Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Galactic Cosmic Rays access to the upper atmosphere and rings of Saturn. AGU Fall Meeting, San Francisco, USA (2016)
Regoli, L. H.; Roussos, E.; Luhmann, J.; Dialynas, K.; Krupp, N.; Jones, G. H.; Coates, A. J.: Energetic environment at Titan's orbit. AGU Fall Meeting, San Francisco, USA (2016)
Lee-Payne, Z.; Grande, M.; Krupp, N.; Paranicas, C.; Roussos, E.; Kollmann, P.: Re-evaluating Galileo Energetic Particle Detector data based on radiation detector decay; for use in estimating Sputtering Erosion rates on Europa. European Planetary Science Congress EPSC , Nantes, France (2015)
Palmaerts, B.; Roussos, E.; Krupp, N.; Kurth, W. S.; Mitchell, D. G.; Dougherty, M. K.: Statistical analysis and multi-instrument overview of the quasi-periodic 1-hour pulsations in Saturn's outer magnetosphere. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Coates, A.; Thomsen, M.; Feyerabend, M.; Jones, G.; Roussos, E.; Krupp, N.: Pickup Ion Signatures in the Vicinity of Titan. AGU Fall Meeting, San Francisco, USA (2015)
Roussos, E.; Krupp, N.; Fraenz, M.; Kollmann, P.; Truscott, P.; Futaana, Y.: Hot Plasma Environment Model (HPEM): A empirical model for describing time-dependent processes of the jovian energetic electron environment. European Planetary Science Congress EPSC , Nantes, France (2015)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Tracing of energetic particles in the vicinity of Titan. European Geosciences Union General Assembly, Vienna, Austria (2014)
Regoli, L.; Feyerabend, M.; Kotova, A.; Roussos, E.; Jones, G.; Krupp, N.; Coates, A.: Mapping the flow of energetic particles in Titan's exobase. 10 years of Cassini-Huygens in the Saturnian system, London, UK (2014)
Krupp, N.: Drei-dimensionale Richtungsverteilungen und relative Häufigkeiten energiereicher Ionen in der Magnetosphäre des Jupiter. Dissertation, Technische Universität Braunschweig (1994)
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.