Feldman, U.; Dammasch, I. E.; Landi, E.; Doschek, G. A.: Observations indicating that ≈ 1 × 107 K solar flare plasmas may be produced in situ from ≈ 1 × 106 K coronal plasma. Astrophysical Journal 609, pp. 439 - 451 (2004)
Dammasch, I. E.; Stellmacher, G.; Wiehr, E.: Spectroscopy of solar prominences from space and ground. Astron. Nachrichten 324 (4), pp. 338 - 339 (2003)
Feldman, U.; Landi, E.; Doschek, G. A.; Dammasch, I. E.; Curdt, W.: Free-free emission in the far-ultraviolet spectral range: A resource for diagnosing solar and stellar flare plasmas. Astrophysical Journal 593, pp. 1226 - 1241 (2003)
Stellmacher, G.; Wiehr, E.; Dammasch, I. E.: Spectroscopy of solar prominences simultaneously from space and ground. Solar Physics 217, pp. 133 - 155 (2003)
Dammasch, I. E.; Wilhelm, K.: SUMER observations of solar transition region structures and dynamics. Advances in Space Research 30 (3), pp. 495 - 500 (2002)
Kliem, B.; Dammasch, I. E.; Curdt, W.; Wilhelm, K.: Correlated dynamics of hot and cool plasmas in the main phase of a solar flare. Astrophysical Journal 568, pp. L61 - L65 (2002)
Wilhelm, K.; Dammasch, I. E.; Hassler, D. M.: Transition region and coronal plamas: Instrumentation and spectral analysis. Astrophysics and Space Science 282, pp. 189 - 207 (2002)
Wilhelm, K.; Dammasch, I. E.; Xia, L.: Observations of ultraviolet emission lines in solar coronal holes on the disk with SUMER on SOHO. Advances in Space Research 30 (3), pp. 517 - 522 (2002)
Feldman, U.; Dammasch, I. E.; Wilhelm, K.: On the unresolved fine structure of the solar atmosphere. IV. The interface with the chromosphere. Astrophysical Journal 558, pp. 423 - 427 (2001)
Moran, T.; Gopalswamy, N.; Dammasch, I. E.; Wilhelm, K.: A multi-wavelength study of solar coronal-hole regions showing radio enhancements. Astronomy and Astrophysics 378, pp. 1037 - 1045 (2001)
Feldman, U.; Dammasch, I. E.; Wilhelm, K.: The morphology of the solar upper atmosphere during the sunspot minimum. Space Science Reviews 93, pp. 411 - 472 (2000)
Wilhelm, K.; Dammasch, I. E.; Marsch, E.; Hassler, D. M.: On the source regions of the fast solar wind in polar coronal holes. Astronomy and Astrophysics 353, pp. 749 - 756 (2000)
Wilhelm, K.; Lemaire, P.; Dammasch, I. E.; Hollandt, J.; Schühle, U.; Curdt, W.; Kucera, T.; Hassler, D. M.; Huber, M. C. E.: Solar irradiances of ultraviolet emission lines measured during the minimum of sunspot activity in 1996 and 1997. Physics and Chemistry of the Earth C, 25, pp. 389 - 392 (2000)
Wilhelm, K.; Schühle, U.; Curdt, W.; Dammasch, I. E.; Hollandt, J.; Lemaire, P.; Huber, M. C. E.: Solar spectroradiometry with the telescope and spectrograph SUMER on the Solar and Heliospheric Observatory SOHO. Metrologia 37, pp. 393 - 398 (2000)
Dammasch, I. E.; Hassler, D. M.; Curdt, W.; Wilhelm, K.: Statistical Analysis of EUV Lines Inside and Outside of Solar Coronal Holes. Space Science Reviews 87, pp. 161 - 164 (1999)
Dammasch, I. E.; Wilhelm, K.; Curdt, W.; Hassler, D. M.: The Ne VIII (λ770) resonance line: Solar wavelengths determined by SUMER on SOHO. Astronomy and Astrophysics 346, pp. 285 - 294 (1999)
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.