INFRARED AURORAE IN THE SOLAR SYSTEM Infrared Aurorae in the Solar System Tom Stallard ATMOSPHERIC PHYSICS LABORATORY DEPARTMENT OF PHYSICS AND ASTROMONY.

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INFRARED AURORAE IN THE SOLAR SYSTEM Infrared Aurorae in the Solar System Tom Stallard ATMOSPHERIC PHYSICS LABORATORY DEPARTMENT OF PHYSICS AND ASTROMONY Steve Miller, Henrik Melin, Makenzie Lystrup and the Cassini community, especially: Emma Bunce, Chris Arridge, Nick Achilleos and Michele Dougherty

INFRARED AURORAE IN THE SOLAR SYSTEM H 3 + formation H 2 + h =H e H 2 + e*=H e + e H H 2 =H H H 3 + destruction H X=HX + + H 2 H e - =H + H 2 Hydrocarbons

INFRARED AURORAE IN THE SOLAR SYSTEM Infrared (Connerney et al) Ultraviolet (Clarke et al) Imaging: Jupiter

INFRARED AURORAE IN THE SOLAR SYSTEM Saturn

INFRARED AURORAE IN THE SOLAR SYSTEM Uranus

INFRARED AURORAE IN THE SOLAR SYSTEM Spectroscopy: Jupiter

INFRARED AURORAE IN THE SOLAR SYSTEM Multiple line spectroscopy provides: emission intensities temperature composition cooling rates vertical thermal profile atmospheric densities

INFRARED AURORAE IN THE SOLAR SYSTEM IR observations of Jupiter

INFRARED AURORAE IN THE SOLAR SYSTEM Temperature

INFRARED AURORAE IN THE SOLAR SYSTEM Cooling

INFRARED AURORAE IN THE SOLAR SYSTEM Ion Winds

INFRARED AURORAE IN THE SOLAR SYSTEM

High resolution observations of Saturn

INFRARED AURORAE IN THE SOLAR SYSTEM

Compared with the UV emission

INFRARED AURORAE IN THE SOLAR SYSTEM 1.3” smear

INFRARED AURORAE IN THE SOLAR SYSTEM Infilled Extended Flanks

INFRARED AURORAE IN THE SOLAR SYSTEM

Saturn Jupiter

INFRARED AURORAE IN THE SOLAR SYSTEM Saturn Jupiter Co-rotation breakdown

INFRARED AURORAE IN THE SOLAR SYSTEM Saturn Jupiter Co-rotation breakdownOuter effects

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