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)
Rengel, M.; Hartogh, P.; Jarchow, C.: HHSMT observations of the Venusian mesospheric temperature, winds, and CO abundance around the MESSENGER flyby. Planetary and Space Science 56, pp. 1688 - 1695 (2008)
Rengel, M.; Hartogh, P.; Jarchow, C.: Mesospheric vertical thermal structure and winds on Venus from HHSMT CO spectral-line observations. Planetary and Space Science 56, pp. 1368 - 1384 (2008)
Tachihara, K.; Rengel, M.; Nakajima, Y.; Yamaguchi, N.; André, P.; Neuhäuser, R.; Onishi, T.; Fukui, Y.; Mizuno, A.: Gas and Dust Condensations and a Peculiar Class 0 Object in the Lupus 3 Star-Forming Cloud. Astrophysical Journal 659, pp. 1382 - 1393 (2007)
Limaye, S.; Rengel, M.: 5 - Atmospheric circulation and dynamics - Observations and knowledge gaps. In: Towards understanding the climate of Venus: Applications of terrestrial models to our sister planet, pp. 55 - 72 (Eds. Bengtsson, L.; Bonnet, R.-M.; Grinspoon, D.; Koumoutsaris, S.; Lebonnois, S. et al.). Springer-Verlag, Berlin (2012)
Rengel, M.; Sagawa, H.; Hartogh, P.: Retrieval Simulations of Atmospheric Gases from Herschel observations of Titan. In: Advances in Geosciences, pp. 335 - 348 (Eds. Bhardwaj, A.; Haider, S. A.; Hartogh, P.; Ip, W.-H.; Ito, T. et al.). World Scientific Publishing Co., Singapore (2011)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.: Modeling of the Terminal Velocities of the Dust Ejected Material by the Impact. In: Deep Impact as a World Observatory Event - Synergies in Space, Time (Eds. Kaeufl, H. U.; Sterken, C.). Springer Verlag (2007)
Soderblom, D. R.; Nave, G. (Eds.): About the atomic and molecular databases in the planetary community - A contribution in the Laboratory Astrophysics Data WG IAU 2022 GA session. IAU Symposium, 2024. (2024), 87-91 pp.
de Val-Borro, M.; Hartogh, P.; Jarchow, C.; Rengel, M.; Villanueva, G. L.; Küppers, M.; Biver, M.; Bockelée-Morvan, D.; Crovisier, J.: The volatile composition of comet C/2004 Q2 (Machholz) derived from submillimeter observations. In: Highlights of Spanish Astrophysics VII, Proceedings of the X Scientific Meeting of the Spanish Astronomical Society (SEA) (Eds. Guirado, J. C.; Lara, L. M.; Quilis, V.; Gorgas, J.). (2013)
Küppers, M.; Keller, H. U.; Fornasier, S.; Gutierrez, P.; Hviid, S. F.; Jorda, L.; Knollenberg, J.; Lowry, S. C.; Rengel, M.: Observations of Comet 9P/Tempel 1 and Deep Impact by the OSIRIS Cameras onboard Rosetta. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 29 - 39. Springer Berlin / Heidelberg (2009)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.: Modeling of the Terminal Velocities of the Dust Ejected Material by the Impact. In: Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength, pp. 137 - 142. Springer Berlin / Heidelberg (2009)
Rengel, M.; Küppers, M.; Keller, H. U.; Gutierrez, P.; Hviid, S.: The terminal Velocity of the Deep Impact dust Ejecta. In: Revista Mexicana de Astronomía y Astrofísica (SC)., pp. 25 - 26 (Eds. Magris, G.; Bruzual, G.; Carigi, L.). (2009)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...