Kronberg, E. A.; Grigorenko, E. E.; Turner, D. L.; Reeves, G.; Daly, P. W.; Khotyaintsev, Y.: Comparing and contrasting dispersionless injections at geosynchronous orbit during a substorm event. 4th Cluster-THEMIS workshop, Palm Springs, USA (2016)
Li, K.; Haaland, S.; Daly, P. W.; Kronberg, E. A.; André, M.; Eriksson, A.; Lybekk, B.; Pedersen, A.: Observation of the cold ion stagnation in the ionospheric outflow. European Geosciences Union General Assembly, Vienna, Austria (2016)
Luo, H.; Kronberg, E. A.; Nykyri, K.; Trattner, K. J.; Daly, P. W.; Chen, G. X.; Du, A. M.: IMF dependence of energetic oxygen and hydrogen ion distributions in the near-Earth plasma sheet. 4th Cluster-THEMIS workshop, Palm Springs, USA (2016)
Vilenius, E.; Daly, P. W.; Kronberg, E. A.: Correcting the RAPID Imaging Electron Spectrometer data set for long-term sensitivity decrease. 4th Cluster-THEMIS workshop, Palm Springs, USA (2016)
Kronberg, E. A.; Luo, H.; Daly, P. W.; Grigorenko, E. E.; Klecker, B.: Dynamics of the energetic oxygen and hydrogen ions in the near-Earth plasma sheet. Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
Kronberg, E.; Mouikis, C.; Kistler, L.; Dandouras, I.; Daly, P. W.; Welling, D.; Grigorenko, E.: On contribution of energetic and heavy ions to the plasma pressure: Storm Sept 27 - Oct 4, 2002. AGU Fall Meeting, San Francisco, USA (2015)
Rashev, M.; Kronberg, E.; Daly, P. W.: On contamination of RAPID/IES data in the radiation belts. Cluster 15th and Double Star 10th anniversary workshop, Venice, Italy (2015)
Grigorenko, E. E.; Kronberg, E. A.; Daly, P. W.; Dolgonosov, M. S.: Ion acceleration in the vicinity of near-Earth X-line. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes, Greece (2014)
Rashev, M. V.; Kronberg, E. A.; Daly, P. W.: Geant4 modelling of RAPID/IES detector on Cluster. Geospace Revisited: a Cluster/MAARBLE/Van Allen Probes Conference, Rhodes, Greece (2014)
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.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.