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PTAL is a H2020 project (2016-2021) consisting of preparing the analysis of in situ space missions (such as Rovers Perseverance, Curiosity, ExoMars) which have near-infrared, Raman, X-ray diffraction and LIBS spectroscopic instruments. The project consisted in observing several analogous samples of planetary surfaces with space or laboratory instruments in order to make a spectral database. This work was done in collaboration with the University of Oslo and the University of Valladolid. The data is accessible on the site https://ptal.eu/ and the associated publications on https://ptal.eu/publications

 

Contact : François Poulet

 

Project Status :
Ended

http://stereo.jhuapl.edu/

Data access: http://idc-solar.ias.u-psud.fr/

 

STEREO (Solar TErrestrial Relations Observatory) is a NASA mission composed of two nearly identical spacecraft that provide us with unprecedented three dimensional views of our Sun. STEREO was successfullly lauched by a Delta II rocket on October 25, 2006 at 8:52pm EDT from Cape Canaveral in Florida.

 

Project Status :
Past

The Sun and its corona as seen by HECOR and HEIT: preliminary results
Launched on September 14, 2009 from White Sands Missile Range (New Mexico), the Herschel sounding rocket was carrying two experiments with strong IAS participation: HECOR and HEIT.

Project Status :
Past

http://smsc.cnes.fr/PICARD/

 

PICARD is a survey on the simultaneous measurement of the absolute total and spectral solar irradiance, solar diameter and shape, and the interior of the Sun by helioseismologic survey.

These measurements obtained throughout the mission will enable study of their variations as a function of solar activity.

 

Contact: P.Boumier

 

Project Status :
Past

PLATO (PLAnetary Transits and Oscillations of stars) a été sélectionnée comme mission M3 du programme Cosmic Vision de l'ESA. Le lancement est prévu en 2026. Son but est de décrire les systèmes stellaires observés et d'en caractériser les planètes.

L'équipe sera fortement impliquée dans le segment sol (ainsi que dans l'analyse scientifique).

 

Contacts: M. Ollivier (pour la partie exoplanètes) et T. Appourchaux (pour la partie stellaire)
 

Project Status :
En développement

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