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AGU: Journal of Geophysical Research, Space Physics

 

Keywords

  • Nitrogen VUV emission
  • dayglow
  • transition probability

Index Terms

  • Atmospheric Composition and Structure: Airglow and aurora
  • Planetary Sciences: Solar System Objects: Titan
  • Atmospheric Composition and Structure: Planetary atmospheres
  • Atmospheric Composition and Structure: Radiation: transmission and scattering
  • Mathematical Geophysics: Spectral analysis
Abstract
Cited By (3)
 

Abstract

Experimental and coupled-channels investigation of the radiative properties of the N2 c4 1Σu+X 1Σg+ band system

Xianming Liu

Planetary and Space Science Division, Space Environment Technologies, Pasadena, California, USA

Donald E. Shemansky

Planetary and Space Science Division, Space Environment Technologies, Pasadena, California, USA

Charles P. Malone

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Paul V. Johnson

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Joseph M. Ajello

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Isik Kanik

Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA

Alan N. Heays

Research School of Physical Sciences and Engineering, The Australian National University, Canberra, Australian Capital Territory, Australia

Brenton R. Lewis

Research School of Physical Sciences and Engineering, The Australian National University, Canberra, Australian Capital Territory, Australia

Stephen T. Gibson

Research School of Physical Sciences and Engineering, The Australian National University, Canberra, Australian Capital Territory, Australia

Glenn Stark

Department of Physics, Wellesley College, Wellesley, Massachusetts, USA

The emission properties of the N2 c4 1Σ u +X 1Σ g + band system have been investigated in a joint experimental and coupled-channels theoretical study. Relative intensities of the c4 1Σ u +(0) − X 1Σ g +(v i ) transitions, measured via electron-impact-induced emission spectroscopy, are combined with a coupled-channel Schrödinger equation (CSE) model of the N2 molecule, enabling determination of the diabatic electronic transition moment for the c4 1Σ u +X 1Σ g + system as a function of internuclear distance. The CSE rotational transition probabilities are further verified by comparison with a high-resolution experimental spectrum. Spontaneous transition probabilities of the c4 1Σ u +X 1Σ g + band system, required for modeling atmospheric emission, can now be calculated reliably.

Received 31 August 2007; accepted 6 November 2007; published 14 February 2008.

Citation: Liu, X., D. E. Shemansky, C. P. Malone, P. V. Johnson, J. M. Ajello, I. Kanik, A. N. Heays, B. R. Lewis, S. T. Gibson, and G. Stark (2008), Experimental and coupled-channels investigation of the radiative properties of the N2 c4 1Σu+X 1Σg+ band system, J. Geophys. Res., 113, A02304, doi:10.1029/2007JA012787.

Cited By

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