Doerr, H.-P.; Iglesias, F.; Lagg, A.; van Noort, M.; The GRIS+ Tteam: GRIS+ - Instrument Setup and First Data. GREGOR technical development meeting, Potsdam, Germany (2017)
Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Olspert, N.; Brandenburg, A.; Warnecke, J.; Lagg, A.; Arlt, R.: Stellar convection models with Kramers-type opacity law. Session 'Fundamental aspects of turbulent convection,' of the DPG-FrÜhjahrstagung, Dresden, Germany (2017)
Käpylä, P. J.; Käpylä, M. J.; Rheinhardt, M.; Olspert, N.; Brandenburg, A.; Warnecke, J.; Lagg, A.; Arlt, R.: Implications of extended subadiabtic layers for stellar dynamos. 2nd Conference on Natural Dynamos, Valtice, Czech Republic (2017)
Lagg, A.: Measurements of Photospheric Magnetic Fields: Spectro-Polarimetry at High Spatial Resolution (invited review). SOLARNET IV: The Physics of the Sun from the Interior to the Outer Atmosphere, Lanzarote, Spain (2017)
Lagg, A.: Measuring quiet-Sun magnetic fields in the photosphere: Recent advances and future perspectives (invited talk). IAPSO - IAMAS -IAGA Joint Assembly, Capetown, South Africa (2017)
Siu-Tapia, A. L.; Lagg, A.; Solanki, S. K.; van Noort, M.; Rempel, M.: Photospheric counter-Evershed flows in the penumbra of sunspots. Solarnet IV Meeting "The physics of the Sun from the interior to the outer atmosphere", Lanzarote, Spain (2017)
Siu-Tapia, A. L.; Lagg, A.; Solanki, S. K.; van Noort, M.; Rempel, M.: Anomalous counter Evershed flows: HINODE observations and MHD simulations. IAU Symposium 327: Fine structure and dynamics of the solar atmosphere, Cartagena de Indias, Colombia (2016)
Lagg, A.: Chromospheric magnetic fields measurements. ISSI workshop on Solar Magnetic Fields: From Measurements towards Understanding, Bern, Switzerland (2015)
Lagg, A.; Gris-Team: Quiet-Sun Magnetism: A New Perspective from GRIS / GREGOR. Coimbra Solar Physics Meeting "Ground-based Solar Observations in the Space Instrumentation Era", Coimbra, Portugal (2015)
Lagg, A.: First Chromospheric (He I 1083 nm) and Photospheric (Fe I 1565 nm) Observations with GREGOR/GRIS. Indo-German Workshop on Solar Astronomy, Bangalore, India (2014)
Lagg, A.; Bernasconi, P.; Katsukawa, Y.; del Toro Iniesta, J.C.; Berkefeld, T.; Solanki, S. K.: SUNRISE III: The Solar Atmosphere in 3D and High Rssolution. 2021 Scientific Ballooning Technologies Workshop, online (2021)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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.
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.