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Emission spectra produced from thermal energy charge transfer reactions of Ar+ ions with CS and PN radicals

โœ Scribed by Hiroshi Obase; Masaharu Tsuji; Yukio Nishimura


Book ID
107942048
Publisher
Elsevier Science
Year
1984
Tongue
English
Weight
641 KB
Volume
87
Category
Article
ISSN
0301-0104

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๐Ÿ“œ SIMILAR VOLUMES


CS2+(A-X) emission produced from the cha
โœ Minoru Endoh; Masaharu Tsuji; Yukio Nishimura ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 476 KB

## CS? in an Ar afterglow eshibircd rrnission from the 0'. 1' and 2' levels of CSG(x 'n,-% 'II,). The excitation source was attributed to Ar;. The vibrational frequencies of CS;(.?: U: = 4 and u'; + $u: = 3) were detcrkined from the vibrational analysis of the (u'; ,&.O) progressions from the O" l

N2+(Bโ€”X) Emission produced from the ther
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\(\mathrm{N}_{2}^{+}\left(\mathrm{B}^{2} \Sigma_{\mathrm{u}}^{+}-\mathrm{X}^{2} \Sigma_{\mathrm{g}}^{+}\right)\)emission was observed from the near-resonant charge transfer between \(\mathrm{Ne}_{2}^{+}\)and \(\mathrm{N}_{2}\). Vibrational populations for \(v^{\prime}=0\) and 1 of \(N_{2}^{+}(B)\) w

SO+(A2ฮ -X2ฮ r) emission produced from a d
โœ Masaharu Tsuji; Chikashi Yamagiwa; Minoru Endoh; Yukio Nishimura ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 484 KB

The extensive bands observed from the hehum afterglow reaction of SO\* m the 250-540 mn region are assigned to the new SO+(A \*rt--X\*l$) system produced from the He\*/S02 dissociative charge-transfer reaction at themA energy. They had been erroneously mterpreted as the SO; (c-4 system produced from

The rotational distribution of OCS+(รƒ 2ฮ 
โœ Masaharu Tsuji; John P. Maier; Hiroshi Obase; Hiroshi Sekiya; Yukio Nishmura ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 364 KB

The OCS'(A 'lTrrR 'Up: Q= l/2,3/2) emission resultmg from the Ar+('P,,,) +OCS charge-transfer reaction has been reexamined in a low-pressure flowing afterglow. The fluorescence channel in the the 0" level was found to be open for rotationally excited levels up to Jz 170 ( z 5500 cm-'). The rotation