Thomas, N.; Davidsson, B.; El-Maarry, M. R.; Fornasier, S.; Giacomini, L.; Gracia-Berna, A. G.; Hviid, S. F.; Ip, W.-H.; Jorda, L.; Keller, H. U.et al.; Knollenberg, J.; Kührt, E.; La Forgia, F.; Lai, I. L.; Liao, Y.; Marschall, R.; Massironi, M.; Mottola, S.; Pajola, M.; Poch, O.; Pommerol, A.; Preusker, F.; Scholten, F.; Su, C. C.; Wu, J. S.; Vincent, J.-B.; Sierks, H.; Barbieri, C.; Lamy, P. L.; Rodrigo, R.; Koschny, D.; Rickman, H.; A'Hearn, M. F.; Barucci, M. A.; Bertaux, J.-L.; Bertini, I.; Cremonese, G.; Da Deppo, V.; Debei, S.; de Cecco, M.; Fulle, M.; Groussin, O.; Gutierrez, P. J.; Kramm, J.-R.; Küppers, M.; Lara, L. M.; Lazzarin, M.; Lopez Moreno, J. J.; Marzari, F.; Michalik, H.; Naletto, G.; Agarwal, J.; Güttler, C.; Oklay, N.; Tubiana, C.: Redistribution of particles across the nucleus of comet 67P/Churyumov-Gerasimenko. Astronomy and Astrophysics 583, A17 (2015)
Schmedemann, N.; Kneissl, T.; Ivanov, B. A.; Michael, G. G.; Wagner, R. J.; Neukum, G.; Ruesch, O.; Hiesinger, H.; Krohn, K.; Roatsch, T.et al.; Preusker, F.; Sierks, H.; Jaumann, R.; Reddy, V.; Nathues, A.; Walter, S. H. G.; Neesemann, A.; Raymond, C. A.; Russell, C. T.: The cratering record, chronology and surface ages of (4) Vesta in comparison to smaller asteroids and the ages of HED meteorites. Planetary and Space Science 103, pp. 104 - 130 (2014)
Vincent, J.-B.; Schenk, P.; Nathues, A.; Sierks, H.; Hoffmann, M.; Gaskell, R. W.; Marchi, S.; O'Brien, D. P.; Sykes, M.; Russell, C. T.et al.; Fulchignoni, M.; Keller, H. U.; Raymond, C.; Palmer, E.; Preusker, F.: Crater Depth-to-Diameter Distribution and Surface Properties of (4)Vesta. Planetary and Space Science 103, pp. 57 - 65 (2014)
Le Corre, L.; Reddy, V.; Schmedemann, N.; Becker, K. J.; O'Brien, D. P.; Yamashita, N.; Peplowski, P. N.; Prettyman, T. H.; Li, J.-Y.; Cloutis, E. A.et al.; Denevi, B. W.; Kneisl, T.; Palmer, E.; Gaskell, R. W.; Nathues, A.; Gaffey, M. J.; Mittlefehldt, D. W.; Garry, W. B.; Sierks, H.; Russell, C. T.; Raymond, C. A.; De Sanctis, M. C.; Ammanito, E.: Olivine or impact melt: Nature of the ``Orange'' material on Vesta from Dawn. Icarus 226 (2), pp. 1568 - 1594 (2013)
Reddy, V.; Le Corre, L.; O'Brien, D. P.; Nathues, A.; Cloutis, E. A.; Durda, D. D.; Bottke, W. F.; Bhatt, M. U.; Nesvorny, D.; Buczkowski, D.et al.; Scully, J. E. C.; Palmer, E. M.; Sierks, H.; Mann, P. J.; Becker, K. J.; Beck, A. W.; Mittlefehldt, D.; Li, J.-Y.; Gaskell, R.; Russell, C. T.; Gaffey, M. J.; McSween, H. Y.; McCord, T. B.; Combe, J.-P.; Blewett, D.: Corrigendum to ``Delivery of dark material to Vesta via carbonaceous chondritic impacts'' [Icarus 221, pg 544, 2012]. Icarus 223 (1), p. 632 - 632 (2013)
Reddy, V.; Li, J.-Y.; Le Corre, L.; Scully, J. E. C.; Gaskell, R.; Russell, C. T.; Park, R. S.; Nathues, A.; Raymond, C.; Gaffey, M. J.et al.; Sierks, H.; Becker, K. J.; McFadden, L. A.: Comparing Dawn, Hubble Space Telescope, and ground-based interpretations of (4) Vesta. Icarus 226 (1), pp. 1103 - 1114 (2013)
Thangjam, G.; Reddy, V.; Le Corre, L.; Nathues, A.; Sierks, H.; Hiesinger, H.; li, J.-Y.; Sanchez, J. A.; Russell, C. T.; Gaskell, R.et al.; Raymond, C.: Lithologic mapping of HED terrains on Vesta using Dawn Framing Camera color data. Meteoritics and Planetary Science 48, pp. 2199 - 2210 (2013)
Vincent, J.-B.; Lara, L. M.; Tozzi, G. P.; Lin, Z.-Y.; Sierks, H.: Spin and activity of comet 67P/Churyumov-Gerasimenko. Astronomy and Astrophysics 549, A121 (2013)
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, ...