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I. Merke et al. / Journal of Molecular Structure 795 (2006) 185–189
spectroscopy) had been completely converted to SO2F2.
Purification of SO2F2 was achieved by fractional condensation
using a standard greaseless vacuum line.
Magnetic hyperfine structure was caused by spin–spin and
spin–rotation interactions of the fluorine nuclei. From these
hyperfine structures of the transitions, which closely resemble
those of the ground state, it was concluded that the vibrational
state to which they belong had to have A1 or A2 symmetry.
The K-pattern, which is usually mainly governed by inertia
asymmetry, was different from any of the other vibrational
satellite sets or the ground state, distinguishing this set from the
alternative assignment as a lower-energy vibrational satellite of
the 34S-isotopomer.
Intensity comparison with transitions of the 34S-isotopomer
resulted in an estimated state population of roughly one-third
that of the natural abundance of sulfur-34 (w4%), confirming
the initial assumption of population for a state with relatively
high energy. In fact, only one of the remaining fundamental
states, namely n2, could conceivably have satellite sets of such
intensity. Since the n2 state has an energy of w850 cmK1, this
assignment yields in the molecular beam a vibrational
temperature for this state of about 280G10 K, i.e. no
substantial cooling. For comparison, the satellite sets of the
dyad states n4 and n5 (w380 cmK1) had intensities correspond-
ing to an average vibrational temperature of about 170 K, those
of the triad states n3, n7 and n9 (all three w550 cmK1) of about
220 K. The rotational temperature is dramatically lower,
usually less than 10 K.
In Aachen the measurements in the frequency region
10–40 GHz were carried out using supersonic molecular
beam Fourier transform microwave (MB-FTMW) spec-
trometers which have been described elsewhere [12,13]. In
all cases, a mixture of about 1% SO2F2 in helium was used. The
stagnation pressure was typically 100 kPa. Due to only partly
resolved fluorine spin–spin and spin–rotation coupling, the
accuracy for the center frequency was limited to about 2 kHz.
Transitions in the frequency region 50–110 GHz were
recorded using an absorption-type spectrometer with source
modulation and 2f phase sensitive detection. Schottky diodes
were used as detectors. The pressure in the cell was about 2 Pa
throughout and the centers of unblended lines could be
determined with an accuracy of about 10–30 kHz depending
on their intensity.
In Lille, the millimeterwave (MMW) spectrum was
measured with a source-modulation spectrometer using as
source either harmonics of a Gunn diode between 150 and
250 GHz, or a Thomson-CSF backward-wave oscillator
between 420 and 450 GHz. In both cases a He-cooled InSb
bolometer was used as detector. The accuracy of the
measurements varies between 50 and 200 kHz for unblended
lines depending on the spectral region and the frequency step
chosen to record the spectrum.
3.2. Rovibrational spectrum
The IR spectrum of n2 was obtained in Wuppertal in
connection with our previous study of the n8 band, see Ref. [9]
for experimental details. The resolution (1/maximum optical
path difference) was 0.0024 cmK1, the precision of isolated
lines of medium intensity 0.0001 cmK1. Owing to the density
The n2 band is located ca. 38 cmK1 below the slightly more
intense n8 band, and therefore the R-branch of n2 is overlapped
by the P-branch of n8 giving rise to a high line density in the
region between the band centers. The reader is referred to
Fig. 1 of Ref. [9] for a survey spectrum of the n2 and n8 bands of
SO2F2.
The Q-branch of n2 is located at 849.5 cmK1 degrading
towards smaller wavenumbers. The band shows the typical
appearance of an A-type band with P- (Fig. 1) and R-clusters
(Fig. 2) spaced (BCC), w0.338 cmK1. Nuclear spin statistical
weights are clearly observed in the clusters: lines with Ka odd
are three times stronger than lines with Ka even. The most
intense transitions are governed by the selection rule DKaZ0.
However, transitions with DKaZG2 are also present as
indicated by weaker cluster structures partly overlapping the
DKaZ0 clusters.
The assignment of J-quantum numbers to the P- and
R-branch cluster structures (Figs. 1 and 2) was straightforward.
However, the assignment to Ka of the individual cluster lines
could not be done just by inspection since in A-type bands the
unsplit KaZJ or JK1 lines at the onset of the cluster are
relatively weak. Overlap from DKaZG2 clusters also
complicated the assignment. We finally used ground state
combination differences (GSCDs) based on the ground state
constants [9] and assigned in this way ca. 1100 DKaZ0 and ca.
800 DKaZG2 P- and R-branch lines. The maximum upper
state quantum numbers are JZ68 and KaZ59. For KaO47 only
lines with odd Ka values were assigned. Low-Ka lines are weak
and we were not able to assign with confidence lines where Ka
of the spectrum the effective precision is about 0.0002 cmK1
3. Description of the spectra and assignments
3.1. Rotational spectrum
.
The initial MW experiments, in the frequency range around
30 GHz (w1 cmK1), had to take into account the observation
that in the previously recorded MB-FTMW spectra of SO2F2,
the vibrational satellite transitions of the known states nx, ny, nz,
nw, nu [2] (now assigned as n4, n5, n9, n7, n3) had intensities
which indicated distinctly different vibrational temperatures.
This is due to the fact that in a beam molecules are not in
thermodynamic equilibrium. Therefore formally different
vibrational and rotational temperatures have to be assigned to
different states. In particular, higher energy states appeared to
reveal higher vibrational temperature, i.e. less cooling and
hence enhanced relative intensity in the supersonic expansion.
Searches for the SF stretching state satellites were made on the
low-frequency sides of the transitions of the ground state, and
weak line patterns, characteristic for a near-prolate top, and
belonging to a hitherto unknown species eventually emerged.
These findings were then confirmed by the assignment of
further transitions in lower (w10 and w20 GHz) and higher
frequency ranges (50–435 GHz).