Rengel, M.; Teyssier, D.; Mueller, M.; Jellema, W.; Moreno, R.; Avruch, I.: Solar System Objects as Prime Calibrators for Herschel/HIFI. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
Limaye, S.; Bougher, S.; Clancy, R.; Grassi, D.; Imamura, T.; Kohler, E.; Krause, P.; Lebonnois, S.; Mahieux, A.; Migliorini, A.et al.; Montmessin, F.; Pätzold, M.; Piccialli, A.; Rengel, M.; Rodin, A.; Sandor, B.; Sorning, M.; Tellmann, S.; Widemann, T.; Müller-Wodarg, I.; Zasova, L.: Towards a Self Consistent Model of the Thermal Structure of the Venus Atmosphere. European Planetary Science Congress EPSC, Cascais, Portugal (2014)
Rengel, M.; Sagawa, H.; Hartogh, P.: Venusian Mesospheric thermal structure and winds from May 2009 SMT CO spectral- line observations. 40th COSPAR Scientific Assembly, Moscow, Russia (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)
Teyssier, D.; Avruch, I.; Beaulieu, S.; Braine, J.; Marston, A.; Morris, P.; Olberg, M.; Rengel, M.; Shipman, R.: Herschel Explanatory Supplement Volume II - The Heterodyne Instrument for Far Infrared (HIFI) Handbook. Herschel Science Centre, ESA (2017)
Teyssier, D.; Rengel, M.: The Herschel/Heterodyne Instrument for the Far-Infrared (HIFI) Reference Position Spectra Data Products: Release notes. Herschel Science Centre, ESA (2016)
Avruch, I.; Beaulieu, S.; Boogert, A.; Marston, T.; McCoey, C.; Olberg, M.; Rengel, M.; Shipman, R.: The Heterodyne Instrument for the Far Infrared (HIFI) Observers' Manual. HIFI Instrument Control Center (2011)
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, ...