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)
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.
Application deadline 1 October 2023. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
Philipp Löschl has co-authored an excellent publication on Solar Orbiter data which has been awarded best Solar Physics paper of 2022 (Gherardo Valori et al. 2022)