Stubbe, P.; Kopka, H.: On the ionospheric modification experiment projected at MPI Lindau: Scientific objectives. In: AGARD Artificial Modification of Propagation Media, p. 9-1-9-11. (1977)
Stubbe, P.; Kopka, H.; Zwick, R.: On the ionospheric modification experiment projected at MPI Lindau: Practival realization. In: AGARD Artificial Modification of Propagation Media, p. 10-1-10-7. (1977)
Stubbe, P.: The F-region - A Review. In: Atmospheres of Earth and the Planets, pp. 269 - 280 (Ed. McCormac, B. M.). D. Reidel Publishing Company, Dordrecht (1975)
Chandra, S.; Stubbe, P.: Ionen- und Neutralgaszusammensetzung während eines magnetischen Sturmes. In: Kleinheubacher Berichte 14, pp. 183 - 187. (1971)
Stubbe, P.: The effect of electric fields on the F regin behaviour as compared with neutral wind effects. In: Proc Symposium Future Appl. Satellite Beacon Exper., p. 32-1-32-7. (1970)
Stubbe, P.: On the possibility of evaluating the hydrogen concentration in the upper atmosphere by comparing the bottomside and topside electron contents. In: Proc. Symposium Future Appl. Satellite Beacon Exper., p. 32-1}-{32-7. (1970)
Stubbe, P.: The attachment coefficient in the F-layer and its temperature dependence. In: Proc. of the Advanced Study Institute, Finse (Norway) April 1965, pp. 249 - 257. North-Holland Publishing Company, Amsterdam 1966 (1966)
Becker, W.; Stubbe, P.: Temperature variation in the F region during the last sunspot cycle. In: Proc. Intern. Conf. Ion., London July 1962. The Institute of Pysics and the Physical Society London 1963, pp. 35 - 42. (1963)
Stubbe, P.: Das photochemische, dynamische und thermodynamische Verhalten der oberen Ionosphere. Habilitation, Georg-August-Universität Göttingen (1973)
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".
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.