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)
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.
First icy cold, then midnight sun: at the Arctic Circle, the team will prepare the next flight of the balloon-borne solar observatory - and hopes for solar fireworks.
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, ...