Davidsson, B. J. R.; Schloerb, F. P.; Fornasier, S.; Oklay, N.; Gutiérrez, P. J.; Buratti, B. J.; Chmielewski, A. B.; Gulkis, S.; Hofstadter, M. D.; Keller, H. U.et al.; Sierks, H.; Güttler, C.; Küppers, M.; Rickman, H.; Choukroun, M.; Lee, S.; Lellouch, E.; Lethuillier, A.; Da Deppo, V.; Groussin, O.; Kührt, E.; Thomas, N.; Tubiana, C.; El-Maarry, M. R.; La Forgia, F.; Mottola, S.; Pajola, M.: CO2-driven surface changes in the Hapi region on Comet 67P/Churyumov-Gerasimenko. Monthly Notices of the Royal Astronomical Society 516, pp. 6009 - 6040 (2022)
Haslebacher, N.; Gerig, S.-B.; Thomas, N.; Marschall, R.; Zakharov, V.; Tubiana, C.: A numerical model of dust particle impacts during a cometary encounter with application to ESA's Comet Interceptor mission. Acta Astronautica 195, pp. 243 - 250 (2022)
Buratti, B. J.; Britt, D. T.; Soderblom, L. A.; Hicks, M. D.; Boice, D. C.; Brown, R. H.; Meier, R.; Nelson, R. M.; Oberst, J.; Owen, T. C.et al.; Rivkin, A. S.; Sandel, B. R.; Stern, S. A.; Thomas, N.; Yelle, R. V.: 9969 Braille: Deep Space 1 infrared spectroscopy, geometric albedo, and classification. Icarus 167 (1), pp. 129 - 135 (2004)
Thomas, N.; Lüthi, B. S.; Hviid, S. F.; Keller, H. U.; Markiewicz, W. J.; Blümchen, T.; Basilevsky, A. T.; Smith, P. H.; Tanner, R.; Oquest, C.et al.; Reynolds, R.; Josset, J.-L.; Beauvivre, S.; Hofmann, B.; Rüffer, P.; Pillinger, C. T.: The microscope for Beagle 2. Planetary and Space Science 52 (9), pp. 853 - 866 (2004)
Ho, T. M.; Thomas, N.; Boice, D. C.; Köllein, C.; Soderblom, L. A.: Comparative study of the dust emission of 19P/Borrelly (Deep Space 1) and 1P/Halley. Advances in Space Research 31 (12), pp. 2583 - 2589 (2003)
Barucci, M. A.; Boehnhardt, H.; Dotto, E.; Doressoundiram, A.; Romon, J.; Lazzarin, M.; Fornasier, S.; de Bergh, C.; Tozzi, G. P.; Delsanti, A.et al.; Hainaut, O.; Barrera, L.; Birkle, K.; Meech, K.; Ortiz, J. L.; Sekiguchi, T.; Thomas, N.; Watanabe, J.; West, R. M.; Davies, J. K.: Visible and near-infrared spectroscopy of the Centaur 32532 (2001 PT13). ESO Large Programm on TNOs and Centaurs: First spectroscopy results. Astronomy and Astrophysics 392, pp. 335 - 339 (2002)
Boice, D. C.; Soderblom, L. A.; Britt, D. T.; Brown, R. H.; Sandel, B. R.; Yelle, R. V.; Buratti, B. J.; Hicks, M. D.; Nelson, R. M.; Rayman, M. D.et al.; Oberst, J.; Thomas, N.: The Deep Space 1 encounter with comet 19P/Borrelly. Earth, Moon and Planets 89 (1-4), pp. 301 - 324 (2002)
Markiewicz, W. J.; Keller, H. U.; Thomas, N.; Titov, D.; Forget, F.: Optical properties of the Martian aerosols in the visible spectral range. Advances in Space Research 29 (2), pp. 175 - 181 (2002)
Popp, J.; Tarcea, N.; Kiefer, W.; Hilchenbach, M.; Thomas, N.; Stuffler, T.; Hofer, S.; Stoffler, D.; Greshake, A.: The effect of surface texture on the mineralogical analysis of chondritic meteorites using Raman spectroscopy. Planetary and Space Science 50 (9), pp. 865 - 870 (2002)
Soderblom, L. A.; Becker, T. L.; Bennett, G.; Boice, D. C.; Britt, D. T.; Brown, R. H.; Buratti, B. J.; Isbell, C.; Giese, B.; Hare, T.et al.; Hicks, M. D.; Howington-Kraus, E.; Kirk, R. L.; Lee, M.; Nelson, R. M.; Oberst, J.; Owen, T. C.; Rayman, D. M.; Sandel, B. R.; Stern, A. S.; Thomas, N.; Yelle, R. V.: Observations of Comet 19P/Borrelly by the Miniature Integrated Camera and Spectrometer Aboard Deep Space 1. Science 296, pp. 1087 - 1091 (2002)
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, ...