Gent, F. A.; Mac Low, M.-M.; Käpylä, M. J.; Singh, N. K.: Small-scale Dynamo in Supernova-driven Interstellar Turbulence. The Astrophysical Journal Letters 910 (2), L15 (2021)
Jingade, N.; Singh, N. K.: Mean field dynamo action in shearing flows - II. Fluctuating kinetic helicity with zero mean. Monthly Notices of the Royal Astronomical Society 508 (4), pp. 5163 - 5175 (2021)
Jingade, N.; Singh, N. K.: Mean field dynamo action in shear flows. I: fixed kinetic helicity. Monthly Notices of the Royal Astronomical Society 495 (4), pp. 4557 - 4569 (2020)
Käpylä, M. J.; Alvarez Vizoso, J.; Rheinhardt, M.; Brandenburg, A.; Käpylä, P.; Singh, N. K.: On the Existence of Shear-current Effects in Magnetized Burgulence. The Astrophysical Journal 905 (2), 179 (2020)
Singh, N. K.; Raichur, H.; Käpylä, M. J.; Rheinhardt, M.; Brandenburg, A.; Käpylä, P. J.: f-mode strengthening from a localised bipolar subsurface magnetic field. Geophysical and Astrophysical Fluid Dynamics 114 (1-2), pp. 196 - 212 (2020)
Brandenburg, A.; Bracco, A.; Kahniashvili, T.; Mandal, S.; Pol, A. R.; Petrie, G. J. D.; Singh, N. K.: E and B Polarizations from Inhomogeneous and Solar Surface Turbulence. The Astrophysical Journal 870 (2), 87 (2019)
Chamandy, L.; Singh, N. K.: Non-linear galactic dynamos and the magnetic Rädler effect. Monthly Notices of the Royal Astronomical Society 481 (1), pp. 1300 - 1319 (2018)
Jingade, N.; Singh, N. K.; Sridhar , S.: Generation of large-scale magnetic fields due to fluctuating α in shearing systems. Journal of Plasma Physics 84 (6), 735840601 (2018)
Jingade, N.; Singh, N. K.; Sridhar, S.: Generation of large-scale magnetic fields due to fluctuating alpha in shearing systems. Journal of Plasma Physics 84 (6), 735840601 (2018)
Singh, N. K.; Käpylä, M. J.; Brandenburg, A.; Käpylä, P. J.; Lagg, A.; Virtanen, I.: Bihelical Spectrum of Solar Magnetic Helicity and Its Evolution. The Astrophysical Journal 863 (2), 182 (2018)
Singh, N. K.; Rogachevskii, I.; Brandenburg, A.: Enhancement of Small-scale Turbulent Dynamo by Large-scale Shear. The Astrophysical Journal Letters 850 (1), L 8 (2017)
Singh, N. K.; Sridhar, S.: Plane shearing waves of arbitrary form: Exact solutions of the Navier-Stokes equations. Eur. Phys. J. Plus 132 (9), 403 (2017)
Singh, N. K.: Bihelical Spectrum of Solar Magnetic Helicity and Its Evolution during cycle 24 from SOLIS/VSM data. Solar Helicities in Theory and Observations: Implications for Space Weather and Dynamo Theory, Stockholm, Schweden (2019)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".