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N:Peterlongo; Marie;;; 
FN: Marie Peterlongo 
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<lom:entry>Exoplanete-SESP-FluxUV</lom:entry>
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<lom:string language="fre">Flux UV</lom:string>
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<lom:string language="fre">Ce chapitre présente les principales émissions UV observées dans les hautes atmosphères des planètes. On décrit non seulement les émissions aurorales que l'on peut observer dans le visible depuis la surface de la Terre, mais aussi d'autres émissions plus ténues qui nous donnent des informations sur la composition, la dynamique et la variabilité des hautes atmosphères planétaires. Les différents processus à l'origine de ces émissions : interaction du rayonnement solaire avec l'atmosphère, précipitation de particules énergétiques, réactions chimiques, etc... sont décrits et illustrés par différents exemples dans le système solaire. Ce cours est accompagné d'exercices. </lom:string>
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<lom:entity>BEGIN:VCARD 
VERSION:3.0 
N:Chauffray;Jean-Yves;;; 
FN:Jean-Yves Chauffray
ORG:Université de Versaille Saint-Quentin UVSQ;LATMOS; 
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<lom:dateTime>2016-08-25</lom:dateTime>
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<lom:entity>BEGIN:VCARD 
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N: ;;;; 
FN: Observatoire de Paris
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N: ;;;; 
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