1981
DOI: 10.1016/0022-2852(81)90179-x
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A simultaneous analysis of the microwave, submillimeterwave, far infrared, and infrared-microwave two-photon transitions between the ground and ν2 inversion-rotation levels of 14NH3

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Cited by 125 publications
(18 citation statements)
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“…We employed the SPFIT software [85,86] to implement the effective Hamiltonian developed in [80][81][82][83][84]7]. It is in the same general form as the effective Hamlitonian used by Belov et al [45], Urban et al [64], and Poynter and Margolis [54,55]. Using the notational convention by Sarka and Schrötter [7] this effective Hamiltonian (H) can be expressed as follows (bold symbols distinguish vectorial or tensorial operators from scalar quantities):…”
Section: Resultsmentioning
confidence: 99%
“…We employed the SPFIT software [85,86] to implement the effective Hamiltonian developed in [80][81][82][83][84]7]. It is in the same general form as the effective Hamlitonian used by Belov et al [45], Urban et al [64], and Poynter and Margolis [54,55]. Using the notational convention by Sarka and Schrötter [7] this effective Hamiltonian (H) can be expressed as follows (bold symbols distinguish vectorial or tensorial operators from scalar quantities):…”
Section: Resultsmentioning
confidence: 99%
“…Tunneling splittings are described better. The ground-state tunneling splitting is 0.6 cm −1 , on AMMPOT2, which is 25% off the experimental value of 0.79 cm −1 (Urban et al 1981). Marquardt et al (2005) also reviewed other PESs for ammonia that are important from the prospective of high-resolution spectroscopy (Lin et al 2002, Yurchenko et al 2005a,b,c, Rajamäki et al 2003, Leonard et al 2003.…”
Section: Ammoniamentioning
confidence: 89%
“…For 14 NH 3 , there exists a large number of at least partially assigned high-resolution experimental spectra [2,13,20,[29][30][31]38,41,42,45,46,[50][51][52][53][54]57,62,67,69,76,77,79,[84][85][86]88,91,92,95,96,98,99,112,119,[128][129][130]132,135,139,140,142,146,148]. The data from room-temperature measurements are augmented by data from a number of warm (373 K) [31,46], hot (up to 1640 K) [129,135,137,…”
Section: Experimental Data and Data Treatmentmentioning
confidence: 99%
“…This was done by setting the energy of the ð000 0 0 0 Þ [11] state to 16.172993 cm -1 resulting from an EH fit [52], with an assumed zero uncertainty. (IIb) 81UrSpPaKa [45]: The lines measured include a few Δk ¼ 7 3 "perturbation allowed" transitions.…”
Section: Magic Numbersmentioning
confidence: 99%
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