Abstract
A technique is described for the investigation of gaseous spectra at high radio-frequencies. The sensitivity of the method is such that an absorption of 2 x 10
-6
per cm. of path can be detected at wave-lengths around 1 cm. The inversion spectrum of ammonia in the ground vibrational state has been examined at wave-lengths between 1.1 and 1.6 cm. and found to contain an extensive fine structure, arising from centrifugal distortion of the molecule. Twenty-nine lines have been identified, each corresponding to a different rotational quantum state. The wave numbers of these lines can be accurately represented by the formula
v
= 0.7935 + [-0.0050
5
J
2
+J+0.0070
4
K
2
] + 0.63[-0.0050J
2
+J+ 0.0070K
2
]
2
cm.
-1
(vacuo) where
J, K
are the rotational quantum numbers of the symmetrical top molecule. Detailed measurements of 18 lines at a pressure of 0.5 mm. Hg show that their half widths, due to collision broadening, lie between 2 and 5 x 10
-4
cm.
-1
, while their intensities agree with the theoretical values, within the experimental error of ± 5%. The integrated intensity at a pressure of 4.5 mm. Hg, over the interval 0.67 to 0.87 cm.
-1
, agrees with the calculated intensity to better than 1%.
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