Jordan, S.; Aznar Cuadrado, R.; Napiwotzki, R.; Schmid, H. M.; Solanki, S. K.: The fraction of DA white dwarfs with kilo-Gauss magnetic fields. Astronomy and Astrophysics 462, pp. 1097 - 1101 (2007)
Krivova, N. A.; Balmaceda, L.; Solanki, S. K.: Reconstruction of solar total irradiance since 1700 from the surface magnetic flux. Astronomy and Astrophysics 467, pp. 335 - 346 (2007)
Lagg, A.; Woch, J.; Solanki, S. K.; Krupp, N.: Supersonic Downflows in the Vicinity of a Growing Pore: Evidence of unresolved magnetic fine structure at chromospheric heights. Astronomy and Astrophysics 462, pp. 1147 - 1155 (2007)
Martínez González, M. J.; Collados, M.; Ruiz Cobo, B.; Solanki, S. K.: Low-lying magnetic loops in the solar internetwork. Astronomy and Astrophysics 469, pp. L39 - L42 (2007)
Mathew, S. K.; Martínez Pillet, V.; Solanki, S. K.; Krivova, N. A.: Properties of sunspots in cycle 23. I. Dependence of brightness on sunspot size and cycle phase. Astronomy and Astrophysics 465, pp. 291 - 304 (2007)
Raouafi, N.-E.; Harvey, J. W.; Solanki, S. K.: Properties of solar polar coronal plumes constrained by UVCS data. Astrophysical Journal 658, pp. 643 - 656 (2007)
Selwa, M.; Murawski, K.; Solanki, S. K.; Wang, T. J.: Energy leakage as an attenuation mechanism for vertical kink oscillations in solar coronal wave guides. Astronomy and Astrophysics 462, pp. 1127 - 1135 (2007)
Tripathi, D.; Solanki, S. K.; Mason, H. E.; Webb, D. F.: A bright coronal downflow seen in multi-wavelength observations: Evidence of a bifurcating flux-rope? Astronomy and Astrophysics 472, pp. 633 - 642 (2007)
Usoskin, I. G.; Solanki, S. K.; Kovaltsov, G. A.: Grand minima and maxima of solar activity: New observational constraints. Astronomy and Astrophysics 471, pp. 301 - 309 (2007)
Zakharov, V.; Gandorfer, A.; Solanki, S. K.; Löfdahl, A.: Erratum in ``A comparative study of the contrast of solar magnetic elements in CN and CH'' (vol 437, pg L43, 2005). Astronomy and Astrophysics 461 (2), p. 695 - 695 (2007)
Zhang, J.; Solanki, S. K.; Woch, J.: Discovery of inward moving magnetic enhancements in sunspot penumbrae. Astronomy and Astrophysics 475 (2), pp. 695 - 700 (2007)
Zhang, J.; Solanki, S. K.; Woch, J.; Wang, J.: The velocity structure of moving magnetic feature pairs around sunspots: Support for the U-loop model. Astronomy and Astrophysics 471, pp. 1035 - 1041 (2007)
Borrero, J. M.; Solanki, S. K.; Lagg, A.; Socas-Navarro, H.; Lites, B.: On the fine structure of sunspot penumbrae: III. The vertical extension of penumbral filaments. Astronomy and Astrophysics 450, pp. 383 - 393 (2006)
Gandorfer, A. M.; Solanki, S. K.; Barthol, P.; Lites, B. W.; Martínez Pillet, V.; Schmidt, W.; Soltau, D.; Title, A. M.: SUNRISE: High resolution UV/VIS observations of the Sun from the stratosphere. Proceedings of the SPIE 6267, 62670S (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)
Loukitcheva, M.; Solanki, S. K.; White, S.: The dynamics of the solar chromosphere: comparison of model predictions with millimeter-interferometer observations. Astronomy and Astrophysics 456, pp. 713 - 723 (2006)
Raouafi, N.-E.; Solanki, S. K.: Sensitivity of solar off-limb line profiles to electron density stratification and the velocity distribution anisotropy. Astronomy and Astrophysics 445, pp. 735 - 745 (2006)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.