Graf, U. U.; Simon, R.; Stutzki, J.; Colgan, S. W. J.; Guan, X.; Güsten, R.; Hartogh, P.; Honingh, C. E.; Hübers, H.-W.: [12Cii] and [13C ii] 158 μ m emission from NGC 2024: Large column densities of ionized carbon. Astronomy and Astrophysics 542, L16 (2012)
Gulkis, S.; Keihm, S.; Kamp, L.; Lee, S.; Hartogh, P.; Crovisier, J.; Lellouch, E.; Encrenaz, P.; Bockelée-Morvan, D.; Hofstadter, M.et al.; Beaudin, G.; Janssen, M.; Weissman, P.; von Allmen, P. A.; Encrenaz, T.; Backus, C. R.; Ip, W.-H.; Schloerb, P. F.; Biver, N.; Spilker, T.; Mann, I.: Continuum and spectroscopic observations of asteroid (21) Lutetia at millimeter and submillimeter wavelengths with the MIRO instrument on the Rosetta spacecraft. Planetary and Space Science 66, pp. 31 - 42 (2012)
Hallgren, K.; Hartogh, P.: First detection of tidal behaviour in polar mesospheric water vapour by ground based microwave spectroscopy. Atmos. Chem. Phys. 12, pp. 3753 - 3759 (2012)
Mommert, M.; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E.; Müller, T. G.; Peixinho, N.et al.; Lellouch, E.; Szalai, N.; Henry, F.; Duffard, R.; Fornasier, S.; Hartogh, P.; Mueller, M.; Ortiz, J. L.; Protopapa, S.; Rengel, M.; Thirouin, A.: TNOs are Cool: A survey of the trans-Neptunian region V. Physical characterization of 18 Plutinos using Herschel PACS observations. Astronomy and Astrophysics 541, A93 (2012)
Moreno, R.; Lellouch, E.; Lara, L.; Feuchtgruber, H.; Rengel, M.; Hartogh, P.; Courtin, R.: The abundance, vertical distribution and origin of H2O in Titan's atmosphere: Herschel observations and photochemical modelling. Icarus 221, pp. 753 - 767 (2012)
Okada, Y.; Güsten, R.; Requena-Torres, M. A.; Röllig, M.; Hartogh, P.; Hübers, H.-W.; Klein, T.; Ricken, O.; Simon, R.; Stutzki, J.: Dynamics and photodissociation region properties in IC 1396A. Astronomy and Astrophysics 542, L10 (2012)
Simon, R.; Schneider, N.; Stutzki, J.; Güsten, R.; Graf, U. U.; Hartogh, P.; Guan, X.; Staguhn, J. G.; Bendord, D. J.: SOFIA observations of S106: dynamics of the warm gas. Astronomy and Astrophysics 542, L12 (2012)
Sonnemann, G. R.; Hartogh, P.; Berger, U.; Lübken, F.-J.; Grygalashvyly, M.: Anthropogenic effects on the distribution of minor chemical constituents in the mesosphere/lower thermosphere - A model study. Advances in Space Research 50 (5), pp. 598 - 618 (2012)
Stevens, M. H.; Lossow, S.; Fiedler, J.; Baumgarten, G.; Lübken, F.-J.; Hallgren, K.; Hartogh, P.; Randall, C. E.; Lumpe, J.; Bailey, S. M.et al.; Niciejewski, R.; Meier, R. R.; Plane, J. M. C.; Kochenash, A. J.; Murtagh, D. P.; Englert, C. R.: Bright polar mesospheric clouds formed by main engine exhaust from the space shuttles final launch. Journal Geophysical Research 117, D19206 (2012)
Yiğit, E.; Medvedev, A. S.; Aylward, A. D.; Ridley, A. J.; Harris, M. J.; Moldwin, M. B.; Hartogh, P.: Dynamical effects of internal gravity waves in the equinoctial thermosphere. Journal of Atmospheric and Solar-Terrestrial Physics 90-91, pp. 104 - 116 (2012)
Courtin, R.; Swinyard, B. M.; Moreno, R.; Fulton, T.; Lellouch, E.; Rengel, M.; Hartogh, P.: First results of Herschel-SPIRE observations of Titan. Astronomy and Astrophysics 536, L2 (2011)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".