Goetz, W.; Hecht, M. H.; Hviid, S. F.; Madsen, M. B.; Pike, W. T.; Staufer, U.; Velbel, M. A.; Harrit, N. H.; Zych, E.; Edgett, K. S.: Search for ultraviolet luminescence of soil particles at the Phoenix landing site, Mars. Planetary and Space Science 70 (1), pp. 134 - 147 (2012)
Küppers, M.; Moissl, R.; Vincent, J.-B.; Besse, S.; Hviid, S. F.; Carry, B.; Grieger, B.; Sierks, H.; Keller, H. U.; Marchi, S.et al.; the team, O.: Boulders on Lutetia. Planetary and Space Science 66 (1), pp. 71 - 78 (2012)
Fornasier, S.; Mottola, S.; Barucci, M. A.; Sierks, H.; Hviid, S.: Photometric observations of asteroid 4 Vesta by the OSIRIS cameras onboard the Rosetta spacecraft. Astronomy and Astrophysics 533, L9 (2011)
Goetz, W.; Pike, W. T.; Hviid, S. F.; Madsen, M. B.; Morris, R. V.; Hecht, M. H.; Staufer, U.; Leer, K.; Sykulska, H.; Hemmig, E.et al.; Marshall, J.; Morookian, J. M.; Parrat, D.; Vijendran, S.; Bos, B. J.; El Maarry, M. R.; Keller, H. U.; Kramm, R.; Markiewicz, W. J.; Drube, L.; Blaney, D.; Arvidson, R. E.; Bell III, J. F.; Reynolds, R.; Smith, P. H.; Woida, P.; Woida, R.; Tanner, R.: Microscopy analysis of soils at the Phoenix landing site, Mars: Classification of soil particles and description of their optical and magnetic properties. Journal Geophysical Research 115, E00E22 (2010)
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Lamy, P. L.; Faury, G.; Jorda, L.; Kaasalainen, M.; Hviid, S. F.: Multi-color, rotationally resolved photometry of asteroid 21 Lutetia from OSIRIS/Rosetta observations. Astronomy and Astrophysics 521, A19 (2010)
Luethi, B. S.; Thomas, N.; Hviid, S. F.; Rueffer, P.: An efficient autofocus algorithm for a visible microscope on a Mars lander. Planetary and Space Science 58 (10), pp. 1258 - 1264 (2010)
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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, ...