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)
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.