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)
Heller, R.; Duda, J.-P.; Winkler, M.; Reitner, J.; Gizon, L.: Habitability of the Early Earth: A Faint Young Sun and Strong Tidal Heating due to a Closer Moon. ESRP Meeting, Jena, Germany (2022)
Gizon, L.; MPS Team: Global-scale Rossby waves in the solar interior. Dynamics of the Sun and Stars: Honoring the Life and Work of Michael J. Thompson,, Boulder, USA (2019)
Nagashima, K.; Birch, A.; Schou, J.; Hindman, B.; Gizon, L.: Monte-Carlo test of an improved multi-ridge fitting code for ring-diagram analysis. Dynamics of the Sun & Stars: Honoring the Life & Work of Michael Thompson , Boulder, CO, USA (2019)
Yang, D.; Gizon, L.; Fournier, D.; Lindsey, C.: Improved helioseismic imaging of the farside. Dynamics of the Sun and Stars: Honoring the Life and Work of Michael J. Thompson,, Boulder, USA (2019)
Pourabdian, M.; Gizon, L.; Hohage, T.; Fournier, D.; Hanson, C. S.: Optimal averaging for helioseismic measurements using the singular value decomposition. XXXth General Assembly of the International Astronomical Union, Vienna, Austria (2019)
Poulier, P.-L.; Gizon, L.; Fournier, D.; Duvall, T.: On the validity of the frozen-in approximation for acoustic wave propagation through solar granulation. XXXth General Assembly of the International Astronomical Union, Vienna, Austria (2019)
Proxauf, B.; Gizon, L.; Löptien, B.; Birch, A.; Schou, J.; Bogart, R. S.: On the depth dependence of solar equatorial Rossby waves. Solar Dynamics Observatory Workshop Catalyzing Solar Connections, Ghent, Belgium (2018)
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.