• PMR-Database

    - A database of Photochemical Model Results -

    Planetary atmospheres are complex systems where numerous physical and chemical processes take place.
    In order to understand what really happens in these atmospheres, scientists develop specific models, usually called photochemical models.
    These models include the major processes that control their composition.

    In the following pages, we present the latest results our team obtained from the photochemical models we have developed for various planetary atmospheres.
    You will be able to see figures of abundance profiles of all species included in our models (with references to the corresponding papers).
    Text files are also available to facilitate their use by observers and other modelers.

    Presentation and motivations in this short article

    Click on a planet to see theoretical abundance profiles

    Neptune Triton Titan Jupiter Jupiter
    Neptune's atmosphere Triton's atmosphere Titan's atmosphere Jupiter's atmosphere Saturn's atmosphere
Design and construction: Sylvia Lopez and Michel Dobrijevic

About me

Dr. Michel Dobrijevic

LAB - Laboratoire d'Astrophysique de Bordeaux
OASU - Observatoire Aquitain des Sciences de l'Univers
Université de Bordeaux