Constraints on Titan's middle atmosphere ammonia abundance from Herschel/SPIRE sub-millimetre spectra

Sub-millimetre spectra measured with Herschel's SPIRE Fourier Transform Spectrometer were used to search for ammonia (NH3) in Titan's stratosphere. Observations were taken during 2010 and 2011, just after Titan's northern spring equinox, which occurred in mid-2009. In our analysis we...

Täydet tiedot

Bibliografiset tiedot
Päätekijät: Teanby, N, Irwin, P, Nixon, C, Courtin, R, Swinyard, B, Moreno, R, Lellouch, E, Rengel, M, Hartogh, P
Aineistotyyppi: Journal article
Kieli:English
Julkaistu: 2013

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