| 000 | 04906nlm1a2200961 4500 | ||
|---|---|---|---|
| 001 | 657984 | ||
| 005 | 20231030041533.0 | ||
| 035 | _a(RuTPU)RU\TPU\network\24963 | ||
| 035 | _aRU\TPU\network\24733 | ||
| 090 | _a657984 | ||
| 100 | _a20180425a2017 k y0engy50 ba | ||
| 101 | 0 | _aeng | |
| 102 | _aNL | ||
| 135 | _adrcn ---uucaa | ||
| 181 | 0 | _ai | |
| 182 | 0 | _ab | |
| 200 | 1 |
_aThe HITRAN2016 molecular spectroscopic database _fI. E. Gordon [et al.] |
|
| 203 |
_aText _celectronic |
||
| 300 | _aTitle screen | ||
| 320 | _a[References: 641 tit.] | ||
| 330 | _aThis paper describes the contents of the 2016 edition of the HITRAN molecular spectroscopic compilation. The new edition replaces the previous HITRAN edition of 2012 and its updates during the intervening years. The HITRAN molecular absorption compilation is composed of five major components: the traditional line-by-line spectroscopic parameters required for high-resolution radiative-transfer codes, infrared absorption cross-sections for molecules not yet amenable to representation in a line-by-line form, collision-induced absorption data, aerosol indices of refraction, and general tables such as partition sums that apply globally to the data. The new HITRAN is greatly extended in terms of accuracy, spectral coverage, additional absorption phenomena, added line-shape formalisms, and validity. Moreover, molecules, isotopologues, and perturbing gases have been added that address the issues of atmospheres beyond the Earth. Of considerable note, experimental IR cross-sections for almost 300 additional molecules important in different areas of atmospheric science have been added to the database. The compilation can be accessed through www.hitran.org. Most of the HITRAN data have now been cast into an underlying relational database structure that offers many advantages over the long-standing sequential text-based structure. The new structure empowers the user in many ways. It enables the incorporation of an extended set of fundamental parameters per transition, sophisticated line-shape formalisms, easy user-defined output formats, and very convenient searching, filtering, and plotting of data. A powerful application programming interface making use of structured query language (SQL) features for higher-level applications of HITRAN is also provided. | ||
| 333 | _aРежим доступа: по договору с организацией-держателем ресурса | ||
| 461 | _tJournal of Quantitative Spectroscopy and Radiative Transfer | ||
| 463 |
_tVol. 203 _v[P. 3-69] _d2017 |
||
| 610 | 1 | _aэлектронный ресурс | |
| 610 | 1 | _aтруды учёных ТПУ | |
| 610 | 1 | _aмолекулярно-спектроскопическая база данных | |
| 610 | 1 | _aHITRAN | |
| 701 | 1 |
_aGordon _bI. E. |
|
| 701 | 1 |
_aRothman _bL. S. |
|
| 701 | 1 |
_aHill _bC. |
|
| 701 | 1 |
_aKochanov _bR. V. |
|
| 701 | 1 |
_aTan _bY. |
|
| 701 | 1 |
_aBernath _bP. F. |
|
| 701 | 1 |
_aBirk _bM. |
|
| 701 | 1 |
_aBoudon _bV. |
|
| 701 | 1 |
_aCampargue _bA. |
|
| 701 | 1 |
_aChance _bK. V. |
|
| 701 | 1 |
_aDrouin _bB. J. |
|
| 701 | 1 |
_aFlaud _bJ. -M. |
|
| 701 | 1 |
_aGamache _bR. R. |
|
| 701 | 1 |
_aHodges _bJ. T. |
|
| 701 | 1 |
_aJacquemart _bD. |
|
| 701 | 1 |
_aPerevalov _bV. I. |
|
| 701 | 1 |
_aPerrin _bA. |
|
| 701 | 1 |
_aShine _bK. P. |
|
| 701 | 1 |
_aSmith _bM.-A.H. |
|
| 701 | 1 |
_aTennyson _bJ. |
|
| 701 | 1 |
_aToon _bG. C. |
|
| 701 | 1 |
_aTran _bH. |
|
| 701 | 1 |
_aTyuterev _bVl. G. |
|
| 701 | 1 |
_aBarbe _bA. |
|
| 701 | 1 |
_aCsaszar _bA. G. |
|
| 701 | 1 |
_aDevi _bV. M. |
|
| 701 | 1 |
_aFurtenbacher _bT. |
|
| 701 | 1 |
_aHarrison _bJ. J. |
|
| 701 | 1 |
_aHartmann _bJ. -M. |
|
| 701 | 1 |
_aJolly _bA. |
|
| 701 | 1 |
_aJohnson _bT. J. |
|
| 701 | 1 |
_aKarman _bT. ] |
|
| 701 | 1 |
_aKleiner _bI. |
|
| 701 | 1 |
_aKyuberis _bA. A. |
|
| 701 | 1 |
_aLoos _bJ. |
|
| 701 | 1 |
_aLyulin _bO. M. |
|
| 701 | 1 |
_aMassie _bS. T. |
|
| 701 | 1 |
_aMikhailenko _bS. N. _cphysicist _cAssociate Professor of Tomsk Polytechnic University, Candidate of physical and mathematical sciences _f1962- _gSemen Nikolaevich _2stltpush _3(RuTPU)RU\TPU\pers\34035 |
|
| 701 | 1 |
_aMoazzen-Ahmadi _bN. |
|
| 701 | 1 |
_aMuller _bH.S.P. |
|
| 701 | 1 |
_aNaumenko _bO. V. |
|
| 701 | 1 |
_aNikitin _bA. V. |
|
| 701 | 1 |
_aPolyansky _bO. L. |
|
| 701 | 1 |
_aRey _bM. |
|
| 701 | 1 |
_aRotger _bM. |
|
| 701 | 1 |
_aSharpe _bS. W. |
|
| 701 | 1 |
_aSung _bK. |
|
| 701 | 1 |
_aStarikova _bE. |
|
| 701 | 1 |
_aTashkun _bS. A. |
|
| 701 | 1 |
_aVander Auwera _bJ. |
|
| 701 | 1 |
_aWagner _bG. |
|
| 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 _c20180425 _gRCR |
|
| 856 | 4 | _uhttps://doi.org/10.1016/j.jqsrt.2017.06.038 | |
| 942 | _cCF | ||