Mecheri, R.; Marsch, E.: Ray tracing of ion-cyclotron waves in a coronal funnel. In: Modern Solar Facilities-Advanced Solar Science, S. 355 - 358 (Hg. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen (2007)
Teriaca, L.; Schühle, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The Lower Transition Region As Seen In The H I Lyman-alpha Line. In: The Second Solar Orbiter Workshop, 16-20 October 2006, Athens, Greece (Hg. Marsch, E.; Tsinganos, K.; Marsden, R.; Conroy, L.). ESA Publ. Div., Noordwijk (2007)
Marsch, E.: Origin and evolution of the solar wind. In: Solar Activity and its Magnetic Origin, Proceedings of the International Astronomical Union, Symposium S233, S. 259 - 268 (Hg. Bothmer, V.; Hady, A.). Cambridge University Press, Cambridge, U.K. (2006)
Marsch, E.: Coronal origins of the solar wind - sources of steady streams and transient flows caused by solar magnetic eruptions. In: Solar Influence on the Heliosphere and Earth's Environment: Recent Progress and Prospects, S. 111 - 118 (Hg. Gopalswamy, N.; Bhattacharyya, A.). Quest Publications for ILWS and Indian Institute of Geomagnetism (2006)
Marsch, E.; Zhou, G.-Q.; He, J.-S.; Tu, C.-Y.: On the structure of the solar transition region. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Matteini, L.; Landi, S.; Hellinger, P.; Velli, M.; Maksimovic, M.; Pantellini, F.; Marsch, E.: On the role of the parallel proton fire hose instability in the expanding solar wind: Simulations and observations. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Mecheri, R.; Marsch, E.: Drift-instabilities in a coronal funnel within the multi-fluid description. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Solanki, S. K.; Marsch, E.: Solar microscopy: unveiling the Sun's basic physical processes at their intrinsic scales. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Teriaca, L.; Schühle, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The dynamic nature of the solar transition region as revealed by spectroscopy of the hydrogen Lyman-alpha line. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Tu, C.-Y.; He, J.-S.; Marsch, E.: Plasma Outflows and Open Magnetic Fields in a Quiet-Sun Region. In: Proceedings of SOHO 17 - 10 Years of SOHO and Beyond, 7-12 May 2006, Giardini Naxos, Sicily, Italy (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2006)
Marsch, E.: Importance of kinetic effects in heating the open and closed corona. In: Proceedings of the Solar Wind 11/SOHO 16 Conference, 12-17 June 2005, Whistler, Canada, S. 191 - 198 (Hg. Fleck, B.; Zurbuchen, T. H.). ESA Publ. Div., Noordwijk (2005)
Mecheri, R.; Marsch, E.: Beam-instabilities in a coronal funnel within the multi-fluid description. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Hg. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Teriaca, L.; Schühl{}e, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The structure of the lower transition region as inferred from the hydrogen Lyman-α line radiance. In: Proceedings of the International Scientific Conference on Chromospheric and Coronal Magnetic Fields (Hg. Innes, D. E.; Lagg, A.; Solanki, S. K.; Danesy, D.). ESA Publ. Div., Noordwijk (2005)
Teriaca, L.; Schühle, U.; Solanki, S. K.; Curdt, W.; Marsch, E.: The dynamics of the lower transition region as inferred from the hydrogen Lyman-α line radiance. In: Proceedings of the 11th European Solar Physics Meeting - The Dynamic Sun: Challenges for Theory and Observations, 11-16 September 2005 (Hg. Danesy, D.; Poedts, S.; De Groof, A.; Andries, J.). ESA Publ. Div., Noordwijk (2005)
Tu, C.-Y.; Zhou, C.; Marsch, E.; Wilhelm, K.; Xia, L.-D.; Zhao, L.; Wang, J.-X.: The height of solar wind origin in coronal funnels and a 3-D scenario for solar wind formation. In: Proceedings of the Solar Wind 11/SOHO 16 Conference, 12-17 June 2005, Whistler, Canada, S. 131 - 134 (Hg. Fleck, B.; Zurbuchen, T. H.). ESA Publ. Div., Noordwijk (2005)
Marsch, E.: Waves in the solar corona. In: Stars as Suns: Activity, Evolution and Planets, S. 449 - 460 (Hg. Dupree, A. K.; Benz, A. O.). Astronomical Society of the Pacific, USA (2004)
Xia, L. D.; Marsch, E.: Observational constraints on ion acceleration by waves in coronal holes. In: Proc. of SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE, S. 387 - 390 (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Xia, L. D.; Marsch, E.; Wilhelm, K.: Topological changes of the magnetic network as seen in different UV/EUV emission lines. In: Proc. of SOHO 13 - Waves, Oscillations and Small-Scale Transient Events in the Solar Atmosphere: A Joint View from SOHO and TRACE, S. 169 - 174 (Hg. Lacoste, H.). ESA Publ. Div., Noordwijk (2004)
Marsch, E.: The microscopic state of the solar wind. In: Solar Wind Ten: Proceedings of the Tenth International Solar Wind Conference, S. 399 - 404 (Hg. Velli, M.; Bruno, R.; Malara, F.). American Institute of Physics (2003)
Sichtung von Bewerbungen an mehreren Terminen pro Jahr. Promotionsprojekte in Planetenwissenschaften, Sonnensytemforschung, Kosmochemie, Exoplaneten, Sonnenphysik, stellare Astrophysik, Magnetfelder der Sonne, Helioseismologie, Asteroseismologie ...
Als erste Raumsonde schaut Solar Orbiter auf die Pole der Sonne – und findet das Magnetfeld dort im Ausnahmezustand. Aktuell polt sich das Magnetfeld der Sonne um.
First Light! Das Spektro-Polarimeter des weltweit größten Sonnenteleskops auf Hawaii schaut erstmals auf die Sonne. Das Instrument wurde in Deutschland entwickelt.
Wenige Monate nach Inbetriebnahme hat die Raumsonde einen Strahlungsausbruch auf der Sonne beobachtet – und in eine kaum erforschte Schicht unseres Sterns geschaut.
Dr. Theodosios Chatzistergos blickt in die Vergangenheit unseres Sterns und wertet historische Sonnenbeobachtungen aus. Nun erhält er eine wichtige Auszeichnung.