Extended analysis of the v12 band of 12C2H4 for astrophysical applications: Line strengths, widths, and shifts; Journal of Quantitative Spectroscopy and Radiative Transfer; Vol. 233

מידע ביבליוגרפי
Parent link:Journal of Quantitative Spectroscopy and Radiative Transfer
Vol. 233.— 2019.— [P. 57-66]
מחבר תאגידי: Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
מחברים אחרים: Ulenekov (Ulenikov) O. N. Oleg Nikolaevich, Bekhtereva E. S. Elena Sergeevna, Gromova O. V. Olga Vasilievna, Kakaulin A. N. Aleksey Nikolaevich, Sydow Ch. Christian, Bauerecker S. Sigurd
סיכום:Title screen
The 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.
Режим доступа: по договору с организацией-держателем ресурса
שפה:אנגלית
יצא לאור: 2019
נושאים:
גישה מקוונת:https://doi.org/10.1016/j.jqsrt.2019.05.017
פורמט: אלקטרוני Book Chapter
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=664266

MARC

LEADER 00000naa0a2200000 4500
001 664266
005 20250424145408.0
035 |a (RuTPU)RU\TPU\network\35450 
035 |a RU\TPU\network\29694 
090 |a 664266 
100 |a 20210406d2019 k||y0rusy50 ba 
101 0 |a eng 
102 |a NL 
135 |a drcn ---uucaa 
181 0 |a i  
182 0 |a b 
200 1 |a Extended analysis of the v12 band of 12C2H4 for astrophysical applications: Line strengths, widths, and shifts  |f O. N. Ulenekov, E. S. Bekhtereva, O. V. Gromova [et al.] 
203 |a Text  |c electronic 
300 |a Title screen 
320 |a [References: 81 tit.] 
330 |a The 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 |a Режим доступа: по договору с организацией-держателем ресурса 
338 |b Российский фонд фундаментальных исследований  |d 18–02–00819 A 
461 |t Journal of Quantitative Spectroscopy and Radiative Transfer 
463 |t Vol. 233  |v [P. 57-66]  |d 2019 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
610 1 |a high-resolution spectra 
610 1 |a ethylene 
610 1 |a спектры высокого разрешения 
701 1 |a Ulenekov (Ulenikov)  |b O. N.  |c physicist  |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences  |f 1949-  |g Oleg Nikolaevich  |3 (RuTPU)RU\TPU\pers\34331  |9 17837 
701 1 |a Bekhtereva  |b E. S.  |c physicist  |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences  |f 1974-  |g Elena Sergeevna  |3 (RuTPU)RU\TPU\pers\34450  |9 17851 
701 1 |a Gromova  |b O. V.  |c physicist  |c Professor of Tomsk Polytechnic University, Candidate of physical and mathematical sciences  |f 1982-  |g Olga Vasilievna  |3 (RuTPU)RU\TPU\pers\34333  |9 17839 
701 1 |a Kakaulin  |b A. N.  |c physicist  |c Technician of Tomsk Polytechnic University  |f 1998-  |g Aleksey Nikolaevich  |3 (RuTPU)RU\TPU\pers\47224 
701 1 |a Sydow  |b Ch.  |g Christian 
701 1 |a Bauerecker  |b S.  |g Sigurd 
712 0 2 |a Национальный исследовательский Томский политехнический университет  |b Исследовательская школа физики высокоэнергетических процессов  |c (2017- )  |3 (RuTPU)RU\TPU\col\23551 
801 0 |a RU  |b 63413507  |c 20220524  |g RCR 
850 |a 63413507 
856 4 |u https://doi.org/10.1016/j.jqsrt.2019.05.017 
942 |c CF