Sizemore, H. G.; Platz, T.; Schorghofer, N.; Prettyman, T. H.; De Sanctis, M. C.; Crown, D. A.; Schmedemann, N.; Neesemann, A.; Kneissl, T.; Marchi, S.et al.; Schenk, P. M.; Bland, M. T.; Schmidt, B. E.; Hughson, K. H. G.; Tosi, F.; Zambon, F.; Mest, S. C.; Yingst, R. A.; Williams, D. A.; Russell, C. T.; Raymond, C. A.: Pitted terrains on (1) Ceres and implications for shallow subsurface volatile distribution. Geophysical Research Letters 44 (13), pp. 6570 - 6578 (2017)
Adeli, S.; Hauber, E.; Kleinhans, M.; Le Deit, L.; Platz, T.; Fawdon, P.; Jaumann, R.: Amazonian-aged fluvial system and associated ice-related features in Terra Cimmeria, Mars. Icarus 277, pp. 286 - 299 (2016)
Buczkowski, D. L.; Schmidt, B. E.; Williams, D. A.; Mest, S. C.; Scully, J. E. C.; Ermakov, A. I.; Preusker, F.; Schenk, P.; Otto, K. A.; Hiesinger, H.et al.; O'Brien D.and Marchi, S.; Sizemore, H.; Hughson, K.; Chilton, H.; Bland, M.; Byrne, S.; Schorghofer, N.; Platz, T.; Jaumann, R.; Roatsch, T.; Sykes, M. V.; Nathues, A.; De Sanctis, M. C.; Raymond, C. A.; Russell, C. T.: The geomorphology of Ceres. Science 353, aaf4332 (2016)
Hiesinger, H.; Marchi, S.; Schmedemann, N.; Schenk, P.; Pasckert, J. H.; Neesemann, A.; O'Brien, D. P.; Kneissl, T.; Ermakov, A. I.; Fu, R. R.et al.; Bland, M. T.; Nathues, A.; Platz, T.; Williams, D. A.; Jaumann, R.; Castillo-Rogez, J. C.; Ruesch, O.; Schmidt, B.; Park, R. S.; Preusker, F.; Buczkowski, D. L.; Russell, C. T.; Raymond, C. A.: Cratering on Ceres: Implications for its crust and evolution. Science 353, aaf4759 (2016)
Musiol, S.; Holohan, E. P.; Cailleau, B.; Platz, T.; Dumke, A.; Walter, T. R.; Williams, D. A.; van Gasselt, S.: Lithospheric flexure and gravity spreading of Olympus Mons volcano, Mars. Journal Geophysical Research 121 (3), pp. 255 - 272 (2016)
Rodriguez, J. A. P.; Fairen, A. G.; Tanaka, K. L.; Zarroca, M.; Linares, R.; Platz, T.; Komatsu, G.; Miyamoto, H.; Kargel, J. S.; Yan, J.et al.; Gulick, V.; Higuchi, K.; Baker, V. R.; Glines, N.: Tsunami waves extensively resurfaced the shorelines of an early Martian ocean. Sci. Rep. 6, 25106 (2016)
Ruesch, O.; Platz, T.; Schenk, P.; McFadden, L. A.; Castillo-Rogez, J. C.; Quick, L. C.; Byrne, S.; Preusker, F.; O'Brien, D. P.; Schmedemann, N.et al.; Williams, D. A.; Li, J.-Y.; Bland, M. T.; Hiesinger, H.; Kneissl, T.; Neesemann, A.; Schaefer, M.; Pasckert, J. H.; Schmidt, B. E.; Buczkowski, D. L.; Sykes, M. V.; Nathues, A.; Roatsch, T.; Hoffmann, M.; Raymond, C. A.; Russell, C. T.: Cryovolcanism on Ceres. Science 353, aaf4286 (2016)
Schorghofer, N.; Mazarico, E.; Platz, T.; Preusker, F.; Schroeder, S. E.; Raymond, C. A.; Russell, C. T.: The permanently shadowed regions of dwarf planet Ceres. Geophysical Research Letters 43 (13), pp. 6783 - 6789 (2016)
Thangjam, G.; Nathues, A.; Mengel, K.; Schäfer, M.; Hoffmann, M.; Cloutis, E. A.; Mann, P.; Müller, C.; Platz, T.; Schäfer, T.: Three-dimensional spectral analysis of compositional heterogeneity at Arruntia crater on (4) Vesta using Dawn FC. Icarus 267, pp. 344 - 363 (2016)
Nathues, A.; Hoffmann, M.; Schaefer, M.; Le Corre, L.; Reddy, V.; Platz, T.; Cloutis, E. A.; Christensen, U.; Kneissl, T.; Li, J.-Y.et al.; Mengel, K.; Schmedemann, N.; Schaefer, T.; Russell, C. T.; Applin, D. M.; Buczkowski, D. L.; Izawa, M. R. M.; Keller, H. U.; OBrien, D. P.; Pieters, C. M.; Raymond, C. A.; Ripken, J.; Schenk, P. M.; Schmidt, B. E.; Sierks, H.; Sykes, M. V.; Thangjam, G. S.; Vincent, J.-B.: Sublimation in bright spots on Ceres. Nature 528, pp. 237 - 240 (2015)
Buczkowski, D. L.; Schenk, P. M.; Scully, J. E. C.; Otto, K.; von der Gathen, I.; Williams, D. A.; Mest, S. C.; Park, R.; Preusker, F.; Jaumann, R.et al.; Roatsch, T.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C. A.; Russell, C. T.: Linear Structures on Ceres: Morphology, Orientation, and Possible Formation Mechanisms. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Buczkowski, D.; Williams, D.; Scully, J.; Mest, S.; Crown, D.; Aileen Yingst, R.; Schenk, P.; Jaumann, R.; Roatsch, T.; Preusker, F.et al.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C.; Russell, C.: Geological Mapping of the Ac-H-9 Occator Quadrangle of Ceres from NASA Dawn Mission. European Geosciences Union General Assembly, Vienna, Austria (2016)
Buczkowski, D. L.; Williams, D. A.; Scully, J. E. C.; Mest, S. C.; Crown, D. A.; Yingst, R. A.; Schenk, P. M.; Jaumann, R.; Roatsch, T.; Preusker, F.et al.; Platz, T.; Nathues, A.; Hoffmann, M.; Schaefer, M.; Marchi, S.; De Sanctis, M. C.; Raymond, C. A.; Russell, C. T.: Geologic Mapping of the Ac-H-9 Occator Quadrangle of Ceres from NASA's Dawn Mission. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
Crown, D.; Yingst, A.; Mest, S.; Platz, T.; Sizemore, H.; Berman, D.; Williams, D.; Roatsch, T.; Preusker, F.; Nathues, A.et al.; Hoffman, M.; Schäfer, M.; Raymond, C.; Russell, C.: Geological Mapping of the Ac-H-14 Yalode Quadrangle of Ceres from NASA's Dawn Mission. European Geosciences Union General Assembly, Vienna, Austria (2016)
Crown, D. A.; Yingst, R. A.; Mest, S. C.; Platz, T.; Sizemore, H. G.; Berman, D. C.; Williams, D. A.; Roatsch, T.; Preusker, F.; Nathues, A.et al.; Hoffman, M.; Schäfer, M.; Raymond, C. A.; Russell, C. T.; the Dawn Science Team: Geologic Mapping of the Ac-H-14 Yalode Quadrangle of Ceres from NASA's Dawn Mission. 47th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2016)
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, ...