Bischof, W.; Borchers, R.; Fabian, P.; Krüger, B. C.: Increased concentration and vertical distribution of carbon dioxide in the stratosphere. Nature 316, pp. 135 - 136 (1985)
Fabian, P.; Borchers, R.; Krüger, B. C.; Lal, S.: The vertical distribution of CHCLF2 (CFC-22) in the stratosphere. Geophysical Research Letters 12, pp. 1 - 3 (1985)
Fabian, P.; Borchers, R.; Krüger, B. C.; Lal, S.: The vertical distribution of CFC-114 in the atmosphere. Journal Geophysical Research 90, pp. 13091 - 13093 (1985)
Fabian, P.; Borchers, R.; Gömer, D.; Penkett, S. A.: Vertical profiles of halocarbons in the stratosphere. Advances in Space Research 4, pp. 135 - 138 (1984)
Schmidt, M.; Borchers, R.; Fabian, P.; Flentje, G.; Matthews, W. A.; Szabo, A.; Lal, S.: Trace gas measurements during aircraft flights in the tropopause region over Europe and North Africa. J. Atmos. Chem. 2, pp. 133 - 143 (1984)
Borchers, R.; Fabian, P.; Penkett, S. A.: First measurements of the vertical distribution of CCl4 and CH3CCl3 in the stratosphere. Naturwissenschaften 10, pp. 14 - 16 (1983)
Fabian, P.; Borchers, R.; Weiler, K. H.; Schmidt, U.; Volz, A.; Ehhalt, D. H.; Seiler, W.; Müller, F.: Simultaneously measured vertical profiles of H2, CH4, CO, N2O, CFCl3 and CF2Cl2 in the midlatitude stratosphere and troposphere. Journal Geophysical Research 84, pp. 3149 - 3154 (1979)
Widdel, H. U.; Rose, G.; Borchers, R.: Results of conductivity, ion mobility and ion concentration measurements obtained with a parachutet Gerdien aspiration analyses probe in heights below 70 km. Journal of Atmospheric and Terrestrial Physics 41, pp. 1141 - 1147 (1979)
Widdel, H. U.; Rose, G.; Borchers, R.: Payload BIII - an instrument package for the measurement of conductivity, concentration an mobility of positive and negative ions in the meosphere. J. Geophys. 44, pp. 179 - 188 (1977)
Widdel, H. U.; Rose, G.; Borchers, R.: Experimental results on the variation of electric conductivity an ion mobility in the mesosphere. Journal Geophysical Research 81, pp. 6217 - 6220 (1976)
Borchers, R.; Rose, G.; Widdel, H. U.: Ergebnisse von Ionendichte- und Ionenbeweglichkeitsmessungen mit einer Fallschirmsonde im Höhenbereich von 72 bis 39 km. Kleinheubacher Berichte 14, pp. 255 - 262 (1971)
Rose, G.; Widdel, H. U.; Borchers, R.: A mesosphere payload to measure the concentration and mobility of positive and negative ions in the height range between 72 and 40 km. J. Brit. Interpl. Soc. 24, pp. 215 - 231 (1971)
Widdel, H. U.; Rose, G.; Borchers, R.: Results of concentration and mobility measurements of positively and negatively charged particles taken by a rocket-borne parachutet aspiration (Gerdien) probe in the height region from 72 to 39 km. Pageoph 84, pp. 154 - 160 (1971)
Borchers, R.; Harnisch, J.: Individual contribution of participant no. In: ``The partitioning of ClOy in the stratosphere'', Final report to the European Commission on CEC Contract EV5V-CT93-0346, pp. 93 - 115 (Ed. Camy-Peyret, C.). European Commission, Paris (1996)
Widdel, H. U.; Rose, G.; Borchers, R.: Results of conductivity, ion mobility and ion concentration measurements taken with a parachute Gerdien Kondensor experiment during the winter anomaly campaign. In: COSPAR Space Res., pp. 125 - 127 (Eds. Rycroft, M. J.; Stickland, A. C.). Pergamon Press Oxford (1978)
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.