Team leaders
- Laurent Gizon (lead)
professor, MPI for Solar System Research, Germany
Expertise: Helioseismology. Contributed to the first papers reporting the discovery and identification of solar inertial modes. - Rhita-Maria Ouazzani (co-lead)
Associate astronomer, LIRA Observatoire de Paris-PSL, France
Expertise: modeling of stellar pulsations including effect of rotation and magnetic field in 2D. Contributed to the first paper reporting the detection of pure inertial modes in stars.
Team experts
- Victoria Antoci, senior researcher, DTU Technical University of Denmark
Asteroseismic and spectrocopic data analysis of rotational and pulsational variables. Specialist of intermediate-mass stars (Leader of Kepler WG4: A- and F-type stars). - Yuto Bekki, postdoc, MPI for Solar System Research, Germany
Realistic linear models of solar inertial modes; Nonlinear evolution of baroclinicaly unstable high-latitude modes. - Lisa Bugnet, assistant professor, Institute of Science and Technology Austria
Modeling of stellar pulsations using perturbative approaches. Seismic inferences of magnetic fields in sellar interiors. - Nick Featherstone, lead scientist, SWRI Boulder, USA
State-of-the-art numerical simulations of solar rotating magnetoconvection. - Hideyuki Hotta, professor, ISEE Nagoya, Japan
State-of-the-art numerical simulations of solar rotating magnetoconvection. - Rekha Jain, reader, University of Sheffield, UK
Analytical models of travelling modes of solar rotating convection. - Shravan Hanasoge, professor, TIFR Mumbai, India
Mode-coupling helioseismology applied to the study of solar inertial modes. - Francois Lignières, directeur de recherche, IRAP, Observatoire Midi-Pyrénées, Toulouse, France
Dynamics of stellar interiors; convection, rotation, magnetic field, and pulsations. - Hideyuki Saio, emeritus professor, Tohoku University, Sendai, Japan
Models of stellar inertial and gravito-inertial modes, including stability. Interpretation of Kepler photometry of intermediate-mass stars. - Masao Takata, assistant professor, University of Tokyo, Japan
Models of stellar inertial and gravito-inertial modes. Seismic diagnostics based on gravito-inertial modes (including Rossby and pure inertial modes) in intermediate-mass stars.
Stellar members / Solar members