Andriopoulou, M.; Roussos, E.; Krupp, N.; Paranicas, C.; Thomsen, M.; Krimigis, S.; Dougherty, M.; Glassmeier, K.-H.: Spatial and temporal dependence of the convective electric field in Saturn's inner magnetosphere. Icarus 229, pp. 57 - 70 (2014)
Roussos, E.; Andriopoulou, M.; Krupp, N.; Kotova, A.; Paranicas, C.; Krimigis, S. M.; Mitchell, D. G.: Numerical simulation of energetic electron microsignature drifts at Saturn: Methods and applications. Icarus 226 (2), pp. 1595 - 1611 (2013)
Andriopoulou, M.; Roussos, E.; Krupp, N.; Paranicas, C.; Thomsen, M.; Krimigis, S.; Dougherty, M. K.; Glassmeier, K. -.: A noon-to-midnight electric field and nightside dynamics in Saturns inner magnetosphere, using microsignature observations. Icarus 220, pp. 503 - 513 (2012)
Thomsen, M. F.; Roussos, E.; Andriopoulou, M.; Kollmann, P.; Arridge, C. S.; Paranicas, C. P.; Gurnett, D. A.; Powell, R. L.; Tokar, R. L.; Young, T. D.: Saturn's inner magnetospheric convection pattern: Further evidence. Journal Geophysical Research 117, A09208 (2012)
Roussos, E.; Krupp, N.; Mitchell, D. G.; Paranicas, C.; Palmaerts, B.; Paranicas, C.; Krimigis, S. M.; Andriopoulou, M.; Kurth, W. S.; Badman, S.et al.; Masters, A.; Dougherty, M. K.: Quasi-Periodic injections of relativistic electrons in Saturn's magnetosphere. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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.
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.