On the detectability of Jovian oscillations with infrared heterodyne measurements
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The abundance of H <inf>2</inf> in Titans troposphere from the Cassini CIRS investigation
2012, Planetary and Space ScienceCitation Excerpt :A measurement of the H2 mole fraction in the range 200–1000 km would be extremely valuable in assessing the reality of such a gradient, and in characterizing it, if indeed it exists. In theory, the measurement of the H2 quadupole lines—the S(0) line at 354.37 cm−1, the S(1) line at 587.03 cm−1, or the S(2) line at 814.42 cm−1—through heterodyne techniques could provide such a test, although the technical feasibility of this kind of observation is not obvious (Mosser et al., 1992). Another test, concerning the plausibility of the “downdraft” interpretation for the H2 polar enhancement, will be to monitor the latitude profile of the H2 mole fraction at the time of equinox and afterwards.
High resolution diode laser and heterodyne spectroscopy with applications toward remote sensing
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