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Srivastava, N.; Schwenn, R.; Inhester, B.; Stenborg, G.; Podlipnik, B.: Measurements of flow speeds and acceleration in gradually evolving solar mass ejections as observed by LASCO. In: Proc. 9th Int. Solar Wind Conf. ``Solar Wind Nine'', Nantucket, MA, USA, 5-9 October 1998, pp. 115 - 118 (Eds. Habbal, S. R.; Esser, R.; Hollweg, J. V.; Isenberg, P. A.). The American Institute of Physics, Woodbury, NY, USA (1999)
Srivastava, N.; Schwenn, R.; Stenborg, G.: Comparative study of coronal mass ejections associated with eruptive prominences. In: Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999, pp. 621 - 626 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Stenborg, G.; Bagalá, L. G.; Bauer, O. H.; Fernández Borda, R.; Francile, C.; Haerendel, G.; Rovira, M. G.; Schwenn, R.: First combined observations in the German-Argentinean solar observatory: Correlations in quiet and eruptive phenomena at the limb. In: IAGA Conference, Birmingham, August 1999. (1999)
Stenborg, G.; Schwenn, R.; Inhester, B.; Srivastava, N.: On the rotation rate of the emission solar corona. In: Proc. 9th European Meeting on Solar Physics: Magnetic Fields and Solar Processes, Florence, Italy, 12-18 September 1999, pp. 1107 - 1113 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1999)
Stenborg, G.; Schwenn, R.; Srivastava, N.: MICA observations of coronal transients. In: Proc. 8th SOHO Workshop `Plasma Dynamics and Diagnostics in the Solar Transition Region and Corona', Paris, France, 22-25 June 1999, pp. 627 - 632 (Eds. Vial, J.-C.; Kaldeich-Schürmann, B.). ESA Publ. Div., Noordwijk (1999)
Stenborg, G.; Schwenn, R.; Srivastava, N.; Inhester, B.; Podlipnik, B.; Rovira, M.; Francile, C.: Recent observations of the solar corona with a new ground-based coronagraph in Argentina (MICA). In: Proc. 9th Int. Solar Wind Conf. ``Solar Wind Nine'', Nantucket, MA, USA, 5-9 October 1998, pp. 561 - 564 (Eds. Habbal, S. R.; Esser, R.; Hollweg, J. V.; Isenberg, P. A.). The American Institute of Physics, Woodbury, NY, USA (1999)
Andrews, M. D.; Morrill, J. S.; Howard, R. A.; Biesecker, D. A.; Schwenn, R.; Llebaria, A.: The dynamics of the quiet corona as observed by the LASCO C2 and C3 coronagraphs. In: Proc. 31st ESLAB Symp. ``Correlated Phenomena at the Sun, in the Heliosphere and in Geospace'', ESTEC, pp. 303 - 305 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
Boulade, S.; Delannée, C.; Koutchmy, S.; Lamy, P.; Llebaria, A.; Howard, R.; Schwenn, R.; Simnett, G.: Analysis of a high latitude slow CME with travelling ejecta. In: ``The Corona and Solar Wind Near Minimum Activity'',, pp. 217 - 221 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
Crosby, N.; Vilmer, N.; Drago, F. C.; Pick, M.; Kerdraon, A.; Khan, J.; Schwenn, R.: Non-thermal weak radio bursts: X-ray and/or EUV counterparts? In: Proc. Fifth SOHO Workshop ``The Corona and Solar Wind Near Minimum Activity'', Oslo, pp. 299 - 301 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
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Klein, K.-L.; Klassen, A.; Aurass, H.; Schwenn, R.; the LASCO Team: On the propagation of a large-scale shock wave in the corona. In: Proc. Fifth SOHO Workshop ``The Corona and Solar Wind Near Minimum Activity'', Oslo, pp. 461 - 464 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
Lamy, P.; Llebaria, A.; Koutchmy, S.; Reynet, P.; Molodensky, M.; Howard, R.; Schwenn, R.; Simmnet, G.: Characterization of polar plumes from LASCO-C2 images in early 1996. In: Proc. Fifth SOHO Wokshop ``The Corona and Solar Wind Near Minimum Activity'', pp. 487 - 490 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
Lamy, P.; Quemerais, E.; Llebaria, A.; Bout, M.; Howard, R.; Schwenn, R.; Simmnet, G.: Electronic densities in coronal holes from LASCO-C2 images. In: Proc. Fifth SOHO Wokshop ``The Corona and Solar Wind Near Minimum Activity'', pp. 491 - 494 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
Michels, D. J.; Howard, R. A.; Koomen, M. J.; Plunkett, S.; Brueckner, G. E.; Lamy, P.; Schwenn, R.; Biesecker, D. A.: Visibility of earth-directed coronal mass ejections. In: Proc. Fifth SOHO Workshop ``The Corona and Solar Wind Near Minimum Activity'', Oslo, pp. 567 - 570 (Ed. Wilson, A.). ESA Publ. Div., Noordwijk (1997)
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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".