Blanc, M.; Andrews, D. J.; Coates, A. J.; Hamilton, D. C.; Jackman, C. M.; Jia, X.; Kotova, A.; Morooka, M.; Smith, H. T.; Westlake, J. H.: Saturn Plasma Sources and Associated Transport Processes. Space Science Reviews 192, pp. 237 - 283 (2015)
Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Modeling of the energetic ion observations in the vicinity of Rhea and Dione. Icarus 258, pp. 402 - 417 (2015)
Beth, A.; Garnier, P.; Toublanc, D.; Dandouras, I.; Mazelle, C.; Kotova, A.: Modeling the satellite particle population in the planetary exospheres: Application to Earth, Titan and Mars. Icarus 227, pp. 21 - 36 (2014)
Krupp, N.; Roussos, E.; Kriegel, H.; Kollmann, P.; Kivelson, M. G.; Kotova, A.; Paranicas, C.; Mitchell, D. G.; Krimigis, S. M.; Khurana, K. K.: Energetic particle measurements in the vicinity of Dione during the three Cassini encounters 2005-2011. Icarus 226, pp. 617 - 628 (2013)
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)
Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Galactic Cosmic Rays in the inner magnetosphere of Saturn. European Geosciences Union General Assembly, Vienna, Austria (2015)
Kotova, A.; Roussos, E.; Krupp, N.; Dandouras, I.: Galactic Cosmic Rays tracing in the inner magnetosphere of Saturn. MIMI Team Meeting, Atlanta, Georgia, USA (2015)
Krupp, N.; Roussos, E.; Kotova, A.; Khurana, K. K.; Jones, G. H.; Simon, S.: Enceladus flybys in the view of energetic particles. European Planetary Science Congress EPSC , Nantes, France (2015)
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)
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.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.