CO^+ Comet-Tail Emission and Chemiluminescence in Collisions of N^+ Ions with CO Molecules in the Energy Range 10-300 eV

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概要

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• Light emission in collisions of N + ion beams with CO molecules was observed in the LAB energy range l0-300 eV. Intense emission due to the transition A 2H-X 2E of CO + formed by charge transfer was observed and used to determine the vibrational population distribution in the upper electronic energy state. The distribution is different from that produced in the Ar+<:O or the Nt-CO col-lision system. Chemiluminescence which is presumed to be due to excited CN + ions formed in the reactive collisions of N + with CO was observed in the spectral range shorter than 3 100 A and at collision energies of 40-150 eV. Line spectra of C(3s IP-2p2 ID and 3s IP-2p2 IS) were also clearly found. C(3s IP) atoms, at least part of them, are thought to be produced by another branch of the reaction of N + with CO.

• 社団法人日本物理学会の論文
• 1981-10-15

著者

• Sasaki Hiromi

  Laboratory Of Physiological Sciences Faculty Of Human Sciences Waseda University

• Inouye H

  Hirao Active Glass Project Erato Jst Keihanna-plaza

• Sasaki H

  Tohoku Gakuin Univ. Miyagi

• Sasaki Hisashi

  Department Of Physics Division Of Material Science Nagoya University

• Inouye Hokotomo

  Research Institute For Scientific Measurements

• Sasaki Hiromi

  Research Institute For Scientific Measurements Tohoku University

• Ishikawa Toshiaki

  Research Institute for Scientific Measurements, Tohoku University

• Ishikawa Toshiaki

  Research Institute For Scientific Measurements Tohoku University

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