Photolysis of metal oxides as a source of atoms in planetary exospheres; Planetary and Space Science; Vol. 145

Xehetasun bibliografikoak
Parent link:Planetary and Space Science
Vol. 145.— 2017.— [P. 38-48]
Erakunde egilea: Национальный исследовательский Томский политехнический университет (ТПУ) Институт физики высоких технологий (ИФВТ) Кафедра общей химии и химической технологии (ОХХТ)
Beste egile batzuk: Valiev R. R. Rashid Rinatovich, Berezhnoy A. A. Aleksey Anatoljevich, Sidorenko A. D. Anna Dmitrievna, Merzlikin B. S. Boris Sergeevich, Cherepanov V. N. Viktor Nikolaevich
Gaia:Title screen
The cross sections of photolysis of LiO, NaO, KO, MgO, and CaO molecules have been calculated by the use of quantum chemistry methods. The maximal values for photolysis cross sections of alkali metal monoxides have the order of 10−17 cm2, and for alkaline earth metal monoxides these values are less on 1-2 orders of the magnitude. The lifetimes of photolysis at 1 astronomical unit are estimated as 5, 3, 60, 70, and 3,000 s for LiO, NaO, KO, MgO, and CaO, respectively. Typical kinetic energies of main peaks of photolysis-generated metal atoms are determined. Impact-produced LiO, NaO, KO, and MgO molecules are destroyed in the lunar and Hermean exospheres almost completely during the first ballistic flight while CaO molecule is more stable against destruction by photolysis. Photolysis-generated metal atoms in planetary exospheres can be detected by performing high-resolution spectral observations of velocity distribution of exospheric metal atoms.
Режим доступа: по договору с организацией-держателем ресурса
Hizkuntza:ingelesa
Argitaratua: 2017
Gaiak:
Sarrera elektronikoa:https://doi.org/10.1016/j.pss.2017.07.011
Formatua: Baliabide elektronikoa Liburu kapitulua
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=655866

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200 1 |a Photolysis of metal oxides as a source of atoms in planetary exospheres  |f R. R. Valiev [et al.] 
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330 |a The cross sections of photolysis of LiO, NaO, KO, MgO, and CaO molecules have been calculated by the use of quantum chemistry methods. The maximal values for photolysis cross sections of alkali metal monoxides have the order of 10−17 cm2, and for alkaline earth metal monoxides these values are less on 1-2 orders of the magnitude. The lifetimes of photolysis at 1 astronomical unit are estimated as 5, 3, 60, 70, and 3,000 s for LiO, NaO, KO, MgO, and CaO, respectively. Typical kinetic energies of main peaks of photolysis-generated metal atoms are determined. Impact-produced LiO, NaO, KO, and MgO molecules are destroyed in the lunar and Hermean exospheres almost completely during the first ballistic flight while CaO molecule is more stable against destruction by photolysis. Photolysis-generated metal atoms in planetary exospheres can be detected by performing high-resolution spectral observations of velocity distribution of exospheric metal atoms. 
333 |a Режим доступа: по договору с организацией-держателем ресурса 
461 |t Planetary and Space Science 
463 |t Vol. 145  |v [P. 38-48]  |d 2017 
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701 1 |a Valiev  |b R. R.  |c chemist  |c Assistant of Tomsk Polytechnic University  |f 1983-  |g Rashid Rinatovich  |3 (RuTPU)RU\TPU\pers\34114 
701 1 |a Berezhnoy  |b A. A.  |g Aleksey Anatoljevich 
701 1 |a Sidorenko  |b A. D.  |g Anna Dmitrievna 
701 1 |a Merzlikin  |b B. S.  |c mathematician  |c research engineer, Senior Lecturer of Tomsk Polytechnic University, candidate of physico-mathematical Sciences  |f 1987-  |g Boris Sergeevich  |3 (RuTPU)RU\TPU\pers\30925  |9 15163 
701 1 |a Cherepanov  |b V. N.  |g Viktor Nikolaevich 
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