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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...