Biskri, S.; Antoine, J. P.; Inhester, B.; Mekideche, F.: Extraction of solar coronal magnetic loops with the directional 2d wavelet transform. Solar Physics 262, pp. 373 - 385 (2010)
Mierla, M.; Inhester, B.; Antunes, A.; Boursier, Y.; Byrne, J. P.; Colaninno, R.; Davila, J.; de Koning, C. A.; Gallagher, P. T.; Gissot, S.et al.; Howard, R. A.; Howard, T. A.; Kramar, M.; Lamy, P.; Liewer, P. C.; Maloney, S.; Marque, C.; McAteer, T. J.; Moran, T.; Rodriguez, L.; Srivastava, N.; Cyr, O. C. S.; Stenborg, G.; Temmer, M.; Thernisien, A.; Vourlidas, A.; West, M. J.; Wood, B. E.; Zhukov, A. N.: On the 3-D reconstruction of Coronal Mass Ejections using coronagraph data. Annales Geophysicae 28 (1), pp. 203 - 215 (2010)
Wiegelmann, T.; Inhester, B.: How to deal with measurement errors and lacking data in nonlinear force-free coronal magnetic field modelling? Astronomy and Astrophysics 516, A107 (2010)
DeRosa, M. L.; Schrijver, C. J.; Barnes, G.; Leka, K. D.; Lites, B. W.; Aschwanden, M. J.; Amari, T.; Canou, A.; McTiernan, J. M.; Régnier, S.et al.; Thalmann, J. K.; Valori, G.; Wheatland, M. S.; Wiegelmann, T.; Cheung, M. C. M.; Conlon, P. A.; Fuhrmann, M.; Inhester, B.; Tadesse, T.: A Critical Assessment of Nonlinear Force-Free Field Modeling of the Solar Corona for Active Region 10953. Astrophysical Journal 696, pp. 1780 - 1791 (2009)
Kramar, M.; Jones, S.; Davila, J.; Inhester, B.; Mierla, M.: On the Tomographic Reconstruction of the 3D Electron Density for the Solar Corona from STEREO COR1 Data. Solar Physics 259 (1-2), pp. 109 - 121 (2009)
Mierla, M.; Inhester, B.; Marque, C.; Rodriguez, L.; Gissot, S.; Zhukov, A. N.; Berghmans, D.; Davila, J.: On 3D Reconstruction of Coronal Mass Ejections: I. Method Description and Application to SECCHI-COR Data. Solar Physics 259 (1-2), pp. 123 - 141 (2009)
Srivastava, N.; Inhester, B.; Mierla, M.; Podlipnik, B.: 3D Reconstruction of the Leading Edge of the 20 May 2007 Partial Halo CME. Solar Physics 259 (1-2), pp. 213 - 225 (2009)
Tadesse, T.; Wiegelmann, T.; Inhester, B.: Nonlinear force-free coronal magnetic field modelling and preprocessing of vector magnetograms in spherical geometry. Astronomy and Astrophysics 508, pp. 421 - 432 (2009)
Wiegelmann, T.; Inhester, B.; Feng, L.: Solar stereoscopy where are we and what developments do we require to progress? Annales Geophysicae 27, pp. 2925 - 2936 (2009)
Aschwanden, M. J.; Burlaga, L. F.; Kaiser, M. L.; Ng, C. K.; Reames, D. V.; Reiner, M. J.; Gombosi, T. I.; Lugaz, N.; Manchester, W.; Roussev, I. I.et al.; Zurbuchen, T. H.; Farrugia, C. J.; Galvin, A. B.; Lee, M. A.; Linker, J. A.; Mikić, Z.; Riley, P.; Alexander, D.; Sandman, A. W.; Cook, J. W.; Howard, R. A.; Odstrčil, D.; Pizzo, V. J.; Kóta, J.; Liewer, P. C.; Luhmann, J. G.; Inhester, B.; Schwenn, R. W.; Solanki, S. K.; Vasyliūnas, V. M.; Wiegelmann, T.; Blush, L.; Bochsler, P.; Cairns, I. H.; Robinson, P. A.; Bothmer, V.; Kecskemety, K.; Llebaria, A.; Maksimovic, M.; Scholer, M.; Wimmer-Schweingruber, R. F.: Theoretical Modeling for the Stereo Mission. Space Science Reviews 136, pp. 565 - 604 (2008)
Mierla, M.; Davila, J.; Thompson, W.; Inhester, B.; Srivastava, N.; Kramar, M.; St. Cyr, O. C.; Stenborg, G.; Howard, R. A.: A Quick Method for Estimating the Propagation Direction of Coronal Mass Ejections Using STEREO-COR1 Images. Solar Physics 252, pp. 385 - 396 (2008)
Ruan, P.; Wiegelmann, T.; Inhester, B.; Neukirch, T.; Solanki, S. K.; Feng, L.: A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum. Astronomy and Astrophysics 481, pp. 827 - 834 (2008)
Aschwanden, M. J.; Lee, J. K.; Gary, G. A.; Smith, M.; Inhester, B.: Comparison of Five Numerical Codes for Automated Tracing of Coronal Loops. Solar Physics 248, pp. 359 - 377 (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, ...