Orton, G.; Fletcher, L. N.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Encrenaz, T.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Cavalié, T.et al.; Moses, J.; Burgdorf, M.; Hammel, H.; Line, M.; Mainzer, A. K.; Hofstadter, M.; Sandell, G. H.; Dowell, C. D.; Pantin, E.; Fujiyoshi, T.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. American Astronomical Society, DPS meeting #46, Tucson, AZ, USA (2014)
Orton, G.; Fletcher, L.; Feuchtgruber, H.; Lellouch, E.; Moreno, R.; Hartogh, P.; Jarchow, C.; Swinyard, B.; Moses, J.; Burgdorf, M.et al.; Hammel, H.; Line, M.; Mainzer, A.; Hofstadter, M.; Sandell, G.; Dowell, C.: Models for Temperature and Composition in Uranus from Spitzer, Herschel and Ground-Based Infrared through Millimeter Observations. EGU General Assembly, Vienna, Austria (2014)
Rengel, M.; Moreno, R.; Courtin, R.; Lellouch, E.; Sagawa, H.; Hartogh, P.; Swinyard, B.; Lara, L.; Feuchtgruber, H.; Jarchow, C.et al.; Fulton, T.; Cernicharo, J.; Bockelée-Morvan, D.; Biver, N.; Banaszkiewicz, M.; González, A.: Tracing the gas composition of Titan's atmosphere with Herschel: Advances and Discoveries. 46th Annual Meeting of the Division for Planetary Sciences, Tucson, AZ, USA (2014)
Rezac, L.; Jarchow, C.; Hartogh, P.: Inversion simulations for the MIRO instrument on board of the Rosetta orbiter: characterizing the information content. 11th Annual Meeting, Asia Oceania Geosciences Society, Sapporo, Japan (2014)
Rezac, L.; de Val-Borro, M.; Hartogh, P.; Cavalié, T.; Jarchow, C.; Rengel, M.; Dobrijevic, M.: New Determination of the HCN Profile in the Stratosphere of Neptune from Millimeter-wave Spectroscopy. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
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.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)