical model describing the changes in the isotopic com
position of stratospheric water vapor that result from methane oxidation an
d reactions with O(D-1). We then compare model calculations with measuremen
ts made with the Smithsonian Astrophysical Observatory far-infrared spectro
meter during seven balloon flights that took place between 1989 and 1997. T
he agreement between the model calculations and measurements establishes th
e validity of the model and the internal consistency of the data set. Final
ly, we use the model and measurements together to estimate the mixing ratio
and isotopic composition of water vapor entering the stratosphere and find
that the average over all flights of the water vapor mixing ratio, deltaD,
delta O-18, and delta O-17 are 3.48 +/- 0.15 parts per million by volume,
-679 +/- 20 parts per thousand, -128 +/- 31 parts per thousand, and -84 +/-
31 parts per thousand, respectively, where the errors indicate the estimat
ed accuracy.