Förster, M.; Haaland, S.; Dorboos, E.: Thermospheric vorticity at high geomagnetic latitudes from CHAMP data and its IMF dependence. Annales Geophysicae 29, pp. 181 - 186 (2011)
Kronberg, E. A.; Bučík, R.; Haaland, S.; Klecker, B.; Keika, K.; Desai, M. I.; Daly, P. W.; Yamauchi, M.; Gómez-Herrero, R.; Lui, A. T. Y.: On the origin of the energetic ion events measured upstream the Earth's bow shock by STEREO, Cluster and Geotail. Journal Geophysical Research 116, A02210 (2011)
Østgaard, N.; Laundal, K. M.; Juusola, L.; Åsnes, A.; Haaland, S. E.; Weygand, J. M.: Interhemispherical asymmetry of substorm onset locations and the interplanetary magnetic field. Geophysical Research Letters 38, L08104 (2011)
Teh, W.-L.; Sonnerup, B. U. Ö.; Paschmann, G.; Haaland, S. E.: Local structure of directional discontinuities in the solar wind. Journal Geophysical Research 116, A04105 (2011)
Vaivads, A.; Andersson, G.; Bale, S. D.; Cully, C. M.; Keyser, J. D.; Fujimoto, M.; Grahn, S.; Haaland, S.; Ji, H.; Khotyaintsev, Y. V.et al.; Lazarian, A.; Lavraud, B.; Mann, I. R.; Nakamura, R.; Nakamura, T. K. M.; Narita, Y.; Retinò, A.; Sahraoui, F.; Schekochihin, A.; Schwartz, S. J.; Shinohara, I.; Sorriso-Valvo, L.: EIDOSCOPE: particle acceleration at plasma boundaries. Experimental Astronomy Astrophysical Instrumentation and Methods 33, pp. 491 - 527 (2011)
Blagau, A.; Klecker, B.; Paschmann, G.; Haaland, S.; Marghitu, O.; Scholer, M.: A new technique for determining orientation and motion of a 2-D, non-planar magnetopause. Annales Geophysicae 28, pp. 753 - 778 (2010)
Haaland, S.; Kronberg, E. A.; Daly, P. W.; Fränz, M.; Degener, L.; Georgescu, E.; Dandouras, I.: Spectral characteristics of protons in the Earth's plasmasheet: statistical results from Cluster RAPID and CIS. Annales Geophysicae 28, pp. 1483 - 1498 (2010)
Haaland, S.; Munteanu, C.; Mailyan, B.: Solar wind propagation delay: Comment on ``Minimum variance analysis-based propagation of the solar wind observations: Application to real-time global magnetohydrodynamic simulations''. Space Weather 8, S06005 (2010)
Förster, M.; Feldstein, Y. I.; Haaland, S. E.; Dremukhina, L. A.; Gromova, L. I.; Levitin, A. E.: Magnetospheric convection from Cluster EDI measurements compared with the ground-based ionospheric convection model IZMEM,. Annales Geophysicae 27, pp. 3077 - 3087 (2009)
Haaland, S.; Lybekk, B.; Svenes, K.; Pedersen, A.; Förster, M.; Vaith, H.; Torbert, R.: Plasma transport in the magnetotail lobes. Annales Geophysicae 27, pp. 3577 - 3590 (2009)
Lindstedt, T.; Khotyaintsev, Y. V.; Vaivads, A.; André, M.; Fear, R. C.; Lavraud, B.; Haaland, S.; Owen, C. J.: Separatrix regions of magnetic reconnection at the magnetopause. Annales Geophysicae 27, pp. 4039 - 4056 (2009)
Østgaard, N.; Snekvik, K.; Borg, A. L.; Åsnes, A.; Pedersen, A.; Øieroset, M.; Phan, T.; Haaland, S. E.: Can magnetotail reconnection produce the auroral intensities observed in the conjugate ionosphere? Journal Geophysical Research 114, A06204 (2009)
Förster, M.; Haaland, S.; Paschmann, G.; Quinn, J. M.; Torbert, R. B.; Vaith, H.; Kletzing, C. A.: High-latitude plasma convection during Northward IMF as derived from in-situ magnetospheric Cluster EDI measurements. Annales Geophysicae 26, pp. 2685 - 2700 (2008)
Mailyan, B.; Munteanu, C.; Haaland, S.: What is the best method to calculate the solar wind propagation delay? Annales Geophysicae 26, pp. 2383 - 2394 (2008)
Snekvik, K.; Nakamura, R.; Östgaard, N.; Haaland, S.; Retinó, A.: The Hall current system revealed as a statistical significant pattern during fast flows. Annales Geophysicae 26, pp. 3429 - 3437 (2008)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).