Dikarev, V.; Preuß, O.; Solanki, S.; Krüger, H.; Krivov, A.: The Local Dust Foregrounds in the Microwave Sky. I. Thermal Emission Spectra. Astrophysical Journal 705, pp. 670 - 682 (2009)
Dikarev, V.; Preuss, O.; Solanki, S. K.; Krüger, H.; Krivov, A.: Understanding the WMAP results: low-order multipoles and dust in the vicinity of the solar system. Earth, Moon and Planets 102, pp. 555 - 561 (2007)
Preuss, O.; Solanki, S. K.; Haugan, M. P.; Jordan, S.: Gravity-induced birefringence within the framework of Poincaré gauge theory. Physical Review D 72, p. 042001 (2005)
Preuss, O.; Haugan, M. P.; Solanki, S. K.; Jordan, S.: An astronomical search for evidence of new physics: Limits on gravity-induced birefringence from the magnetic white dwarf RE J0317-853. Physical Review D 70 (6), 067101 (2004)
Preuss, O.; Schüssler, M.; Holzwarth, V.; Solanki, S. K.: Distribution of magnetically confined circumstellar matter in oblique rotators. Astronomy and Astrophysics 417, pp. 987 - 992 (2004)
Solanki, S. K.; Preuss, O.; Haugan, M.; Gandorfer, A.; Povel, H. P.; Steiner, P.; Stucki, K.; Bernasconi, P. N.; Soltau, D.: Solar constraints on new couplings between electromagnetism and gravity. Physical Review D 69, 062001 (2004)
Neiner, C.; Geers, V. C.; Henrichs, H. F.; Floquet, M.; Frémat, Y. H.; Hubert, A. M.; Preuss, O.; Wiersema, K.: Discovery of a magnetic field in the Slowly Pulsating B star ζ Cassiopeiae. Astronomy and Astrophysics 406 (3), pp. 1019 - 1031 (2003)
Neiner, C.; Henrichs, H. F.; Floquet, M.; Fremat, Y.; Preuss, O.; Hubert, A. M.; Geers, V. C.; Tijani, A. H.; Nichols, J. S.; Jankov, S.: Rotation, pulsations and magnetic field in V 2052 Ophiuchi: A new He-strong star. Astronomy and Astrophysics 411 (3), pp. 565 - 579 (2003)
Neiner, C.; Hubert, A. M.; Frémat, Y.; Floquet, M.; Jankov, S.; Preuss, O.; Henrichs, H. F.; Zorec, J.: Rotation and magnetic field in the Be star ω Orionis. Astronomy and Astrophysics 409 (1), pp. 275 - 286 (2003)
Laemmerzahl, C.; Preuss, O.; Dittus, H.: Is the physics within the Solar system really understood? In: Lasers, Clocks, and Drag-Free: Technologies for Future Exploration in Space and Tests of Gravity (Ed. Laemmerzahl, C.). (2006)
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, ...