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Watermann, J.; Stauning, P.; Luehr, H.; Newell, P. T.; Christiansen, F.; Schlegel, K.: Are small-scale field-aligned currents and magneto sheath-like particle precipitation signatures of the same low-altitude cusp? Advances in Space Research 43 (1), pp. 41 - 46 (2009)
Cai, H. T.; Ma, S. Y.; Fan, Y.; Liu, Y. C.; Schlegel, K.: Climatological features of electron density in the polar ionosphere from long-term observations of EISCAT/ESR radar. Annales Geophysicae 25, pp. 2561 - 2569 (2007)
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Cai, H. T.; Ma, S. Y.; Schlegel, K.: Climatologic characteristics of high-latitude ionosphere - EISCAT observations and comparison with the IRI model. Chinese J. Geophys. 48 (3), pp. 471 - 479 (2005)
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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".