Park, J.; Innes, D. E.; Bučík, R.; Moon, Y.-J.; Kahler, S. W.: Study of solar energetic particle associations with coronal extreme-ultraviolet waves. Astrophysical Journal 808 (1), 3 (2015)
Price, D. J.; Taroyan, Y.; Innes, D. E.; Bradshaw, S. J.: Forward Modelling of a Brightening Observed by AIA. Solar Physics 290, pp. 1931 - 1945 (2015)
Bučík, R.; Innes, D. E.; Mall, U.; Korth, A.; Mason, G. M.; Gomez-Herrero, R.: Multi-spacecraft observations of recurrent 3He-rich solar energetic particles. Astrophysical Journal 786 (1), 71 (2014)
Carlyle, J.; Williams, D. R.; van Driel-Gesztelyi, L.; Innes, D.; Hillier, A.; Matthews, S.: Investigating the Dynamics and Density Evolution of Returning Plasma Blobs from the 2011 June 7 Eruption. Astrophysical Journal 782 (2), 87 (2014)
Guo, L.-J.; Huang, Y.-M.; Bhattacharjee, A.; Innes, D. E.: Rayleigh-Taylor Type Instabilities in the Reconnection Exhaust Jet as a Mechanism for Supra-Arcade Downflows in the Sun. Astrophysical Journal 796 (2), L29 (2014)
Innes, D. E.; Guo, L.-J.; Bhattacharjee, A.; Huang, Y.-M.; Schmit, D.: Observations of Supra-Arcade Fans: Instabilities at the Head of Reconnection Jets. Astrophysical Journal 796 (1), 27 (2014)
Chen, N.; Ip, W.-H.; Innes, D.: Flare-Associated Type III Radio Bursts and Dynamics of the EUV Jet from Sdo/Aia and Rhessi Observations. Astrophysical Journal 769 (2), 96 (2013)
Fletcher, L.; Hannah, I. G.; Hudson, H. S.; Innes, D. E.: Flare Ribbon Energetics in the Early Phase of an SDO Flare. Astrophysical Journal 771 (2), 104 (2013)
Kumar, P.; Innes, D. E.: Multiwavelength Observations of an Eruptive Flare: Evidence for Blast Waves and Break-Out. Solar Physics 288 (1), pp. 255 - 268 (2013)
Kumar, P.; Innes, D. E.; Inhester, B.: Solar Dynamics Observatory/Atmospheric Imaging Assembly Observations of a Reflecting Longitudinal Wave in a Coronal Loop. Astrophysical Journal 779 (1), L7 (2013)
Lee, K. S.; Innes, D. E.; Moon, Y. J.; Shibata, K.; Lee, J. Y.; Park, Y. D.: Fast extreme-ultraviolet dimming associated with a coronal jet seen in multi-wavelength and stereoscopic observations. Astrophysical Journal 766, pp. 1 - 12 (2013)
Park, J.; Innes, D. E.; Bučík, R.; Moon, Y.-J.: The source regions of solar energetic particles detected by widely separated spacecraft. Astrophysical Journal 779 (2), 184 (2013)
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".