Vertical profiles of HCN, HC3N, and C2H2 in Titan's atmosphere derived from Cassini/CIRS data

Mid-infrared limb spectra in the range 600-1400 cm-1 taken with the Composite InfraRed Spectrometer (CIRS) on-board the Cassini spacecraft were used to determine vertical profiles of HCN, HC3N, C2H2, and temperature in Titan's atmosphere. Both high (0.5 cm-1) and low (13.5 cm-1) spectral resolu...

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Hlavní autoři:	Teanby, N, Irwin, P, de Kok, R, Vinatier, S, Bezard, B, Nixon, C, Flasar, F, Calcutt, S, Bowles, N, Fletcher, L, Howett, C, Taylor, F
Médium:	Journal article
Jazyk:	English
Vydáno:	2007

Vertical profiles of HCN, HC3N, and C2H2 in Titan's atmosphere derived from Cassini/CIRS data

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