Attie, R.; Innes, D. E.; Solanki, S. K.; Glassmeier, K.-H.: Relationship between supergranulation flows, magnetic cancellation and network flares. Astronomy and Astrophysics 596, A15 (2016)
Yousefzadeh, M.; Safari, H.; Attie, R.; Alipour, N.: Motion and Magnetic Flux Changes of Coronal Bright Points Relative to Supergranular Cell Boundaries. Solar Physics 291, pp. 29 - 39 (2015)
Attie, R.; Innes, D. E.; Potts, H. E.: Evidence of photospheric vortex flows at supergranular junctions observed by FG/SOT (Hinode). Astronomy and Astrophysics 493 (2), pp. L13 - L16 (2009)
Innes, D. E.; Genetelli, A.; Attie, R.; Potts, H. E.: Quiet Sun mini-coronal mass ejections activated by supergranular flows. Astronomy and Astrophysics 495, p. 319 (2009)
Innes, D. E.; Attie, R.; Hara, H.; Madjarska, M. S.: EIS/ Hinode Observations of Doppler Flow Seen through the 40-Arcsec Wide-Slit. Solar Physics 252, pp. 283 - 292 (2008)
Attie, R.; Innes, D. E.: Explosive Event in the Quiet Sun Seen by XRT-EIS and SUMER. In: First Results From Hinode, p. 155 (Eds. Matthews, S. A.; Davis, J. M.; Harra, L. K.). Astronomical Society of the Pacific, San Francisco (2008)
Attie, R.: The relationship between supergranulation flows, magnetic field evolution and network flares. Dissertation, Tech. Univ. Braunschweig, Braunschweig, Braunschweig (2015)
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, ...