Dubinin, E.; Fraenz, M.; Modolo, R.: Magnetic fields and currents at Mars and Venus. AGU Chapman Conference "Currents in Geospace and Beyond", Dubrovnik, Croatia (2016)
Dubinin, E.; Fraenz, M.; Paetzold, M.; McFadden, J.; Eparvier, F.; Brain, D.; Jakosky, B.; Andrews, D.; Barabash, S.: Effects of solar irradiance on the upper ionosphere and ion fluxes at Mars, Mars Express and MAVEN observations. 8th MUAN meeting, Leicester, UK (2016)
Fränz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Barabash, S.; Fedorov, A.: Cold Ion Escape from the Martian Ionosphere. European Planetary Science Congress, Nantes, France (2015)
Barabash, S.; Holmsrtom, M.; Futaana, Y.; Fedorov, A.; Frahm, R.; Fraenz, M.; Dubinin, E.: Phobos-solar wind interaction: Results from Mars Express for the closest-ever fly-by. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Dubinin, E.; Fraenz, M.; Mazelle, C.; Barabash, S.: Large-amplitude coherent structures in plasma near Mars. The 5th Moscow Solar System Symposium (5M-S3), Moscow, Russia (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields and currents at Venus and Mars. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.: Ionospheric magnetic fields at Venus and Mars and their effect on plasma flow in the near planet wakes. EPSC, Estoril, Portugal (2014)
Dubinin, E.; Fraenz, M.; Zhang, T.-L.; Woch, J.; Wei, Y.; Barabash, S.: Asymmetrical response of the ionospheric magnetization and the plasma sheet formation on the IMF orientation. 6th Alfven Conference: Plasma Interactions with Solar System Objects anticipating Rosetta, MAVEN and Mars Orbiter Mission, London, UK (2014)
Wei, Y.; Fränz, M.; Dubinin, E.; Wan, W.; Jarvinen, R.; Zhang, T.-L.; Barabash, S.; Lundin, R.: Ablation of Venusian oxygen ions by unshocked solar wind. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Fan, K.; Wei, Y.; Fränz, M.; Dubinin, E. M.; Mcfadden, J.: Efficiency of Solar wind electric field in accelerating planetary ions. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
Fränz, M.; Dubinin, E. M.; Fan, K.; Maes, L.; Halekas, J.; McFadden, J.; Connerney, J.: Mars in the Solar Wind - Simulations and Observations. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
Fränz, M.; Dubinin, E. M.; Fan, K.; Maes, L.; Halekas, J.; McFadden, J.: Mars in the Solar Wind. 21st EGU General Assembly, EGU2019, Vienna, Austria (2019)
Chai, L.; Wei, Y.; Wan, W.; Zhang, T.; Fraenz, M.; Dubinin, E.; Zhang, H.; Rong, Z.; Barabash, S.: An induced global magnetic field looping around the magnetotail of Venus. European Geosciences Union General Assembly, Vienna, Austria (2016)
Han, Q.; Wei, Y.; Chai, L.; Rong, Z.; Fraenz, M.; Dubinin, E.; Wan, W.; Rong, Z.; Futaana, Y.: EUV0dependence of Venusian ionopause height over the dayside high-latitude region: VEX and PVO observations. European Geosciences Union General Assembly, Vienna, Austria (2016)
Dubinin, E.; Fraenz, M.; Andrews, D.; Witasse, O.; Barabash, S.: Ionosphere of Mars as seen by Mars Express. Effect of crustal fields. European Planetary Science Congress, Nantes, France (2015)
Fränz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Barabash, S.; Fedorov, A.: Cold Ion Escape from the Martian Ionosphere - 2007-2014. European Geosciences Union General Assembly, Vienna, Austria (2015)
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.