000 | 03361nlm1a2200445 4500 | ||
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001 | 664266 | ||
005 | 20231030041923.0 | ||
035 | _a(RuTPU)RU\TPU\network\35450 | ||
035 | _aRU\TPU\network\29694 | ||
090 | _a664266 | ||
100 | _a20210406a2019 k y0engy50 ba | ||
101 | 0 | _aeng | |
102 | _aNL | ||
135 | _adrcn ---uucaa | ||
181 | 0 | _ai | |
182 | 0 | _ab | |
200 | 1 |
_aExtended analysis of the v12 band of 12C2H4 for astrophysical applications: Line strengths, widths, and shifts _fO. N. Ulenekov, E. S. Bekhtereva, O. V. Gromova [et al.] |
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203 |
_aText _celectronic |
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300 | _aTitle screen | ||
320 | _a[References: 81 tit.] | ||
330 | _aThe high-resolution infrared spectra of 12C2H4 were analyzed in the region of 1360 - 1530 cm-1, where the strong V12 band is located. 998 line strengths (1491 transitions) were determined from the fit of their line shapes with a Hartmann-Tran profile (Jmax=48 and Kamax=17) which is about two times more than in the preceding studies. These data were used in the fit of the effective dipole moment parameters and six such parameters were obtained which reproduce the strengths of the 998 initial lines (1491 transitions) with the drms=2.31%. Self-broadening and self-shift coefficients were determined from the multi-spectrum analysis for sets of lines (JKa=KaKc)<-(JKaKc), Ka=0,1,2,3,4,5 (in general, 253 lines for determination of self-broadening coefficients and 225 lines for determination of self-shift coefficients). The line list of 19186 transitions is documented. | ||
333 | _aРежим доступа: по договору с организацией-держателем ресурса | ||
338 |
_bРоссийский фонд фундаментальных исследований _d18–02–00819 A |
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461 | _tJournal of Quantitative Spectroscopy and Radiative Transfer | ||
463 |
_tVol. 233 _v[P. 57-66] _d2019 |
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610 | 1 | _aэлектронный ресурс | |
610 | 1 | _aтруды учёных ТПУ | |
610 | 1 | _ahigh-resolution spectra | |
610 | 1 | _aethylene | |
610 | 1 | _aспектры высокого разрешения | |
701 | 1 |
_aUlenekov _bO. N. _cphysicist _cProfessor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences _f1949- _gOleg Nikolaevich _2stltpush _3(RuTPU)RU\TPU\pers\34331 |
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701 | 1 |
_aBekhtereva _bE. S. _cphysicist _cProfessor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences _f1974- _gElena Sergeevna _2stltpush _3(RuTPU)RU\TPU\pers\34450 |
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701 | 1 |
_aGromova _bO. V. _cphysicist _cProfessor of Tomsk Polytechnic University, Candidate of physical and mathematical sciences _f1982- _gOlga Vasilievna _2stltpush _3(RuTPU)RU\TPU\pers\34333 |
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701 | 1 |
_aKakaulin _bA. N. _cphysicist _cTechnician of Tomsk Polytechnic University _f1998- _gAleksey Nikolaevich _2stltpush _3(RuTPU)RU\TPU\pers\47224 |
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701 | 1 |
_aSydow _bCh. _gChristian |
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701 | 1 |
_aBauerecker _bS. _gSigurd |
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712 | 0 | 2 |
_aНациональный исследовательский Томский политехнический университет _bИсследовательская школа физики высокоэнергетических процессов _c(2017- ) _h8118 _2stltpush _3(RuTPU)RU\TPU\col\23551 |
801 | 2 |
_aRU _b63413507 _c20220524 _gRCR |
|
856 | 4 | _uhttps://doi.org/10.1016/j.jqsrt.2019.05.017 | |
942 | _cCF |