M. Islam et al.rChemical Physics Letters 305 (1999) 311–318
313
quency doubling the output of an excimer-pumped
dye laser ŽLambda-Physik, FL2002.. LIF was ex-
Js37.5 level, the frequency of the pump laser was
then scanned to wavelengths where the Ž2, 0. R-
cited by tuning this UV probe radiation to an appro-
branch IR transition to Js40.5 was expected, again
at a delay corresponding to ca. 1 collision. A LIF
signal was detected when the IR laser was in reso-
nance with the line promoting molecules to the
Js40.5 level. This was confirmed by subsequently
2
q
priate transition in the Ž0, 2. band of the NO A S –
2
X P system at ca. 247 nm.
Experiments on the highest rotational levels Ž Js
3
1.5 and 40.5. required the initial photolysis of NO
2
2
q
to generate rotationally hot NO molecules in the
ground vibrational state. For this purpose, laser radi-
ation was generated at 355 nm by sum frequency
mixing the fundamental and doubled output of a
Nd:YAG laser ŽSpectron, SL 803.. Typical pulse
tuning the UV probe laser to the A S –
2
X P1r2Ž0, 2. transition from this level at short time
delays. The kinetic experiments in which the time
delay between the pulses from the pump and probe
lasers was varied were then performed. In the three
laser experiments, the time delay between the pulse
energies of ca. 20 mJ and a bandwidth of 0.1 cmy1
were obtained.
from the laser photolysing NO and that from the IR
2
The beams from the IR and UV lasers counter-
propagated along the axis of a cylindrical Pyrex cell
with a CaF2 window mounted on each end. The
photomultiplier, interference filter and a collecting
lens were mounted in a central housing which was
clamped to this cell. The equipment for controlling
the firing of the lasers and for recording, accumulat-
ing and analysing the LIF signals was the same as
that described by Frost and Smith w28x.
pump laser was -100 ns.
In all experiments, the time delay between the
pump and probe laser pulses was varied with a delay
generator ŽStanford DG535. and the resulting LIF
signal was detected. To discriminate against scat-
tered light from the probe laser, the fluorescence was
observed using a solar blind photomultiplier tube
ŽHamamatsu R801., through a quartz window and an
interference filter ŽCorion, FWHM 10 nm. centred at
228 nm, which isolated the fluorescence in the Ž0, 0.
Conventional IRUVDR experiments were carried
out to measure the total rates of rotational relaxation
2
q
2
band of the A S –X P system at ca. 226 nm.
The dependence of the observed rate coefficients
on the relative polarisations of the lasers was exam-
ined by rotating the plane of polarisation of the
probe laser through 908 from its usual orientation
using a Fresnel rhomb. The measured rate coeffi-
cients were found to be independent of this change
within the error limits of the measurements. This
confirmed that our measurements yield rates of rota-
tional energy transfer and do not contain a signifi-
cant component due to re-orienting collisions with-
out change of rotational level.
2
from NOŽX P , Õs2, Js7.5, 20.5 and 31.5. in
1
r2
collisions with He, Ar, N and NO. In these experi-
2
ments, the IR pump laser was first tuned to the
appropriate line in the Ž2, 0. vibrational overtone
band using the spectrophone. Then a short delay was
set between the pump and probe pulses and the UV
laser was scanned to bring its frequency into reso-
2
q
nance with the appropriate line in the A S –
2
X PŽ0, 2. band.
IRUVDR experiments on the NO produced from
photolysis of NO were carried out to measure the
2
2
total rates of rotational relaxation from NOŽX P
,
1
r2
Õs2, Js31.5 and 40.5. in collisions with He, Ar,
N . Tuning the lasers was now rather more difficult.
3. Experimental results
2
As m2entioned above, for measurements on
NOŽX P , Õs2, Js31.5., the correct IR pump
The decay in the LIF signals as a function of time
for a given gas mixture was fitted to an exponential
function from which a pseudo-first-order rate coeffi-
cient was obtained. Examples of such fittings for
1
r2
frequency could be located using the spectrophone.
2
In addition, a LIF spectrum from NOŽX P , Õs2.
1
r2
could be taken at a time delay corresponding to ca. 1
2
q
2
2
collision in order to locate the A S –X P1r2Ž0, 2.
transitions from higher, collisionally populated, rota-
tional levels up to Js37.5. With the frequency of
the UV probe laser fixed on the line from the
NOŽX P , Õs2, Js40.5. in mixtures contain-
1r2
ing different partial pressures of helium are shown in
Fig. 1. A series of such measurements was carried
out and the first-order rate coefficients were plotted