Date of Award
Spring 2025
Document Type
Dissertation
Degree Name
Doctor of Philosophy (PhD)
Department
Physics
Program/Concentration
Physics
Committee Director
Peter Bernath
Committee Member
Charles Sukenik
Committee Member
Colm Whelan
Committee Member
Craig Bayse
Committee Member
Balša Terzić
Abstract
Planetary atmospheres are frequently studied using a number of spectroscopic methods. One of these is observing spectra to analyze what molecules are present or chemical reactions may be taking place. To this end, we have produced a line list of the electronic a1Δ−X3Σ− and b1Σ+−X3Σ− transitions of SO. Additionally, a line list pure rovibrational transitions of the a1Δ and X3Σ− states were produced, but lacked the necessary experimental data for the b1Σ+ state. These line lists can be used in further studies, such as for identifying SO abundances on Io, a moon of Jupiter. Cross-section data of cyclopentane as well as collision-induced absorption data of N2-N2, CH4-CH4, and N2-CH4 were taken using a Fourier transform spectrometer, for use in further studies modeling organic molecules in the atmosphere of Titan, a moon of Saturn. Atmospheric Chemistry Experiment (ACE) satellite data was analyzed to produce an atlas of clouds and aerosols for qualitative identification in spectra. Volcanic ash was fitted using Mie scattering calculations, experimental optical constants, and real ACE observations using a bimodal lognormal size distribution. Doppler shifts in ACE data can be used to derive line-of-sight winds, useful in mapping upper atmospheric motion. This wind data was validated against other experimental observations, showing a small shift in ACE measurements.
Rights
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DOI
10.25777/p66x-9k65
ISBN
9798280747463
Recommended Citation
Johnson, Ryan M..
"Planetary Atmospheres"
(2025). Doctor of Philosophy (PhD), Dissertation, Physics, Old Dominion University, DOI: 10.25777/p66x-9k65
https://digitalcommons.odu.edu/physics_etds/215
ORCID
0000-0001-6363-8499