[HTML][HTML] Titan's cold case files-Outstanding questions after Cassini-Huygens
The entry of the Cassini-Huygens spacecraft into orbit around Saturn in July 2004 marked
the start of a golden era in the exploration of Titan, Saturn's giant moon. During the Prime …
the start of a golden era in the exploration of Titan, Saturn's giant moon. During the Prime …
Organic ices in Titan's stratosphere
Titan's stratospheric ice clouds are by far the most complex of any observed in the solar
system, with over a dozen organic vapors condensing out to form a suite of pure and co …
system, with over a dozen organic vapors condensing out to form a suite of pure and co …
Study of Titan's fall southern stratospheric polar cloud composition with Cassini/CIRS: Detection of benzene ice
S Vinatier, B Schmitt, B Bézard, P Rannou, C Dauphin… - Icarus, 2018 - Elsevier
We report the detection of a spectral signature observed at 682 cm− 1 by the Cassini
Composite Infrared Spectrometer (CIRS) in nadir and limb geometry observations of Titan's …
Composite Infrared Spectrometer (CIRS) in nadir and limb geometry observations of Titan's …
The SPECTRAL ice chamber: application to Titan's stratospheric ice clouds
CM Anderson, D Nna-Mvondo… - The Astrophysical …, 2018 - iopscience.iop.org
An ice chamber for obtaining thin-film transmission spectra of Titan-relevant organic ices
between 50 and 11,700 cm− 1 (200–0.85 μm) is described in detail in this work. The ice …
between 50 and 11,700 cm− 1 (200–0.85 μm) is described in detail in this work. The ice …
Experimental Simulation of the Volatile Hydrocarbons Generated by the Long-UV Photoprocessing of (C6H6) Ices with Relevance to Titan's Southern Stratospheric Ice …
Ice clouds containing benzene (C 6 H 6) have recently been detected in the stratosphere at
the south pole of Titan. Their subsequent aging process induced by long-UV solar photons …
the south pole of Titan. Their subsequent aging process induced by long-UV solar photons …
HCN-C₆H₆ co-condensed ice cloud in Titan's stratosphere: Laboratory study of the CIRS-observed HASP cloud
DN Mvondo, CM Anderson, RE Samuelson - 2019 - mdsoar.org
For thirteen years, the Cassini mission to explore Saturn and its icy moons has provided a
large repository of data on Titan's atmosphere. Ice clouds have been repeatedly observed in …
large repository of data on Titan's atmosphere. Ice clouds have been repeatedly observed in …
[PDF][PDF] Investigating Titan's C6H6 stratospheric ices and HASP cloud aging under long-UV radiations
J Mouzay… - EPSC-DPS …, 2019 - meetingorganizer.copernicus.org
The stratosphere of Titan is a complex environment in which solid particles as high altitude-
produced aerosols and vapor phase compounds meet, submitted to long-UV photons …
produced aerosols and vapor phase compounds meet, submitted to long-UV photons …
[PDF][PDF] HCN-C6H6 co-condensed ice cloud in Titan's stratosphere: Laboratory study of the CIRS-observed HASP cloud
For thirteen years, the Cassini mission to explore Saturn and its icy moons has provided a
large repository of data on Titan's atmosphere. Ice clouds have been repeatedly observed in …
large repository of data on Titan's atmosphere. Ice clouds have been repeatedly observed in …
[PDF][PDF] Identifying the enigmatic Haystack and HASP ice clouds observed by CIRS in Titan's stratosphere
Stratospheric ice clouds have been repeatedly observed in Titan's atmosphere by the
Cassini Composite InfraRed Spectrometer (CIRS) since the Cassini spacecraft entered into …
Cassini Composite InfraRed Spectrometer (CIRS) since the Cassini spacecraft entered into …