자료유형 | 학위논문 |
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서명/저자사항 | Assessing the Impact of H2O and CH4 Opacity Data in Exoplanetary Atmospheres: Laboratory Measurements and Radiative Transfer Modeling Approaches. |
개인저자 | Gharib-Nezhad, Ehsan. |
단체저자명 | Arizona State University. Chemistry. |
발행사항 | [S.l.]: Arizona State University., 2019. |
발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2019. |
형태사항 | 128 p. |
기본자료 저록 | Dissertations Abstracts International 81-05B. Dissertation Abstract International |
ISBN | 9781088373958 |
학위논문주기 | Thesis (Ph.D.)--Arizona State University, 2019. |
일반주기 |
Source: Dissertations Abstracts International, Volume: 81-05, Section: B.
Advisor: Line, Michael R. |
이용제한사항 | This item must not be sold to any third party vendors. |
요약 | One strategic objective of the National Aeronautics and Space Administration (NASA) is to find life on distant worlds. Current and future missions either space telescopes or Earth-based observatories are frequently used to collect information through the detection of photons from exoplanet atmospheres. The primary challenge is to fully understand the nature of these exo-atmospheres. To this end, atmospheric modeling and sophisticated data analysis techniques are playing a key role in understanding the emission and transmission spectra of exoplanet atmospheres. Of critical importance to the interpretation of such data are the opacities (or absorption cross-sections) of key molecules and atoms. During my Doctor of Philosophy years, the central focus of my projects was assessing and leveraging these opacity data. I executed this task with three separate projects: 1) laboratory spectroscopic measurement of the infrared spectra of CH4 in H2 perturbing gas in order to extract pressure-broadening and pressure-shifts that are required to accurately model the chemical composition of exoplanet atmospheres |
일반주제명 | Atmospheric chemistry. Astrophysics. Physical chemistry. |
언어 | 영어 |
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