Spectroscopic Parameter Requirements For Remote Sensing Of Terrestrial Planets

Mary Ann H. Smith
Planetary scientists seek to determine the compositions, dynamics, energetics, and chemical behaviors of planetary atmospheres through measurements of atmospheric absorption or emission in a number of wavelength regions. Laboratory studies of molecular spectra are often required to properly interpret telescope and spacecraft observations, particularly for atmospheres of planets such as Mars and Venus that have compositions and temperature and pressure regimes quite di’erent from those in the Earth's atmosphere. While many of the necessary spectroscopic...
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