𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Chemiluminescent reaction at thermal energy: The CS+ (A2Π, −X2∑+) emission produced from the C+(2P) + OCS reaction

✍ Scribed by Kazumi Mizukami; Hiroshi Obase; Masaharu Tsuji; Yukio Nishimura


Publisher
Elsevier Science
Year
1985
Tongue
English
Weight
306 KB
Volume
116
Category
Article
ISSN
0009-2614

No coin nor oath required. For personal study only.

✦ Synopsis


The CS + (A2Hi-X 2~+ ) emission has been observed in the C + (2p)+ocs reaction at thermal energy in a flowing afterglow apparatus. New bands of CS + (A 2 II~-X 2~ + ) from v'= 10-14 to v"= 0-3 were identified. The vibratio.nal populations in the CS + (A21-I~) state were estimated by spectral simulation.


📜 SIMILAR VOLUMES


Chemiluminescent reaction at thermal ene
✍ Masaharu Tsuji; Toshihiko Susuki; Minoru Endoh; Yukio Nishimura 📂 Article 📅 1982 🏛 Elsevier Science 🌐 English ⚖ 280 KB

CO\*(A "ll-X 2P) emission produced from the C(2P) + O2 reaclm hss been observed al thermal cncrgy III a flowing afterdow apparatus. The relabve vIbrational population In the CO\*(A %I) state was dctcrrnmcd The avcngc fmctlon of VIbntional cncrgy dwrbulcd m CO+(A Zn).(/vJ. ws estimated to be 0.20 i 0

SO+(A2Π-X2Πr) emission produced from a d
✍ Masaharu Tsuji; Chikashi Yamagiwa; Minoru Endoh; Yukio Nishimura 📂 Article 📅 1980 🏛 Elsevier Science 🌐 English ⚖ 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+(Ã 2Π
✍ Masaharu Tsuji; John P. Maier; Hiroshi Obase; Hiroshi Sekiya; Yukio Nishmura 📂 Article 📅 1987 🏛 Elsevier Science 🌐 English ⚖ 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

CS2+(A-X) emission produced from the cha
✍ Minoru Endoh; Masaharu Tsuji; Yukio Nishimura 📂 Article 📅 1984 🏛 Elsevier Science 🌐 English ⚖ 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+(B—X) Emission produced from the ther
✍ Hiroshi Obase; Masaharu Tsuji; Yukio Nishimura 📂 Article 📅 1984 🏛 Elsevier Science 🌐 English ⚖ 250 KB

\(\mathrm{N}_{2}^{+}\left(\mathrm{B}^{2} \Sigma_{\mathrm{u}}^{+}-\mathrm{X}^{2} \Sigma_{\mathrm{g}}^{+}\right)\)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