Haaland, S.; Reistad, J.; Tenfjord, P.; Maes, L.; Anekallu, C.; Dorville, N.; DeKeyser, J.: The terrestrial magnetopause - an asymmetric boundary. European Geosciences Union General Assembly, Vienna, Austria (2015)
Li, K.; Haaland, S.; Daly, P. W.; Kronberg, E. A.; André, M.; Eriksson, A.; Lybekk, B.; Pedersen, A.: On the dayside high altitude stagnant region of cold ion outflow. Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
André, M.; Li, K.; Eriksson, A. I. E.; Nilsson, H.; Haaland, S.: Outflow of low-energy ions and the solar cycle. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes- Greece (2014)
Haaland, S.; Reistad, J.; Tenfjord, P.; Maes, L.; DeKeyser, J.; Anekallu, C.; Gjerloev, J.: Dawn-dusk asymmetries in the magnetopause and ring current. AGU Fall meeting, San Francisco, USA (2014)
Walsh, A. P.; Haaland, S.; Forsyth, C.; Keesee, A. M.; Kissinger, J.; Li, K.; Runov, A.; Soucek, J.; Walsh, B. M.; Wing, S.et al.; Taylor, M. G. G. T.: Dawn-dusk asymmetries in the coupled Solar wind-magnetosphere-ionosphere system. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes, Greece (2014)
Krcelic, P.; Haaland, S.; Maes, L.; Slapak, R.; Schillings, A.: Estimating the fate of oxygen ion outflow for a wide energy range. 29th Cluster workshop, Lanzarote, Canary Islands, Spain (2019)
Kronberg, E. A.; Ilie, R.; Smirnov, A.; Gastaldello, F.; Haaland, S.; Berrendorf, M.; Huang, Y.; Daly, P. W.; Ghizzardi, S.; Allen, R. C.: Prediction of soft protons in the near-Earth space using machine learning. Machine Learning in Heliophysics, Amsterdam, Netherlands (2019)
Li, K.; Wei, Y.; Haaland, S.; Kronberg, E. A.; Rong, Z.; Maes, L.; Maggiolo, R.; Andre, M.; Nilsson, H.; Grigorenko, E.: Estimating the Kinetic Energy Budget of the Polar Wind Outflow. EGU General Assembly, Vienna, Austria (2019)
Förster, M.; Rashev, M.; Haaland, S.: Millisecond resolution electron fluxes from the Cluster satellites: Calibrated EDI ambient electron data. European Geosciences Union General Assembly 2017, Vienna, Austria (2017)
Haaland, S.; Baddeley, L.; Bjoland, L.; Gustavsson, B.: Ion outflow at equinox conditions: North-south asymmetries. European Geosciences Union General Assembly, Vienna, Austria (2017)
Haaland, S.; Narita, Y.; Eriksson, E.; Vaivads, A.: Tools for THOR: Structure analysis. European Geosciences Union General Assembly, Vienna, Austria (2017)
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.
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".