Pfeifer, M.; Agarwal, J.; Marschall, R.; Grieger, B.; Lemos, P.: Dynamics and potential origins of decimeter-sized particles around comet 67P/Churyumov-Gerasimenko. Astronomy and Astrophysics 685, p. A136 (2024)
Pfeifer, M.; Agarwal, J.; Schröter, M.: On the trail of a comet's tail: A particle tracking algorithm for comet 67P/Churyumov-Gerasimenko. Astronomy and Astrophysics 659, p. A171 (2022)
Pfeifer, M.: Dust Particle Tracking at Comet 67P/Churyumov-Gerasimenko: General Idea & Current Approach. Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany (2019)
Pfeifer, M.: Dust Particle Tracking at Comet 67P/Churyumov-Gerasimenko: General Idea & Current Approach. Rosetta SWT Meeting , Noordwijk, Netherlands (2019)
Pfeifer, M.: Dust Particle Tracking at Comet 67P/Churyumov-Gerasimenko: General Idea & Current Approach. EPSC-DPS Joint Meeting 2019, Geneva, Switzerland (2019)
Analyzing the high spatial resolution solar Ca II H and K emission data obtained by the SUNRISE mission and building a model of other stars more active than the Sun
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.
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.