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Borchers, R.; Harnisch, J.; Kourtidis, K.: Results of SESAME Cryosampler Flight on March 7, 1995. In: Polar Stratospheric Ozone, Proc. 3rd European Workshop, Schliersee 1995, Air Pollution Research Report 56, pp. 80 - 83 (Eds. Pyle, J. A.; Harris, N. R. P.; Amanatidis, G. T.). European Commission, Luxembourg (1996)
Harnisch, J.: Emission scenarios for CF4 and C2F6 based on reconstructed atmospheric concentrations. In: Proc. Workshop ``Successful Partnership to Reduce PFC Emissions from Primary Aluminium Production'', p. 13. United States Environmental Protectection Agency, Washington DC (1996)
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Harnisch, J.; Sue Wing, I.; Jacoby, H. D.; Prinn, R. G.: Primary Aluminum Production: Climate Policy, Emissions and Costs. Massachusetts Institute of Technology, Cambridge, MA, USA (1998)
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".