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)
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 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.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...