Schwenn, R.: Heliospheric 3D structure and CME propagation as seen from SOHO: recent lessons for space weather predictions. Advances in Space Research 26, pp. 43 - 53 (2000)
Schwenn, R.: Coupling betwen high and low latitudes as observed with LASCO in the solar corona and in interplanetary space. Advances in Space Research 26, pp. 771 - 780 (2000)
Srivastava, N.; Schwenn, R.; Inhester, B.; Martin, S. F.; Hanaoka, Y.: Factors related to the origin of a gradual coronal mass ejection associated with an eruptive prominence on 1998 June 21-22. Astrophysical Journal 534, pp. 468 - 481 (2000)
St. Cyr, O. C.; Howard, R. A.; Sheeley Jr., N. R.; Plunkett, S. P.; Michels, D. J.; Paswaters, S. E.; Koomen, M. J.; Simnett, G. M.; Thompson, B. J.; Gurman, J. B.et al.; Schwenn, R.; Webb, D. F.; Hildner, D. F.; Lamy, P. L.: Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998. Journal Geophysical Research 105, pp. 18169 - 18185 (2000)
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. Journal of Atmospheric and Terrestrial Physics 62, pp. 1553 - 1559 (2000)
Funsten, H. O.; Gosling, J. T.; Riley, P.; St. Cyr, O. C.; Forsyth, R. J.; Howard, R. A.; Schwenn, R.: Combined Ulysses solar wind and SOHO coronal observations of several west limb coronal mass ejections. Journal Geophysical Research 104, pp. 6679 - 6689 (1999)
Maia, D.; Vourlidas, A.; Pick, M.; Howard, R.; Schwenn, R.; Magalhaes, A.: Radio signatures of a fast coronal mass ejection development on November 6, 1997. Journal Geophysical Research 104, pp. 12507 - 12513 (1999)
Schwenn, R.; Wilhelm, K.: Die wichtigsten Sonnenmissionen. Beobachtung der Sonne mit Satellitenteleskopen. Sterne unda Weltraum Special 4, p. 110 (1999)
Axford, W. I.; Marsch, E.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T. K.; Schwenn, R.; Ip, W.-H.; Ksanfomality, L. V.; Thomas, N.; Kogan, A.et al.; Utkin, V. F.; Uspensky, G. R.: Space mission for exploration of the Sun, Mercury and inner heliosphere (``InterHelios''). Advances in Space Research 21, pp. 275 - 289 (1998)
Brueckner, G. E.; Delaboudinière, J. P.; Howard, R. A.; Paswaters, S. E.; St. Cyr, O. C.; Schwenn, R.; Lamy, P. L.; Simnett, G. M.; Thompson, B.; Wang, D.: Geomagnetic storms caused by coronal mass ejections (CMEs): March 1996 through June 1997. Geophysical Research Letters 25, pp. 3019 - 3022 (1998)
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Henke, T.; Woch, J.; Mall, U.; Livi, S.; Wilken, B.; Schwenn, R.; Gloeckler, G.; von Steiger, R.; Forsyth, R. J.; Balogh, A.: Differences in the O7+ /O6+ ratio of magnetic cloud and non-cloud coronal mass ejections. Geophysical Research Letters 25, pp. 3465 - 3468 (1998)
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The European Space Agency (ESA) has given the green light to build the flight models of the spacecraft and science payload for the PLATO mission to search for extrasolar planets.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
In the "Solar and Stellar Interiors" department, Laurent Gizon, Jesper Schou, Aaron Birch, Robert Cameron and others offer PhD projects in solar physics and astrophysics. Helioseismology and asteroseismology are used as important tools to study the oscillating Sun and stars.
The longest-serving solar observatory in space has turned 25 and is still making significant contributions to solar research. Its old age has become an important merit.