Usoskin, I.; Solanki, S. K.; Schüssler, M.; Mursula, K.; Alanko, K.: Millenium-scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s. Physical Review Letters 91, 211101 (2003)
Zhang, J.; Solanki, S. K.; Wang, J.: On the nature of moving magnetic feature pairs around sunspots. Astronomy and Astrophysics 399, pp. 755 - 761 (2003)
Zhang, J.; Woch, J.; Solanki, S. K.; von Steiger, R.; Forsyth, R.: Interplanetary and solar surface properties of coronal holes obseved during solar maximum. Journal Geophysical Research 108 (A4), 1144 (2003)
Berdyugina, S. V.; Solanki, S. K.: The molecular Zeeman effect and diagnostics of solar and stellar magnetic fields. I. Theoretical spectral patterns in the Zeeman regime. Astronomy and Astrophysics 385, pp. 701 - 715 (2002)
Brkovic, A.; Landi, E.; Landini, M.; Rüedi, I.; Solanki, S. K.: Models for solar magnetic loops. II: Comparison with SOHO observations on the solar disk. Astronomy and Astrophysics 383, pp. 661 - 677 (2002)
Krivova, N. A.; Solanki, S. K.: The 1.3-year and 156-day periodicities in sunspot data: wavelet analysis suggests a common origin. Astronomy and Astrophysics 394, pp. 701 - 706 (2002)
Ortiz, A.; Solanki, S. K.; Domingo, V.; Fligge, M.; Sanahuja, B.: On the intensity contrast of solar photospheric faculae and network elements. Astronomy and Astrophysics 388, pp. 1036 - 1047 (2002)
Solanki, S. K.; Fligge, M.: How much of the solar irradiance variation is caused by the magnetic field at the solar surface? Advances in Space Research 29, pp. 1933 - 1940 (2002)
Solanki, S. K.; Krivova, N. A.; Schüssler, M.; Fligge, M.: Search for a relationship between solar cycle amplitude and length. Astronomy and Astrophysics 396, pp. 1029 - 1035 (2002)
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.