CO Cameron band and CO2+ UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production-Reference-Cited by-同舟云学术

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CO Cameron band and CO2+ UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production

Published:2013-06 Issue:6 Volume:118 Page:3660-3671
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Bhardwaj Anil¹,Jain Sonal Kumar¹

Affiliation:

1. Space Physics Laboratory; Vikram Sarabhai Space Centre; Trivandrum India

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/jgra.50345/fullpdf

Reference51 articles.

1. Emission cross sections of CO2 by electron impact in the interval 1260-4500 Å;Ajello;J. Chem. Phys.,1971a

2. Emission cross section of CO by electron impact in the interval 1260-5000 Å;Ajello;J. Chem. Phys.,1971b

3. Venera 11 and Venera 12 observations of EUV Emissions from the upper atmosphere of Venus;Bertaux;Planet. Space Sci.,1981

4. On the role of solar EUV, photoelectrons, and auroral electrons in the chemistry of (C1D) and the production of CI 1931 Å in the inner cometary coma: A case for comet P/Halley;Bhardwaj;J. Geophys. Res.,1999

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1. Modified quantum defect theory: application to analysis of high-resolution Fourier transform spectra of neutral oxygen;The European Physical Journal D;2024-04

2. Model for Nitric oxide and its dayglow emission in the martian upper atmosphere using NGIMS/MAVEN measured neutral and ion densities;Icarus;2022-08

3. Modeling of Diffuse Auroral Emission at Mars: Contribution of MeV Protons;Journal of Geophysical Research: Space Physics;2022-01

4. Laboratory Study of the Cameron Bands, the First Negative Bands, and Fourth Positive Bands in the Middle Ultraviolet 180–280 nm by Electron Impact Upon CO;Journal of Geophysical Research: Planets;2021-01

5. CO+ first-negative band emission: A tracer for CO in the Martian upper atmosphere;Astronomy & Astrophysics;2020-07

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