Jockers, K.; Szutowicz, S.; Villanueva, G.; Bonev, T.; Hartogh, P.: HCN and CN in Comet 2P/Encke: Models of the non-isotropic, rotation-modulated coma and CN parent life time. Icarus 215, pp. 153 - 185 (2011)
Petrova, E. V.; Tishkovets, V. P.; Jockers, K.: Interaction of Particles in the Near Field and Opposition Effects in Regolith-Like Surfaces. Solar System Research 43, pp. 100 - 115 (2009)
Bonev, T.; Jockers, K.; Karpov, N.: A dynamical model with a new inversion technique applied to observations of Comet WM1 (LINEAR). Icarus 197, pp. 183 - 202 (2008)
Petrova, E. V.; Tishkovets, V. P.; Jockers, K.: Rebuttal to comment on Modeling of opposition effects with ensembles of clusters: Interplay of various scattering mechanisms by Elena V. Petrova, Victor P. Tishkovets, Klaus Jockers, 2007 [Icarus 188, 233245]. Icarus 194, pp. 853 - 856 (2008)
Petrova, E.; Tishkovets, V. P.; Jockers, K.: Modelling of opposition effects with ensembles of clusters: Interplay of various scattering mechanisms. Icarus 188, pp. 233 - 245 (2007)
Yankulova, I. M.; Golev, V. K.; Jockers, K.: The luminous infrared composite Seyfert 2 galaxy NGC 7679 through the [O III] λ 5007 emission line. Astronomy and Astrophysics 469 (3), pp. 891 - 898 (2007)
Tishkovets, V. P.; Jockers, K.: Multiple scattering of light by densely packed random media of spherical particles: Dense media vector radiative transfer equation. J. Quant. Spectrosc. Radiat. Transf. 101, pp. 54 - 72 (2006)
Kiselev, N.; Rosenbush, V.; Jockers, K.; Velichko, S.; Sen, K. K.: Database of comet polarimetry: Analysis and some results. Earth, Moon and Planets 97 (3-4), pp. 365 - 378 (2005)
Rosenbush, V. K.; Kiselev, N. N.; Shevchenko, V. G.; Jockers, K.; Shakhovskoy, N. M.; Efimov, Y. S.: Polarization and brightness opposition effects for the E-type Asteroid 64 Angelina. Icarus 178 (1), pp. 222 - 234 (2005)
Grynko, Y.; Jockers, K.; Schwenn, R.: The phase curve of cometary dust: Observations of comet 96P/Machholz 1 at large phase angle with the SOHO LASCO C3 coronagraph. Astronomy and Astrophysics 427 (2), pp. 755 - 761 (2004)
Kulyk, I.; Jockers, K.; Credner, T.; Bonev, T.: The wavelength dependence of the monochromatic extinction coefficient for the observatory on Terskol Peak. Kinematika i Fizika Nebesnykh Tel 20, pp. 372 - 378 (2004)
Petrova, E. V.; Tishkovets, V. P.; Jockers, K.: Polarization of Light Scattered by Solar System Bodies and the Aggregate Model of Dust Particles. Solar System Research 38, pp. 309 - 324 (2004)
Tishkovets, V. P.; Petrova, E. V.; Jockers, K.: Optical properties of aggregate particles comparable in size to the wavelength. J. Quant. Spectrosc. Radiat. Transf. 86 (3), pp. 241 - 265 (2004)
Bonev, T.; Jockers, K.; Petrova, E.; Delva, M.; Borisov, G.; Ivanova, A.: The dust in comet C/1999 S4 (LINEAR) during its disintegration: Narrow-band images, color maps, and dynamical models. Icarus 160, pp. 419 - 436 (2002)
Kiselev, N.; Jockers, K.; Rosenbush, V.: Comparative study of the dust polarimetric properties in split and normal comaes. Earth, Moon and Planets 90, pp. 167 - 176 (2002)
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, ...