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 dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.