Auroras are (generally) high‐latitude atmospheric emissions that result from the precipitation
of energetic charged particles from a planet's magnetosphere. Auroral emissions from the …

This paper describes the status of the 2008 edition of the HITRAN molecular spectroscopic
database. The new edition is the first official public release since the 2004 edition, although …

Chemical and physical processes which may give rise to isotope fractionation of molecular
species in the atmospheres of both Earth and other planets are reviewed, along with …

SINCE their detection in the high latitudes of Jupiter, first by the Voyager Ultraviolet
Spectrometer (UVS) experiment1, 2, then by the International Ultraviolet Explorer (IDE) …

The updated 2009 edition of the spectroscopic database GEISA (Gestion et Etude des
Informations Spectroscopiques Atmosphériques; Management and Study of Atmospheric …

We present our current understanding of the composition, vertical mixing, cloud structure
and the origin of the atmospheres of Jupiter and Saturn. Available observations point to a …

New developments have led to this update of the composition and origin of Jupiter's
atmosphere that were originally discussed in our Planet. Space Sci. 47 (1999) 1243 paper …

We present a study of the formation and distribution of benzene (C6H6) on Titan. Analysis of
the Cassini Mass Spectrometer (INMS) measurements of benzene densities on 12 Titan …

PAHs are important components of the interstellar medium and carbonaceous chondrites,
but have never been identified in the reducing atmospheres of the outer solar system …

Benzene is a simple neutral aromatic compound found in molecular clouds, comets, and
planetary atmospheres. It has been confirmed on Jupiter, Saturn, Titan, and is expected on …