Thesis (M.S.) University of Alaska Fairbanks, 2005A synthetic spectrum of the N₂ Vegard-Kaplan (VK) bands is developed for dayglow conditions at thermospheric altitudes. Due to the change in electron spin, the A³Eu state is metastable (lifetime 2-3 s.) and excited from the X¹Eg⁺ ground state primarily by photo-electron impact. Cascade from higher-energy triplets contributes to the A³Eu⁺ population and, due to its long lifetime, losses due to quenching are significant. Because of quenching, the VK bands were the last of the major N₂ emissions to be observed, as is explained in an historical review of the work of Vegard and Kaplan. Taking as inputs the solar soft x-ray measurements of the Student Nitric Oxide Explorer (SNOE), the model comput...
Recently the Cassini Ultraviolet Imaging Spectrograph (UVIS) has revealed the presence of N<sub>2</s...
[1] P. G. Wilkinson and R. S. Mulliken, J. Chem. Phys. 31, 674 (1959). [2] D. A. Ramsay, Can. J. Phy...
A model for N2 triplet states band emissions in the Venusian dayglow has been developed for low and ...
The First Negative (1N) band emission of the molecular nitrogen ion, N⁺₂ , is one of the most promin...
The vibrational distribution of N₂ triplet states in the sunlit upper thermosphere of Earth is measu...
A model for N2 Vegard-Kaplan band (A 3Σ+u −X1Σ+g) emissions in Martian dayglow has been developed to...
A model for N<SUB>2</SUB> Vegard-Kaplan (VK) band (A<SUP>3</SUP>Σ<SUB>u</SUB><SUP>+</SUP>−X<SUP>1</S...
Lower thermospheric airglow spectra in the wavelength range of 1840 A to 2280 A were analyzed. Thes...
Ultraviolet (UV) spectra obtained from Earth’s dayglow contain important information for understandi...
Spectrograph, wavelength standards, light source, and resolution analysis for Vegard-Kaplan bands em...
Recently the Cassini Ultraviolet Imaging Spectrograph (UVIS) has revealed the presence of N2 Vegard-...
Author Institution: Molecular Physics Laboratory, SRI International; University of California Observ...
plorer (FUSE) obtained spectra of the terrestrial day airglow between 905 and 1184 A ̊ from an altit...
A custom made five panel filter mosaic window was designed, installed and operated with the HiTIES (...
The spectroscopy of the υ = 1 → υ = 0 fundamental vibration-rotation band of nitric oxide (NO) in Ea...
Recently the Cassini Ultraviolet Imaging Spectrograph (UVIS) has revealed the presence of N<sub>2</s...
[1] P. G. Wilkinson and R. S. Mulliken, J. Chem. Phys. 31, 674 (1959). [2] D. A. Ramsay, Can. J. Phy...
A model for N2 triplet states band emissions in the Venusian dayglow has been developed for low and ...
The First Negative (1N) band emission of the molecular nitrogen ion, N⁺₂ , is one of the most promin...
The vibrational distribution of N₂ triplet states in the sunlit upper thermosphere of Earth is measu...
A model for N2 Vegard-Kaplan band (A 3Σ+u −X1Σ+g) emissions in Martian dayglow has been developed to...
A model for N<SUB>2</SUB> Vegard-Kaplan (VK) band (A<SUP>3</SUP>Σ<SUB>u</SUB><SUP>+</SUP>−X<SUP>1</S...
Lower thermospheric airglow spectra in the wavelength range of 1840 A to 2280 A were analyzed. Thes...
Ultraviolet (UV) spectra obtained from Earth’s dayglow contain important information for understandi...
Spectrograph, wavelength standards, light source, and resolution analysis for Vegard-Kaplan bands em...
Recently the Cassini Ultraviolet Imaging Spectrograph (UVIS) has revealed the presence of N2 Vegard-...
Author Institution: Molecular Physics Laboratory, SRI International; University of California Observ...
plorer (FUSE) obtained spectra of the terrestrial day airglow between 905 and 1184 A ̊ from an altit...
A custom made five panel filter mosaic window was designed, installed and operated with the HiTIES (...
The spectroscopy of the υ = 1 → υ = 0 fundamental vibration-rotation band of nitric oxide (NO) in Ea...
Recently the Cassini Ultraviolet Imaging Spectrograph (UVIS) has revealed the presence of N<sub>2</s...
[1] P. G. Wilkinson and R. S. Mulliken, J. Chem. Phys. 31, 674 (1959). [2] D. A. Ramsay, Can. J. Phy...
A model for N2 triplet states band emissions in the Venusian dayglow has been developed for low and ...