Innes, D. E.; Cameron, R. H.; Fletcher, L.; Inhester, B.; Solanki, S. K.: Break up of returning plasma after the 7 June 2011 filament eruption by Rayleigh-Taylor instabilities. Astronomy and Astrophysics 540, L10 (2012)
Tian, H.; McIntosh, S. W.; Wang, T.; Ofman, L.; De Pontieu, B.; Innes, D. E.; Peter, H.: Persistent Doppler Shift Oscillations Observed with Hinode/EIS in the Solar Corona: Spectroscopic Signatures of Alfvénic Waves and Recurring Upflows. Astrophysical Journal 759, 144 (2012)
Innes, D. E.; Cameron, R. H.; Solanki, S. K.: EUV Jets, Type III Radio Bursts and Sunspot Waves Investigated Using SDO/AIA Observations. Astronomy and Astrophysics 531, L13 (2011)
Kamio, S.; Curdt, W.; Teriaca, L.; Innes, D. E.: Evolution of microflares associated with bright points in coronal holes and in quiet regions. Astronomy and Astrophysics 529, A21 (2011)
Matthews, S. A.; Williams, D. R.; Klein, K.-L.; Kontar, E. P.; Smith, D. M.; Lagg, A.; Krucker, S.; Hurford, G. J.; Vilmer, N.; MacKinnon, A. L.et al.; Zharkova, V. V.; Fletcher, L.; Hannah, I. G.; Browning, P. K.; Innes, D. E.; Trottet, G.; Foullon, C.; Nakariakov, V. M.; Green, L. M.; Lamoureux, H.; Forsyth, C.; Walton, D. M.; Mathioudakis, M.; Gandorfer, A.; Martinez-Pillet, V.; Limousin, O.; Verwichte, E.; Dalla, S.; Mann, G.; Aurass, H.; Neukirch, T.: Solar Particle Acceleration Radiation and Kinetics (SPARK). Experimental Astronomy 33, pp. 237 - 269 (2011)
Innes, D. E.; McIntosh, S. W.; Pietarila, A.: STEREO quadrature observations of coronal dimming at the onset of mini-CMEs. Astronomy and Astrophysics 517, L7 (2010)
McIntosh, S. W.; Innes, D. E.; De Pontieu, B.; Leamon, R. J.: STEREO observations of quasi-periodically driven high velocity outflows in polar plumes. Astronomy and Astrophysics 510, L2 (2010)
Attie, R.; Innes, D. E.; Potts, H. E.: Evidence of photospheric vortex flows at supergranular junctions observed by FG/SOT (Hinode). Astronomy and Astrophysics 493 (2), pp. L13 - L16 (2009)
Innes, D. E.; Genetelli, A.; Attie, R.; Potts, H. E.: Quiet Sun mini-coronal mass ejections activated by supergranular flows. Astronomy and Astrophysics 495, p. 319 (2009)
Bazarghan, M.; Safari, H.; Innes, D. E.; Karami, E.; Solanki, S. K.: A nanoflare model for active region radiance: application of artificial neural networks. Astronomy and Astrophysics 492, pp. L13 - L16 (2008)
Chen, P. F.; Innes, D. E.; Solanki, S. K.: SOHO/SUMER observations of prominence oscillation before eruption. Astronomy and Astrophysics 484, pp. 487 - 493 (2008)
Innes, D. E.; Attie, R.; Hara, H.; Madjarska, M. S.: EIS/ Hinode Observations of Doppler Flow Seen through the 40-Arcsec Wide-Slit. Solar Physics 252, pp. 283 - 292 (2008)
Madjarska, M. S.; Doyle, J. G.; Innes, D. E.; Curdt, W.: Jets or High-Velocity Flows Revealed in High-Cadence Spectrometer and Imager Co-observations? Astrophysical Journal 670, pp. L57 - L60 (2007)
Wang, T. J.; Innes, D. E.; Qiu, J.: Determination of the coronal magnetic field from hot-loop oscillations observed by SUMER and SXT. Astrophysical Journal 656 (1), pp. 598 - 609 (2007)
Wang, T. J.; Innes, D. E.; Solanki, S. K.: Fe XIX observations of active region brightenings in the corona. Astronomy and Astrophysics 455, pp. 1105 - 1113 (2006)
Bewsher, D.; Innes, D. E.; Parnell, C. E.; Brown, D. S.: Comparison of blinkers and explosive events: A case study. Astronomy and Astrophysics 432, pp. 307 - 317 (2005)
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.