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)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.