Bekki, Y.: Numerical study of non-toroidal inertial modes with l = m + 1 radial vorticity in the Sun's convection zone. Astronomy and Astrophysics 682, p. A39 (2024)
Bekki, Y.; Cameron, R. H.; Gizon, L.: The Sun's differential rotation is controlled by high-latitude baroclinically unstable inertial modes. Science Advances 10, p. eadk5643 (2024)
Bekki, Y.; Cameron, R. H.: Three-dimensional non-kinematic simulation of the post-emergence evolution of bipolar magnetic regions and the Babcock-Leighton dynamo of the Sun. Astronomy and Astrophysics 670, p. A101 (2023)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Amplitudes of equatorial modes from a nonlinear rotating convection simulation. Astronomy and Astrophysics 666, p. A135 (2022)
Bekki, Y.; Cameron, R. H.; Gizon, L.: Theory of solar oscillations in the inertial frequency range: Linear modes of the convection zone. Astronomy and Astrophysics 662, p. A16 (2022)
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, ...
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.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.