Kramar, M.; Inhester, B.: Inversion of coronal Zeeman and Hanle Observations to reconstruct the coronal magnetic field. Memorie della Società Astronomica Italiana 78 (1), pp. 120 - 125 (2007)
Wiegelmann, T.; Neukirch, T.; Ruan, P.; Inhester, B.: Optimization approach for the computation of magnetohydrostatic coronal equilibria in spherical geometry. Astronomy and Astrophysics 475, pp. 701 - 706 (2007)
Inhester, B.; Wiegelmann, T.: Nonlinear force-free magnetic field extrapolations: comparisonof the Grad-Rubin and Wheatland-Sturrock-Roumeliotis algorithm. Solar Physics 235, pp. 201 - 221 (2006)
Kramar, M.; Inhester, B.; Solanki, S. K.: Vector tomography for the coronal magnetic field. I. Longitudinal Zeeman effect measurements. Astronomy and Astrophysics 456, pp. 665 - 673 (2006)
Wiegelmann, T.; Inhester, B.; Kliem, B.; Valori, G.; Neukirch, T.: Testing non-linear force-free coronal magnetic field extrapolations with the Titov-Démoulin equilibrium. Astronomy and Astrophysics 453, pp. 737 - 741 (2006)
Wiegelmann, T.; Inhester, B.; Sakurai, T.: Preprocessing of vector magnetograph data for a nonlinear force-free magnetic field reconstruction. Solar Physics 233, pp. 215 - 232 (2006)
Raouafi, N.-E.; Mancuso, S.; Solanki, S. K.; Inhester, B.; Mierla, M.; Stenborg, G.; Delaboudiniere, J. P.; Benna, C.: Shock wave driven by an expanding system of loops. Astronomy and Astrophysics 424 (3), pp. 1039 - 1048 (2004)
Wiegelmann, T.; Inhester, B.: Magnetic modelling and tomography: First steps towards a consistent reconstruction of the solar corona. Solar Physics 214, pp. 287 - 312 (2003)
Wilhelm, K.; Inhester, B.; Newmark, J. S.: The inner solar corona seen by SUMER, LASCO/C1, and EIT: Electron densities and temperatures during the rise of the new solar cycle. Astronomy and Astrophysics 382, pp. 328 - 341 (2002)
Portier-Fozzani, F.; Inhester, B.: 3D Coronal structures and their evolutions measured by Stereoscopy, consequences for Space Weather and the STEREO mission. Space Science Reviews 97 (1/4), p. 51 (2001)
Srivastava, N.; Schwenn, R.; Inhester, B.; Martin, S. F.; Hanaoka, Y.: Factors related to the origin of a gradual coronal mass ejection associated with an eruptive prominence on 1998 June 21-22. Astrophysical Journal 534, pp. 468 - 481 (2000)
Innes, D. E.; Inhester, B.; Srivastava, N.; Brekke, P.; Harrison, R. A.; Matthews, S. A.; Noëns, J. C.; Schmieder, B.; Thompson, B. J.: Multi-wavelength observations of the onset phase of a coronal mass ejection. Solar Physics 186, pp. 337 - 361 (1999)
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, ...