Hartogh, P.; Medvedev, A. S.; Jarchow, C.: Middle atmosphere polar warmings on Mars: Simulations and study on the validation with submillimeter observations. Planetary and Space Science 55, S. 1103 - 1112 (2007)
Kuroda, T.; Medvedev, A. S.; Hartogh, P.; Takahashi, M.: Seasonal changes of the baroclinic wave activity in the northern hemisphere of Mars simulated with a GCM. Geophysical Research Letters 34, L09203 (2007)
Kutepov, A. A.; Feofilov, A. G.; Medvedev, A. S.; Pauldrach, A. W. A.; Hartogh, P.: Small-scale temperature fluctuations associated with gravity waves cause additional radiative cooling of the mesopause region. Geophysical Research Letters 34, L24807 (2007)
Medvedev, A. S.; Hartogh, P.: Winter polar warmings and the meridional transport on Mars simulated with a general circulation model. Icarus 186, S. 97 - 110 (2007)
Sonnemann, G. R.; Hartogh, P.; Jarchow, C.; Grygalashvyly, M.; Berger, U.: On the winter anomaly of the night-to-day ratio of ozone in the middle to upper mesosphere in middle to high latitudes. Advances in Space Research 40, S. 846 - 854 (2007)
Graf, U.; Heyminck, S.; Güsten, R.; Hartogh, P.; Hübers, H.-W.; Jacobs, K.; Phillip, M.; Rabanus, D.; Röser, H.-P.; Stutzki, J.et al.; van der Wal, P.; Wagner-Gentner, A.: GREAT: the German first light heterodyne instrument for SOFIA. Proceedings of the SPIE 6275, 62750K (2006)
Sonnemann, G. R.; Grygalashvyly, M.; Hartogh, P.; Jarchow, C.: Behaviour of mesospheric ozone under nearly polar night conditions. Advances in Space Research 38, S. 2402 - 2406 (2006)
Villanueva, G.; Hartogh, P.: The high resolution chirp transform spectrometer for the SOFIA-GREAT instrument. Experimental Astronomy 18, S. 77 - 91 (2006)
Villanueva, G. L.; Hartogh, P.; Reindl, L.: A Digital Dispersive Matching Network for SAW Devices in Chirp Transform Spectrometers. IEEE Trans. Microw. Theory Tech. 54 (4), S. 1415 - 1424 (2006)
Hartogh, P.; Medvedev, A. S.; Kuroda, T.; Saito, R.; Villanueva, G.; Feofilov, A. G.; Kutepov, A. A.; Berger, U.: Description and climatology of a new general circulation model of the Martian atmosphere. Journal Geophysical Research 110, E11008 (2005)
Hartogh, P.; Jarchow, C.; Sonnemann, G. R.; Grygalashvyly, M.: On the spatiotemporal behaviour of ozone within the upper mesosphere/mesopause region under nearly polar night conditions. Journal Geophysical Research 109, D18303 (2004)
Villanueva, G.; Hartogh, P.: The high resolution chirp transform spectrometer for the SOFIA-GREAT instrument. Experimental Astronomy 18 (1-3), S. 77 - 91 (2004)
von Zahn, U.; Baumgarten, G.; Berger, U.; Fiedler, J.; Hartogh, P.: Noctilucent clouds and the mesospheric water vapour: the past decade. Atmos. Chem. Phys. 4, S. 2449 - 2464 (2004)
von Zahn, U.; Berger, U.; Fielder, J.; Hartogh, P.: Noctilucent clouds and the mesospheric water vapour: the past decade. Atmos. Chem. Phys. Discuss. 4, S. 3045 - 3076 (2004)
Stevens, M. H.; Gumbel, J.; Englert, C. R.; Grossmann, K. U.; Rapp, M.; Hartogh, P.: Polar mesospheric clouds formed from space shuttle exhaust. Geophysical Research Letters 30 (10), 1546 (2003)
Feist, D. G.; Aellig, C. P.; Kämpfer, N.; Solomon, P. M.; Barrett, J. W.; Zoonematkermani, S.; Hartogh, P.; Jarchow, C.; Waters, J. W.: Validation of stratospheric ClO measurements from the Millimeter-wave Atmospheric Sounder (MAS). Journal Geophysical Research 105 (D7), S. 9053 - 9062 (2000)
Seele, C.; Hartogh, P.: A case study on middle atmospheric water vapor transport during the February 1998 stratospheric warming. Geophysical Research Letters 27 (20), S. 3309 - 3312 (2000)
Hofstadter, M. D.; Hartogh, P.; McMullin, J. P.; Martin, E. N.; Jarchow, C.; Peters, W.: A search for variability in the HCN to H2CO Ratio on Comet Hale-Bopp. Earth, Moon and Planets 78, S. 53 - 61 (1999)
Erst eisige Kälte, dann Mitternachtssonne: Am Polarkreis bereitet das Team den Flug des ballongetragenen Sonnenobservatoriums vor – und hofft auf ein solares Feuerwerk.
Bewerbungsfrist 1 Oktober 2023. Promotionsprojekte in Planetenwissenschaften, Sonnenphysik, Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
In der mittleren Korona der Sonne entdeckt ein Forscherteam netzartige, dynamische Plasmastrukturen – und einen wichtigen Hinweis auf den Antrieb des Sonnenwindes.