Extinction of Titan haze at 3 micron Virtual Observatory Resource

Authors

1. Courtin R.
2. Kim S.J.
3. Bar-Nun A.

Published by

CDS

Abstract

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.

Keywords

1. solar-system
2. solar-system-planets
3. extinction

Bibliographic source Bibcode

2015A&A...573A..21C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/573/A21

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/573/A21

Document Object Identifer DOI

doi:10.26093/cds/vizier.35730021

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