Rengel, M.; Sagawa, H.; Hartogh, P.: Retrieval Simulations of Atmospheric Gases from Herschel Observations of Titan. Advances in Geosciences, pp. 335 - 348 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; de Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58, pp. 1692 - 1698 (2010)
Sagawa, H.; Hartogh, P.; Rengel, M.; Lange, A.; Cavalié, T.: Preparation for the solar system observations with Herschel: Simulation of Jupiter observations with PACS. Planetary and Space Science 58 (13), pp. 1692 - 1698 (2010)
Cavalié, T.; Billebaud, F.; Dobrijevic, M.; Fouchet, T.; Lellouch, E.; Encrenaz, T.; Brillet, J.; Moriarty-Schieven, G. H.; Wouterloot, J. G. A.; Hartogh, P.: First observation of CO at 345 GHz in the atmosphere of Saturn with the JCMT. New constraints on its origin. Icarus 203, pp. 531 - 540 (2009)
Grygalashvyly, M.; Sonnemann, G. R.; Hartogh, P.: Long-term behavior of the concentration of minor constituents in the mesosphere-a model study. Atmos. Chem. Phys. 9, pp. 2779 - 2792 (2009)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: Correction to Semiannual oscillations in the atmosphere of Mars. Geophysical Research Letters 36, L01202 (2009)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: On Forcing the Winter Polar Warmings in the Martian Middle Atmosphere during Dust storms. J. Meteorol. Soc. Japan 87, pp. 913 - 921 (2009)
Sonnemann, G. R.; Hartogh, P.: Upper stratospheric ozone decrease events due to a positive feedback between ozone and the ozone dissociation rate. Nonlinear Processes in Geophysics 16, pp. 409 - 418 (2009)
Sonnemann, G. R.; Hartogh, P.; Li, S.; Grygalashvyly, M.; Berger, U.: A QBO-signal in mesospheric water vapor measurements at ALOMAR (69.29 N, 16.03 E) and in model calculations by LIMA over a solar cycle. Atmos. Chem. Phys. Discuss. 9, pp. 883 - 903 (2009)
Yiğit, E.; Medvedev, A. S.; Aylward, A. D.; Hartogh, P.; Harris, M. J.: Modeling the effects of gravity wave momentum deposition on the general circulation above the turbopause. Journal Geophysical Research 114, D07101 (2009)
Bhardwaj, A.; Hartogh, P.; Kasaba, Y.; Wu, R. C. Y.: Advances in Planetary Sciences: AOGS 2007 (based on the Forth Annual Meeting of the AOGS, Bangkok, Thailand). Planetary and Space Science 56, p. 1675 (2008)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.