Integral cross sections for the electron-impact excitation of the b 1Πu, c3 1Πu, o3 1Πu, b 1Σu+, c4 1Σu+, G 3Πu, and F 3Πu states of N2

Charles P. Malone, Paul V. Johnson, Xianming Liu, Bahar Ajdari, Isik Kanik, and Murtadha A. Khakoo
Phys. Rev. A 85, 062704 – Published 18 June 2012

Abstract

Integral cross sections for electron-impact excitation out of the ground-state level X1Σg+(v=0) to the b1Πu, c31Πu, o31Πu, b1Σu+, c41Σu+, G3Πu, and F3Πu electronic states in N2 are reported at incident energies ranging between 17.5 and 100 eV. We also provide excitation cross sections using emission-based excitation shape functions and optical oscillator strengths. These cross-section results are of great importance to planetary atmospheric modeling of the emissions observed in Earth's atmosphere as well as those of Titan and Triton, the largest moons of Saturn and Neptune, respectively. Critical comparisons of the present cross sections with previous values are presented in an effort to provide improved cross sections for electron excitation of this fundamental molecule's important transitions.

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  • Received 5 April 2012

DOI:https://doi.org/10.1103/PhysRevA.85.062704

©2012 American Physical Society

Authors & Affiliations

Charles P. Malone1,2, Paul V. Johnson1, Xianming Liu3, Bahar Ajdari2, Isik Kanik1, and Murtadha A. Khakoo2

  • 1Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, California 91109, USA
  • 2Department of Physics, California State University Fullerton, Fullerton, California 92831, USA
  • 3Planetary and Space Science Division, Space Environment Technologies, 1676 Palisades Drive, Pacific Palisades, California 90272, USA

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Vol. 85, Iss. 6 — June 2012

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