Ning, Z.; Innes, D. E.; Solanki, S. K.: Line profile characteristics of solar explosive event bursts. Astronomy and Astrophysics 419, pp. 1141 - 1148 (2004)
Innes, D. E.; McKenzie, D. E.; Wang, T.: Observations of 1000 km s−1 Doppler shift in 107 K solar flare supra-arcade. Solar Physics 217, pp. 267 - 279 (2003)
Landi, E.; Feldman, U.; Innes, D.; Curdt, W.: Mass motions and plasma properties in the 107 K flare solar corona. Astrophysical Journal 582, pp. 506 - 519 (2003)
Innes, D. E.: Coordinated observations of the quiet Sun transition region using SUMER spectra, TRACE images and MDI magnetograms. Astronomy and Astrophysics 378, pp. 1067 - 1077 (2001)
Torsti, J.; Kocharov, L.; Innes, D. E.; Laivola, J.; Sahla, T.: Injection of energetic protons during solar eruption on 1999 May 9: Effect of flare and coronal mass ejection. Astronomy and Astrophysics 365, pp. 198 - 203 (2001)
Brooks, D. H.; Fischbacher, G. A.; Fludra, A.; Harrison, R. A.; Innes, D. E.; Landi, E.; Landini, M.; Lang, J.; Lanzafame, A. C.; Loch, S. D.et al.; McWhirter, R. W. P.; Summers, H. P.: A study of opacity in SOHO-SUMER and SOHO-CDS spectral observations. I. Opacity deduction at the limb. Astronomy and Astrophysics 357, pp. 697 - 715 (2000)
Brooks, D. H.; Fischbacher, G. A.; Fludra, A.; Harrison, R. A.; Innes, D. E.; Landi, E.; Landini, M.; Lang, J.; Lanzafame, A. C.; Loch, S. D.et al.; McWhirter, R. W. P.; Summers, H. P.; Thompson, W. T.: The quiet Sun extreme ultraviolet spectrum observed in normal incidence by the SOHO coronal diagnostic spectrometer. Astronomy and Astrophysics 347, pp. 277 - 312 (1999)
Harrison, R. A.; Lang, J.; Brooks, D. H.; Innes, D. E.: A study of extreme ultraviolet blinker activity. Astronomy and Astrophysics 351, pp. 1115 - 1132 (1999)
Innes, D. E.; Inhester, B.; Srivastava, N.; Brekke, P.; Harrison, R. A.; Matthews, S. A.; Noëns, J. C.; Schmieder, B.; Thompson, B. J.: Multi-wavelength observations of the onset phase of a coronal mass ejection. Solar Physics 186, pp. 337 - 361 (1999)
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".