Fournier, D.; Hohage, T.; Gizon, L.: Parameter identification for the acoustic wave equation in helioseismology. The 12th International Conference on Mathematical and Numerical Aspects of Wave Propagation , Karlsruhe, Germany (2015)
Gizon, L.: Perspectives in Helioseismology. NASA LWS Workshop on Solar Dynamo Frontiers: Helioseismology, 3D Modeling, and Data Assimilation, National Center for Atmospheric Research, Boulder, Colorado, USA (2015)
Gizon, L.: Oblateness of a slowly rotating star from asteroseismology. Kick-off Workshop on "Advances in Seismology: a Dialogue Across Disciplines", Mumbai, India (2015)
Gizon, L.: Introduction to the partner group program. Kick-off Workshop on "Advances in Seismology: a Dialogue Across Disciplines", Mumbai, India (2015)
Gizon, L.; Barucq, H.; Durufle, M.; Birch, A. C.; Chabassier, J.; Fournier, D.; Hanson, C.; Leguèbe, M.: Solving the forward problem of helioseismology in the frequency domain. The 12th International Conference on Mathematical and Numerical Aspects of Wave Propagation, Karlsruhe, Germany (2015)
Langfellner, J.; Gizon, L.; Birch, A. C.: Solar turbulent convection at supergranulation scale. Stellar and Planetary Dynamos, Göttingen, Germany (2015)
Langfellner, J.; Gizon, L.; Birch, A. C.: Anisotropy of the solar network magnetic field around the average supergranule. Solarnet III / HELAS VII / SpaceInn Conference, Freiburg, Germany (2015)
Löptien, B.; Birch, A. C.; Duvall Jr., T. L.; Gizon, L.; Schou, J.: Data compression for helioseismology. SOLARNET III / HELAS VII / SpaceInn Conference "The Sun, the stars, and solar-stellar relations", Freiburg, Germany (2015)
Nagashima, K.; Gizon, L.; Birch, A. C.; Fournier, D.: Measuring and interpreting the amplitude of the cross-covariance function of solar seismic waves. Astronomical Society of Japan spring meeting, Osaka, Japan (2015)
Nagashima, K.; Gizon, L.; Birch, A. C.; Fournier, D.: Measurement of the amplitude of the solar cross-covariance function. Solarnet III / HELAS VII / SpaceInn Conference, Freiburg, Germany (2015)
Gizon, L.: Helioseismology in a Stellar Context: From SDO to PLATO. 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Flagstaff, USA (2014)
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
The MPS is one of the leading institutes worldwide in building instruments for solar research, both for ground based observatories as well as for balloon and space-borne missions. Scientists and engineers of MPS conceive new observing methods and develop novel instruments of highest technological complexity. These instruments are built in house, tested, calibrated, and used at the best solar observatories in the world, or delivered to NASA and ESA to be launched to space.