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Stellar and Solar Physics

Our team aims at providing answers to some key questions of solar and stellar physics, such as the heating process of the corona or the structure of solar and stellar interiors. The magnetic field playing a fundamental role in structuring the atmospheres of solar-type stars, it becomes possible to understand the coupling between the internal generation of magnetic field and its external signatures. The two major research topics are thus the dynamic and internal structure of the Sun and stars, and diagnostic and heating of the outer layers.

 

 

 

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Dernières news

4 weeks 21 hours ago

The SPICE instrument on board ESA's Solar Orbiter mission has successfully obtained its first measurements of the Sun on April 21, 2020. This is a major step for the instrument and for the mission, which was launched on February 10, 2020 and is currently on its way to study the Sun closely.

7 months 13 hours ago

During the Mercury transit on November the 11th, 2019, IAS researchers and the ALCOR astronomy club will organize an afternoon with observations of the Sun, conferences, and workshops. This event will take place on the University campus at the new physics teaching building, "hbar" (building 625).

7 months 2 weeks ago

ESA’s Solar Orbiter mission has completed its test campaign in Europe and is now being packed ready for its journey to Cape Canaveral at the end of this month, ahead of launch in February 2020.

1 year 3 weeks ago

The CLASP-2 telescope was successfully launched on April 11th 2019 by a sounding rocket from White Sands Missile Range (New Mexico, USA). The objective of the CLASP (Chromospheric LAyer SPectropolarimeter) project is to measure the magnetic field in the solar chromosphere using spectro-polarimetric measurements in the ultraviolet.

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