Pourabdian, M.; Gizon, L.; Hohage, T.; Fournier, D.; Hanson, C. S.: Comparison of full-waveform and travel-time inversions in helioseismology. 14th International Conference on Mathematical and Numerical Aspects of Wave Propagation (WAVES2019), Vienna, Austria (2019)
Gottschling, N.; Schunker, H.; Birch, A.; Gizon, L.: Evolution of Flows around Emerging Active Regions. Astronomical Institute at the Ruhr-University Bochum, Bochum, Germany (2019)
Gottschling, N.; Schunker, H.; Birch, A.; Gizon, L.: Evolution of Flows around Emerging Active Regions. 234th Meeting of the American Astronomical Society , St. Louis, Missouri, USA (2019)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: On the latitude dependence of Rossby waves in the Sun. 234th Meeting of the American Astronomical Society, St. Louis, USA (2019)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: Exploring the latitude and depth dependence of solar Rossby waves. 2nd Max Planck Partner Group Workshop on Solar Physics, Mumbai, India (2019)
Gizon, L.: Presentation of Director candidate. Meeting of the Chemistry, Physics and Technology Section of the Scientific Council of the Max Planck Society, Berlin, Germany (2019)
Gizon, L.: Presentation of the Department: Solar and Stellar Interiors. ESRP Meeting; Max Planck Institute for Solar System Research, Goettingen, Germany (2018)
Gizon, L.: Helioseismology as a probe of solar turbulent convection. Max-Planck/Princeton Center for Plasma Physics Workshop 2018, Princeton, NJ, USA (2018)
Gizon, L.: Equatorial Rossby Waves in the Solar Interior. Dynamic Sun II conference: Solar Magnetism from Interior to the Corona, Siem Reap, Angkor Wat, Cambodia (2018)
Gizon, L.: Rotating turbulent convection in the Sun. Discussion Meeting on Turbulence from Angstroms to Light Years. International Centre for Theoretical Sciences (ICTS) of the Tata Institute of Fundamental Research, Bangalore, India (2018)
Ferret, R. Z.; Gizon, L.; Birch, A.; Cameron, R.: New insights on the depth of an average supergranule through forward modeling in time-distance helioseismology. Rocks \& Stars II, Göttingen, Germany (2017)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.