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)
Franco, A. M. S.; Fränz, M.; Echer, E.; Bolzan, M. J. A.: A Statistical Study of ULF Wave Scales Around Mars Using MEX and MAVEN Observations. 50th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2019)
Huybrighs, H.; Roussos, E.; Krupp, N.; Fränz, M.; Futaana, Y.; Barabash, S.; Glassmeier, K.-H.: The search for Europa plume signatures in Galileo plasma particle data. Magnetospheres of the Outer planets conference (MOP), Uppsala, Sweden (2017)
Krupp, N.; Fränz, M.; Roussos, E.; Huybrighs, H.; Barabash, S.; Brandt, P. C.; Paranicas, C.; Mitchell, D. G.; Westlake, J.; Khurana, K.et al.; Jia, X.: Electron measurements in the low-latitude magnetosphere of Jupiter and in the vicinity of the Galilean moons: Current knowledge and future investigations with the PEP JEI and JoEE sensors onboard the JUICE spacecraft. Magnetospheres of the Outer planets conference (MOP), Uppsala, Sweden (2017)
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)
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)
Fraenz, M.; Dubinin, E.; Andrews, D.; Nilsson, H.; Fedorov, A.: Cold ion escape from the Martian ionosphere. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Han, X.; Fraenz, M.; Andrews, D.; Dubinin, E.; Wan, W.; Barabash, S.: The control of Martian ionopause altitude by the crustal and induced magnetic field strength. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Fränz, M.: Ionen mittlerer Energie in der Heliosphäre: Ergebnisse des Ulysses-EPAC-Experiments in der Ekliptik. 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.