Bloomfield, D. S.; Solanki, S. K.; Lagg, A.; Borrero, J. M.; Cally, P. S.: Modified p-modes in penumbral filaments? Astronomy and Astrophysics 469, pp. 1155 - 1161 (2007)
Jess, D. B.; Andic, A.; Mathioudakis, M.; Bloomfield, D. S.; Keenan, F. P.: High-frequency oscillations in a solar active region observed with the RAPID DUAL IMAGER. Astronomy and Astrophysics 473, pp. 943 - 950 (2007)
Jess, D. B.; McAteer, R. T. J.; Mathioudakis, M.; Keenan, F. P.; Andic, A.; Bloomfield, D. S.: Twisting flux tubes as a cause of micro-flaring activity. Astronomy and Astrophysics 476 (2), pp. 971 - 977 (2007)
Bloomfield, D. S.; McAteer, R. T. J.; Mathioudakis, M.; Keenan, F. P.: The influence of magnetic field on oscillations in the solar chromosphere. Astrophysical Journal 652, pp. 812 - 819 (2006)
Bloomfield, D. S.; Lagg, A.; Solanki, S. K.: The nature of running penumbral waves revealed. In: Proc. IAU Symposium 247 ``Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology'', pp. 55 - 58 (Eds. Erdélyi, R.; Mendoza-Briceno, C. A.). International Astronomical Union (2008)
Bloomfield, D. S.; Lagg, A.; Solanki, S. K.: Observations of running waves in a sunspot chromosphere. In: The Physics of Chromospheric Plasmas, pp. 239 - 244 (Eds. Heinzel, P.; Dorotovič, I.; Rutten, R. J.). ASP, San Francisco (2007)
Bloomfield, D. S.; Lagg, A.; Solanki, S. K.; Borrero, J. M.: Modified p-modes in penumbral filaments. In: Modern Solar Facilities - Advanced Solar Science, pp. 241 - 244 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen (2007)
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, ...