Wilhelm, K.: Ergebnisse des Gauß-Versuchs im cgs-Einheitensystem und im Système International d'unités (SI, 9e éd. 2019). Mitteilungen der Gauss-Gesellschaft 58, pp. 67 - 70 (2021)
Wilhelm, K.; Dwivedi, B. N.: On the radial acceleration of disc galaxies. Monthly Notices of the Royal Astronomical Society 494 (3), pp. 4015 - 4025 (2020)
Rao, Y. K.; Srivastava, A. K.; Kayshap, P.; Wilhelm, K.; Dwivedi, B. N.: Plasma Flows in the Cool Loop Systems. The Astrophysical Journal 874 (1), 56 (2019)
Wilhelm, K.; Dwivedi, B. N.: A physical process of the radial acceleration of disc galaxies. Monthly Notices of the Royal Astronomical Society 474 (4), pp. 4723 - 4729 (2018)
Lemaire, P.; Vial, J.-C.; Curdt, W.; Schühle, U.; Wilhelm, K.: Hydrogen Ly-α and Ly-β full Sun line profiles observed with SUMER/SOHO (1996-2009). Astronomy and Astrophysics 581, A26, pp. 1 - 7 (2015)
Wilhelm, K.; Dwivedi, B. N.: Increase of the mean Sun-Earth distance caused by a secular mass accumulation. Astrophysics and Space Science 347, pp. 41 - 45 (2013)
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.