Chandra, S.; Maier, E. J.; Stubbe, P.: The upper atmosphere as a regulator of subauroral red arcs. Planetary and Space Science 20, pp. 461 - 472 (1972)
Chandra, S.; Stubbe, P.: The development of a theoretical model of the atmosphere and ionosphere. Journal of Atmospheric and Terrestrial Physics 34, pp. 1627 - 1633 (1972)
Stubbe, P.: The influence of neutral winds on the NO+ and O2+ densities in the lower ionosphere at night. Journal of Atmospheric and Terrestrial Physics 34, pp. 519 - 523 (1972)
Stubbe, P.: Vertical neutral gas motions and deviations from the barometric law in the lower thermosphere. Planetary and Space Science 20, pp. 209 - 215 (1972)
Chandra, S.; Stubbe, P.: Ion and neutral composition changes in the thermospheric region during magnetic storms. Planetary and Space Science 19, pp. 491 - 502 (1971)
Chandra, S.; Stubbe, P.: On explaining the F-region seasonal anomaly in terms of composition changes in the lower atmosphere. Planetary and Space Science 19, pp. 1014 - 1016 (1971)
Stubbe, P.: Bemerkungen zu der Arbeit von W. Becker, ``Einige Ergebnisse aus Lindauer Elektronendichteprofil-Berechnungen für die innere und äußere Ionosphäre.''. KLeinheubacher Berichte 14, pp. 155 - 158 (1971)
Stubbe, P.; Chandra, S.: On explaining the magnetic storm phenomena in the upper atmosphere and ionosphere. Ind. J. Pure Appl. Phys. 9, pp. 542 - 545 (1971)
Chandra, S.; Stubbe, P.: The diurnal phase anomaly in the upper atmospheric density and temperature. Planetary and Space Science 18, pp. 1021 - 1033 (1970)
Stubbe, P.: Simultaneous solution of the time dependent coupled continuity equations, heat conduction equations, and equations of motion for a system consisting of a neutral gas, an electron gas, and a four component ion gas. Journal of Atmospheric and Terrestrial Physics 32, pp. 865 - 903 (1970)
Stubbe, P.; Chandra, S.: The effect of electric fields on the F regin behaviour as compared with neutral wind effects. Planetary and Space Science 32, pp. 1909 - 1919 (1970)
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".