Extinction of Titan haze at 3 micron

DOI

The chemical nature of the Titan haze is poorly understood. The investigation carried out by the Cassini-Huygens suite of instruments is bringing new insights into this question. This work aims at deriving the vertical variation of the spectral structure of the 3.3-3.4um absorption feature of the Titan haze from Cassini VIMS solar occultation data recorded between 250 and 700km altitude.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35730021
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/573/A21
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/573/A21
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/573/A21
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/573/A21
Provenance
Creator Courtin R.; Kim S.J.; Bar-Nun A.
Publisher CDS
Publication Year 2014
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy