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...
المؤلفون الرئيسيون: | Teanby, N, Irwin, P, Nixon, C, Courtin, R, Swinyard, B, Moreno, R, Lellouch, E, Rengel, M, Hartogh, P |
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التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2013
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مواد مشابهة
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Constraints on Titan's middle atmosphere ammonia abundance from Herschel/SPIRE sub-millimetre spectra
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