Daehler, M.; Bevilacqua, R. M.; Kriebel-Hamilton, D. L.; Goldizen, D.; Olivero, J. J.; Hartmann, G. K.; Degenhardt, W.; Richards, M. L.; Connor, B. J.; Aellig, C. P.: Validation of Millimeter-wave Atmospheric Sounder (MAS) ozone measurements. Journal Geophysical Research 103, pp. 19615 - 19639 (1998)
Aellig, C. P.; Kämpfer, N.; Rudin, C.; Bevilacqua, R. M.; Degenhardt, W.; Hartogh, P.; Jarchow, C.; Künzi, K.; Olivero, J. J.; Croskey, C.et al.; Waters, J. W.; Michelsen, H. A.: Latitudinal distribution of upper stratospheric ClO as derived from space borne microwave spectroscopy. Geophysical Research Letters 23, pp. 2321 - 2324 (1996)
Hartmann, G. K.; Bevilacqua, R. M.; Schwartz, P. R.; Kämpfer, N.; Künzi, K. F.; Aellig, C. P.; Berg, A.; Boogaerts, W.; Connor, B. J.; Croskey, C. L.et al.; Daehler, M.; Degenhardt, W.; Dicken, H. D.; Goldizen, D.; Kriebel, D.; Langen, J.; Loidl, A.; Olivero, J. J.; Pauls, T. A.; Puliafito, S. E.; Richards, M. L.; Rudin, C.; Tsou, J. J.; Waltman, W. B.; Umlauft, G.; Zwick, R.: Measurements of O3, H2O and ClO in the middle atmosphere using the Millimeter-Wave Atmospheric Sounder (MAS). Geophysical Research Letters 23, pp. 2313 - 2316 (1996)
Hartmann, G. K.; Degenhardt, W.; Richards, M. L.; Liebe, H. J.; Hufford, G. A.; Cotton, M. G.; Bevilacqua, R. M.; Olivero, J. J.; Kämpfer, N.; Langen, J.: Zeeman splitting of the 61 Gigahertz oxygen (O2) line in the mesosphere. Geophysical Research Letters 23, pp. 2329 - 2332 (1996)
Puliafito, E.; Bevilacqua, R.; Olivero, J.; Degenhardt, W.: Retrieval error comparison for several inversion techniques used in limb-scanning millimeter-wave spectroscopy. Journal Geophysical Research 100, p. 14257 (1995)
Hartmann, G. K.; Degenhardt, W.; Zwick, R.; Liebe, H. J.; Hufford, G. A.; Cotton, M. G.: Zeeman splitting of the 61 GHz (9+) O2 line in the upper atmosphere measured by MAS. In: Proc. IGARSS'94 on Surface and Atmospheric Remote Sensing: Technologies, Data Analysis and Interpretation, Pasadena, Vol. III, pp. 1338 - 1340 (Ed. Stein, T. I.). Publ. Services IEEE, Piscataway, N. J. (1994)
Puliafito, E.; Puliafito, C.; Hartmann, G. K.; Degenhardt, W.; Hartogh, P.: Bestimmung des Wasserdampf- und Ozongehaltes der Stratosphäre und Mesosphäre aus radiometrischen Messungen. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany (1989)
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".