Portier-Fozzani, F.; Aschwanden, M.; Démoulin, P.; Neupert, W.; Delaboudinière, J.-P.; the EIT Team: Measurement of coronal magnetic twists during loop emergence of NOAA 8069. Solar Physics 203, pp. 289 - 308 (2001)
Portier-Fozzani, F.; Inhester, B.: 3D Coronal structures and their evolutions measured by Stereoscopy, consequences for Space Weather and the STEREO mission. Space Science Reviews 97 (1/4), p. 51 (2001)
Portier-Fozzani, F.; Vandame, B.; Bijaoui, A.; Maucherat, A. J.; EIT Team: A multiscale vision model applied to analyze EIT images of the solar corona. Solar Physics 201, p. 271 (2001)
Portier-Fozzani, F.: 3D Coronal Observations with the Solar Cycle. In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, SOLSPA 2001,, pp. 159 - 162 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
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The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.