Khomenko, E. V.; Collados, M.; Lagg, A.; Solanki, S. K.; Trujillo-Bueno, G.: Statistical properties of magnetic fields in intranetwork. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 445 - 448 (Ed. Sawaya-Lacoste, H.). ESA Publications Division, Noordwijk, The Netherlands (2002)
Mathew, S. K.; Lagg, A.; Solanki, S. K.; Collados, M.; Berdyugina, S.; Krupp, N.; Woch, J.; Frutiger, C.: Inversion of 1.5 μm spectral data of a sunspot. In: Proc. ``Probing the Sun with High Resolution'' (Eds. Venkatkrishnan, S.; Tripathy, S. C.; Venkatkrishnan, P. V.). Alpha Science, Pangbourne (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot from the inversion of IR spectral data. In: 1st Potsdam Thinkshop on Sunspots and Starspots Poster Proceedings, pp. 117 - 118 (Eds. Strassmeier, K. G.; Washuettl, A.). Brandenburgische Universitätsdruckerei, Golm (2002)
Mathew, S. K.; Solanki, S. K.; Lagg, A.; Collados, M.; Berdyugina, S.; Frutiger, C.; Krupp, N.; Woch, J.: Thermal-magnetic relation of a sunspot as inferred from inversion of 1.5 μm spectral data. In: SOLMAG 2002, Proceedings of the Magnetic Coupling of the Solar Atmosphere, Euroconference and IAU Colloquium 188,, pp. 501 - 504 (Ed. Sawaya-Lacoste, H.). ESA Publ. Div., Noordwijk (2002)
Krupp, N.; Lagg, A.; Livi, S.; Wilken, B.; Woch, J.; Williams, D. J.: The Energetic Particles Detector (EPD) Aboard the Galileo Spacecraft. In: The Three Galileos: The Man, the Spacecraft, the Telescope, pp. 319 - 330 (Eds. Barbieri; C.; others). Kluwer, Dordrecht (1997)
Lagg, A.: SUNRISE III: High-resolution exploration of the solar atmospheric stratification. Virtual Annual Meeting of the Astronomische Gesellschaft 2020 (2020)
Lagg, A.; Sunrise consortium: Sunrise -3: High-resolution exploration of the solar atmospheric stratification. 5th Asia Pacific Solar Physics Conference, Pune, India (2020)
Lagg, A.; Sunrise 3 Consortium: SUNRISE-3: a close-up view of the Sun from a stratospheric balloon. Annual Meeting of the German Astronomical Society: “Mission to the Universe: From Earth to Planets, Stars & Galaxies"
, Stuttgart, Germany (2019)
Löptien, B.; Lagg, A.; van Noort, M.; Solanki, S. K.: Relating the magnetic field strength with the umbra-penumbra boundary in sunspots. SolarPolarization Workshop 9, Göttingen, Germany (2019)
Lagg, A.; Sunrise 3 Consortium: Getting ready for the 3rd science flight of Sunrise. 24th ESA Symposium on European Rocket and Balloon Programmes and Related Research, Essen, Germany (2019)
Lagg, A.: Towards better Vector Magnetic Field Maps for Helicity Observations. Solar Helicities in Theory and Observations: Implications for Space Weather and Dynamo Theory, Stockholm, Schweden (2019)
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.