Stenzel, O.: Alkali Metals in Cometary Particles what is the Chemical Context? 50th ESLAB Symposium: From Giotto to Rosetta, Leiden, Netherlands (2016)
Stenzel, O. J.; Paquette, J.; the Cosima Team: Boron and Oxygen in Cometary Particles. 79th Annual Meeting of the Meteoritical Society, Berlin, Germany (2016)
Stenzel, O. J.; Varmuza, K.; Engrand, C.; Ferriere, L.; Brandstätter, F.; Koeberl, C.; Filzmoser, P.; Paquette, J.; Hilchenbach, M.: Using Meteorite Samples as a Test for Correlation Based Analysis of SIMS Data from Cometary Grains. 46th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2015)
Stenzel, O. J.; Varmuza, K.; Engrand, C.; Ferrière, L.; Brandstätter, F.; Koeberl, C.; Filzmoser, P.; Paquette, J.; Hilchenbach, M.: Correlation Based analysis of SIMS Data from Meteorite Samples for Comparison with Cometary Grains. European Planetary Science Congress, Nantes, France (2015)
Paquette, J.; Engrand, C.; Stenzel, O.; Hilchenbach, M.: Measuring Oxygen Isotopes with COSIMA. American Geophysical Union Fall Meeting, San Francisco, USA (2014)
Paquette, J. A.; Stenzel, O.: The Effects of Sputtering Yields on the Rosetta/COSIMA Instrument Efficiency. Asteroids Comets Meteors 2014, Helsinki, Finland (2014)
Reiss, D.; Hoekzema, N. M.; Stenzel, O. J.: Dust Deflation by Dust Devils on Mars Derived from Optical Depth Measurements Using the Shadow Method in HiRISE Images. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
Stenzel, O. J.; Hoekzema, N. M.; Markiewicz, W. J.: Mars' Atmospheric Optical Depth from Mars Express HRSC and Mars Exploration Rovers A Comparison. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
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.