Haaland, S.: Atmospheric Erosion: Hemispheric Asymmetries in ion outflow. Fundamental Physical Processes in Solar-Terrestrial Research and Their Relevance to Planetary Physics 2018, Kona, Hawaii (2018)
Haaland, S.; Kronberg, E. A.; Daly, P. W.; Vilenius, E.: Energetic Particles in Geospace: Characteristics, Sources and Impact Seminar. Istituto di Astrofisica Spaziale e Fisica Cosmica, Milano, Italy (2018)
Haaland, S.: Planetary atmospheric erosion: the role of ion outflow. Fundamental Physical Processes in Solar-Terrestrial Research and Their Relevance to Planetary Physics 2018, Kona, Hawaii (2018)
Haaland, S.; Laundal, K.; Maes, L.; Baddeley, L.; Lybekk, B.: North-south asymmetries in cold ion outflow and lobe density: Cluster observations. European Geosciences Union General Assembly, Vienna, Austria (2016)
Haaland, S.; Baddeley, L.; Maes, L.: Using EISCAT vertical velocities to assess mechanisms for ion outflow. EISCAT and 42AM meeting, hermanus, South Africa (2015)
Haaland, S.; Baddeley, L.; Maes, L.: Using EISCAT vertical velocities to assess mechanisms for ion outflow. EISCAT Symposium and 42AM, Hermanus, South Africa (2015)
Haaland, S.; Foerster, M.; Laundal, K.; McKracken, K.; Maes, L.; Lybekk, B.; Pedersen, A.: North-south asymmetries in magnetospheric and ionospheric plasma circulation (Invited). AGU Fall Meeting, San Francisco, USA (2015)
Haaland, S.; Hasegawa, H.; Dunlop, M.; Fear, R.; Walsh, B.; DeKeyser, J.; Sonnerup, B.; Paschmann, G.: What did we learn from Cluster observations at the magnetopause? Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
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.
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.