Langfellner, J.; Gizon, L.; Birch, A. C.: Evolution of solar intermediate-scale convection. Seismology of the Sun and Distant Stars (HELAS8/SPACEINN/TASC2/KASC9), Angra do Heroismo, Portugal (2016)
Leguebe, M.; Hanson, C. S.; Fournier, D.; Brich, A. C.; Gizon, L.: Accurate numerical solutions to the forward problem of local helioseismology. Seismology of the Sun and the Distant Stars 2016, Angra do Heroísmo, Portugal (2016)
Liang, Z.-C.; Duvall{} Jr., T. L.; Gizon, L.: Solar Cycle Dependence of the Deep Meridional flow. Joint TASC2 \& KASC9 Workshop -- SPACEINN \& HELAS8 Conference, Angra do Heroísmo, Portugal (2016)
Löptien, B.; Birch, A. C.; Duvall{} Jr., T. L.; Gizon, L.; Schou, J.: Measuring active region inflows with local correlation tracking. Solar and Stellar Magnetic Fields - a conference in honor of Manfred Schuessler, Goslar, Germany (2016)
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)
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.
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 magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.