Events
Seminar
Polycyclic aromatic hydrocarbons (PAHs) in Titan's Upper Atmosphere
Tuesday, 26 August 2014, 15:00-16:00
Gebäude: 435, Raum 2.05
Observations of Titan's atmosphere made with the VIMS instrument on board the CASSINI satellite show a strong limb emission around 3.3 µm at high atmospheric altitudes (above 700 km). This emission exhibits the typical spectral signatures of the strong CH4 bands. A detailed analysis of the spectra reveals, however, an additional strong emission centered at 3.28 µm and peaking at about 950 km. We have untangled this spectral emission and found it produced by large amount of heavy polycyclic aromatic hydrocarbons (PAH's). I will describe this research and will briefly discuss about the important consequences of this finding on the origin of Titan's main haze layer.
This event is part of the eventgroup Meteorology Colloquium Karlsruhe
Speaker
Prof. Dr. Manuel Lopez-Puertas
Instituto de Astrofisica de Andalucia (CSIC), Granada, Spain
Prof. Dr. Manuel Lopez-Puertas
Instituto de Astrofisica de Andalucia (CSIC), Granada, Spain
Organizer
Prof. Dr. J. Orphal
IMK-ASF
Karlsruher Institut für Technologie (KIT)
Karlsruhe
Tel: +49 721 608 29121
Fax: +49 721 608 24742
Mail: johannes orphal ∂ kit edu
Prof. Dr. J. Orphal
IMK-ASF
Karlsruher Institut für Technologie (KIT)
Karlsruhe
Tel: +49 721 608 29121
Fax: +49 721 608 24742
Mail: johannes orphal ∂ kit edu
Targetgroup
Scientific Staff
Scientific Staff