Eunsook S. Hwang, Bart Buijsse, Richard A. Copeland, Haris Riris, Clint B. Carlisle and Tom G. Slanger
Evidence from several sources suggest possible
in situ production of N2O in
the stratosphere. Considering that solar photoabsorption
provides a large stratospheric source of
O2(A3Σu+),
and since vibrational levels of v6 are
primarily removed by N2, the
O2(A3Σu+
)+N2 system is studied to determine whether it is
an atmospherically significant N2O source. Using
243–250 nm photoexcitation to produce vibrationally
excited
O2(A3Σu+,
v=7–10), and frequency modulation diode laser
spectroscopy as the detector of N2O, we examine
the products generated in a closed cell. We thereby set an
upper limit of 0.002% on the N2O yield for the
process, and conclude that stratospheric N2O
production by this route is not significant compared to
existing ground-based sources. The stability of
N2O in an
N2O–O3–N2
mixture subjected to prolonged 245 nm radiation is also
studied. For low levels of O3 (10 ppm) and
N2O (40–90 ppb), no loss of N2O
is observed.